Clotting factors and their encoding genes.
\\n\\n
IntechOpen Book Series will also publish a program of research-driven Thematic Edited Volumes that focus on specific areas and allow for a more in-depth overview of a particular subject.
\\n\\nIntechOpen Book Series will be launching regularly to offer our authors and editors exciting opportunities to publish their research Open Access. We will begin by relaunching some of our existing Book Series in this innovative book format, and will expand in 2022 into rapidly growing research fields that are driving and advancing society.
\\n\\nLaunching 2021
\\n\\nArtificial Intelligence, ISSN 2633-1403
\\n\\nVeterinary Medicine and Science, ISSN 2632-0517
\\n\\nBiochemistry, ISSN 2632-0983
\\n\\nBiomedical Engineering, ISSN 2631-5343
\\n\\nInfectious Diseases, ISSN 2631-6188
\\n\\nPhysiology (Coming Soon)
\\n\\nDentistry (Coming Soon)
\\n\\nWe invite you to explore our IntechOpen Book Series, find the right publishing program for you and reach your desired audience in record time.
\\n\\nNote: Edited in October 2021
\\n"}]',published:!0,mainMedia:{caption:"",originalUrl:"/media/original/132"}},components:[{type:"htmlEditorComponent",content:'With the desire to make book publishing more relevant for the digital age and offer innovative Open Access publishing options, we are thrilled to announce the launch of our new publishing format: IntechOpen Book Series.
\n\nDesigned to cover fast-moving research fields in rapidly expanding areas, our Book Series feature a Topic structure allowing us to present the most relevant sub-disciplines. Book Series are headed by Series Editors, and a team of Topic Editors supported by international Editorial Board members. Topics are always open for submissions, with an Annual Volume published each calendar year.
\n\nAfter a robust peer-review process, accepted works are published quickly, thanks to Online First, ensuring research is made available to the scientific community without delay.
\n\nOur innovative Book Series format brings you:
\n\nIntechOpen Book Series will also publish a program of research-driven Thematic Edited Volumes that focus on specific areas and allow for a more in-depth overview of a particular subject.
\n\nIntechOpen Book Series will be launching regularly to offer our authors and editors exciting opportunities to publish their research Open Access. We will begin by relaunching some of our existing Book Series in this innovative book format, and will expand in 2022 into rapidly growing research fields that are driving and advancing society.
\n\nLaunching 2021
\n\nArtificial Intelligence, ISSN 2633-1403
\n\nVeterinary Medicine and Science, ISSN 2632-0517
\n\nBiochemistry, ISSN 2632-0983
\n\nBiomedical Engineering, ISSN 2631-5343
\n\nInfectious Diseases, ISSN 2631-6188
\n\nPhysiology (Coming Soon)
\n\nDentistry (Coming Soon)
\n\nWe invite you to explore our IntechOpen Book Series, find the right publishing program for you and reach your desired audience in record time.
\n\nNote: Edited in October 2021
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Evolutionary robotics is a new method for the automatic creation of autonomous robots. When executing tasks by autonomous robots, we can make the robot learn what to do so as to complete the task from interactions with its environment, but not manually pre-program for all situations. Many researchers have been studying the techniques for evolutionary robotics by using Evolutionary Computation (EC), such as Genetic Algorithms (GA) or Genetic Programming (GP). Their goal is to clarify the applicability of the evolutionary approach to the real-robot learning, especially, in view of the adaptive robot behavior as well as the robustness to noisy and dynamic environments. For this purpose, authors in this book explain a variety of real robots in different fields.\r\nFor instance, in a multi-robot system, several robots simultaneously work to achieve a common goal via interaction; their behaviors can only emerge as a result of evolution and interaction. How to learn such behaviors is a central issue of Distributed Artificial Intelligence (DAI), which has recently attracted much attention. This book addresses the issue in the context of a multi-robot system, in which multiple robots are evolved using EC to solve a cooperative task. Since directly using EC to generate a program of complex behaviors is often very difficult, a number of extensions to basic EC are proposed in this book so as to solve these control problems of the robot.",isbn:null,printIsbn:"978-3-902613-19-6",pdfIsbn:"978-953-51-5829-5",doi:"10.5772/62",price:159,priceEur:175,priceUsd:205,slug:"frontiers_in_evolutionary_robotics",numberOfPages:598,isOpenForSubmission:!1,isInWos:1,isInBkci:!1,hash:null,bookSignature:"Hitoshi Iba",publishedDate:"April 1st 2008",coverURL:"https://cdn.intechopen.com/books/images_new/3600.jpg",numberOfDownloads:74138,numberOfWosCitations:54,numberOfCrossrefCitations:19,numberOfCrossrefCitationsByBook:4,numberOfDimensionsCitations:76,numberOfDimensionsCitationsByBook:4,hasAltmetrics:0,numberOfTotalCitations:149,isAvailableForWebshopOrdering:!0,dateEndFirstStepPublish:null,dateEndSecondStepPublish:null,dateEndThirdStepPublish:null,dateEndFourthStepPublish:null,dateEndFifthStepPublish:null,currentStepOfPublishingProcess:1,indexedIn:"1,2,3,4,5,6,7",editedByType:"Edited by",kuFlag:!1,featuredMarkup:null,editors:[{id:"123552",title:"Prof.",name:"Hitoshi",middleName:null,surname:"Iba",slug:"hitoshi-iba",fullName:"Hitoshi Iba",profilePictureURL:"//cdnintech.com/web/frontend/www/assets/author.svg",biography:null,institutionString:null,position:null,outsideEditionCount:0,totalCites:0,totalAuthoredChapters:"0",totalChapterViews:"0",totalEditedBooks:"1",institution:{name:"University of Tokyo",institutionURL:null,country:{name:"Japan"}}}],equalEditorOne:null,equalEditorTwo:null,equalEditorThree:null,coeditorOne:null,coeditorTwo:null,coeditorThree:null,coeditorFour:null,coeditorFive:null,topics:[{id:"1283",title:"Autonomous Robot",slug:"evolutionary-robotics-autonomous-robot"}],chapters:[{id:"843",title:"A Comparative Evaluation of Methods for Evolving a Cooperative Team",doi:"10.5772/5445",slug:"a_comparative_evaluation_of_methods_for_evolving_a_cooperative_team",totalDownloads:2066,totalCrossrefCites:0,totalDimensionsCites:0,hasAltmetrics:0,abstract:null,signatures:"Takaya Arita and Yasuyuki Suzuki",downloadPdfUrl:"/chapter/pdf-download/843",previewPdfUrl:"/chapter/pdf-preview/843",authors:[null],corrections:null},{id:"844",title:"An Adaptive Penalty Method for Genetic Algorithms in Constrained Optimization Problems",doi:"10.5772/5446",slug:"an_adaptive_penalty_method_for_genetic_algorithms_in_constrained_optimization_problems",totalDownloads:4056,totalCrossrefCites:6,totalDimensionsCites:41,hasAltmetrics:0,abstract:null,signatures:"Helio J. 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From chapter submission and review, to approval and revision, copyediting and design, until final publication, I work closely with authors and editors to ensure a simple and easy publishing process. I maintain constant and effective communication with authors, editors and reviewers, which allows for a level of personal support that enables contributors to fully commit and concentrate on the chapters they are writing, editing, or reviewing. I assist authors in the preparation of their full chapter submissions and track important deadlines and ensure they are met. I help to coordinate internal processes such as linguistic review, and monitor the technical aspects of the process. As an ASM I am also involved in the acquisition of editors. 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Venkateswarlu",coverURL:"https://cdn.intechopen.com/books/images_new/371.jpg",editedByType:"Edited by",editors:[{id:"58592",title:"Dr.",name:"Arun",surname:"Shanker",slug:"arun-shanker",fullName:"Arun Shanker"}],productType:{id:"1",chapterContentType:"chapter",authoredCaption:"Edited by"}}]},chapter:{item:{type:"chapter",id:"77598",title:"Thrombosis-Related DNA Polymorphisms",doi:"10.5772/intechopen.98728",slug:"thrombosis-related-dna-polymorphisms",body:'Thrombotic disorders and their related diseases, particularly cardiovascular diseases, are among the most common causes of morbidity and mortality in the world, causing a heavy burden on public health.
At the era of precision medicine ecosystem, omics technologies are increasingly being used to provide new molecular taxonomy of diseases and more precise approaches to assess risks, to predict and diagnose, and to monitor prognosis, therapeutic management and progression of these diseases.
During the genomic and the post-genomic phases and after the success of the Human Genome project, many genetic markers of complex common multifactorial diseases, in particular thrombosis and cardiovascular diseases have been tested using genetic association studies.
Multiple single and combined genetic variations and polymorphisms especially in the genes of coagulation and hemostasis pathways, as well as in the genes of inflammation and other genes interacting with lifestyle and environmental factors such as immune and oxidative systems were considered.
However, some of those variants remain under debate and clinical genotype–phenotype correlations continue to be uncertain.
To provide an overview of thrombosis-related DNA polymorphisms, we reviewed thrombosis related mechanisms as well as genetic variants associated with arterial and venous thrombosis and embolism and their clinical manifestations.
Classical polymorphisms in the hemostasis and coagulation pathways factors are reported in this first chapter. Besides, other types of genetic polymorphisms and variants having an impact on the susceptibility to venous and arterial thrombotic disease will be documented in a second future part.
Thrombosis is defined as the formation, development, or presence of a blood clot, known as a thrombus, within a blood vessel that may be either a vein or an artery. The prefix “thrombo” come from the Greek “thrombos” meaning a lump or clump.
When thrombosis detaches and travels through blood vessels to another part of the body, it becomes an embolism.
Thrombosis has catastrophic complications by obstructing blood flow leading to ischemia and even infarction of the tissues supplied by the occluded blood vessels.
Embolism is often considered more dangerous than thrombosis because of its predilection to obstruct the entire blood vessel.
Usually, thrombotic diseases are classified according to their occurrence in the venous system of low flow and pressure or in the arterial system of high-flow and pressure.
Venous and arterial thrombotic disorders have long been viewed as separate pathophysiological entities partly because of the recognizable anatomical differences, despite the idea of a common pathogenesis of all thrombosis which is fundamentally the disturbance of hemostasis [1].
In fact, arterial thrombosis has long been apprehended to be a phenomenon of platelet activation, whereas venous thrombosis has been mainly held to be secondary to the activation of the clotting system [1].
Differences observed in the composition of the thrombi, which are platelet rich thrombi in arterial thrombosis and fibrin rich thrombi in venous thrombosis, and the presence of vascular wall damage in particular atheroma in arterial thrombosis reinforced this dichotomy in the concepts of arterial vs. venous thrombosis [2].
Arterial thrombosis involves the formation of white platelet-rich thrombi that occurs after the rupture of atherosclerotic plaques and the exposure of procoagulant material such as lipid-rich macrophages, collagen, tissue factor and/or endothelial breach, in a high shear environment [3].
In contrast, venous thrombosis is usually associated with plasma hypercoagulability and activation of the clotting system with expression of procoagulant factors on an intact endothelium. This activation is the result of the inflammatory process associated or not to a reduced blood flow or a stasis subsequent to prolonged immobility [1].
Actually, the distinctions are not absolute, and there are many evidences that arterial and venous thrombosis have many common underlying mechanisms involving biological factors either responsible for activating coagulation or inflammatory pathways in both the arterial and the venous systems [4].
Moreover, it was shown that patients with venous thromboembolism are at a higher risk of arterial thrombotic complications than matched control individual supporting the interplay between venous and arterial thrombosis pathogenesis [5].
Arterial and venous thrombosis and embolism are associated to a variety of diseases and clinical manifestations such as systemic arterial thrombosis or embolism, ischemic strokes and acute infarction as well as superficial vein thrombosis and acute peripheral venous phlebitis, deep vein thrombosis and acute pulmonary embolism [6]. Obstetrical and placental thrombosis is another clinical presentation of thrombotic disease.
The definition of the term coagulopathies is controversial. They are various conditions in which the aptitude of blood to clot is impaired. However, the term of coagulopathies is used by many health-professionals to design thrombotic states and disorders of coagulation [7].
The definition of the term thrombophilia is more consensual and refers to inherited defects leading to enhanced coagulation, especially of the venous system. On the other hand and for many authors, thrombophilia may be, inherited or acquired, and the hypercoagulability state may arise from an excess or hyperfunction of a procoagulant or a deficiency of an anticoagulant factor [8].
Microvascular thrombosis is defined by the occurrence of microthrombi within the microcirculation. This microthrombogenesis process is associated to various severe clinical diseases such as thrombotic thrombocytopenic purpura, disseminated intravascular coagulation, and antiphospholipid syndrome as well as other thrombotic microangiopathies. It is also observed during systemic infections, cancer, myocardial infarction, stroke and neurodegenerative diseases [9].
Microvascular thrombosis often occurs subsequently to disordered clot formation and disordered inflammation pathway. Recently, during the coronavirus pandemic, it was shown that the novel severe acute respiratory syndrome coronavirus 2, is characterized by a dysregulated immune system and hypercoagulability recognized on the basis of profound d-dimer elevations and evidence of microthrombi and macrothrombi, both in venous and arterial systems. The complex crosstalking between the innate immune system and coagulation pathways culminates in the model of immunothrombosis, ultimately causing microthrombotic complications [9]. Microvessel thrombosis can then cause greatly differing symptoms that range from limited changes in plasma coagulation markers to severe multi-organ failure. Immunothrombosis is critically supported by neutrophil elastase and the activator molecules of blood coagulation tissue factor and factor XII. Identification of the biological driving forces of microvascular thrombosis should help to elucidate the mechanisms promoting pathological vessel occlusions in both microvessels and large vessels [10].
Thrombosis is a pathologic phenomenon related to the disturbance of the dynamic balance of hemostasis. In fact, under normal circumstances, there is a fine balance between the procoagulant, anticoagulant and fibrinolytic pathways.
Hemostasis is the physiological mechanism aiming to protect the vascular system and to keep it intact after injury. The dynamic hemostatic balance comprising interactions between endothelial cells, thrombocytes, coagulation, and fibrinolysis prompts the regulation of hemostasis in order to assure the function of tissues and organs. This mechanism ensures the control of hemorrhage and thrombosis pathway activation and provide a matrix in wound healing and tissue repair. The amount of fibrin layers, at a site of injury inducing the progress of the tissue repair, is controlled by hemostasis balance [11].
When this equilibrium is disturbed under any condition, the physiologic process becomes pathologic leading to bleeding or to thrombotic troubles.
Numerous genetic, acquired and environmental factors can disturb the balance in favor of coagulation, leading to the pathologic formation of thrombi in veins, arteries, or cardiac chambers [1, 12].
The German pathologist Rudolf Virchow recognized that if this dynamic balance was altered by venous stasis, abnormal coagulability and vessel wall damages, microthrombi could propagate to form macroscopic thrombi. This understanding of thrombosis formation has been baptized as the triad theory in 1856 (Figure 1) [13]. Mechanisms of stasis, hypercoagulability, and endothelial dysfunction have been, subsequently elucidated as well as the different major factors involved in the hemostasis and coagulation cascade and fibrinolytic system, both at the biochemical and genetic levels [14].
The triad contributing together to venous thrombosis described by Rudolph Virchow.
Typically, arterial thrombotic disease is interrelated to atherosclerosis and thrombosis, as well as their interaction designed by the term atherothrombosis. Acute arterial thrombosis occurs at the site of a ruptured, lipid-rich atherosclerotic plaque. This event contributes to the transition of a stable atherosclerotic disease to an acute state [3]. Depending on the localization of atherosclerotic plaques, arterial thrombotic disease may be an acute infarction such as myocardial or brain infarctions, ischemic stroke, or peripheral arterial occlusion leading to ischemia. Arterial thrombosis can also be due to other pathological conditions favoring arterial clotting and turbulences such as atrial fibrillation and antiphospholipid syndrome [1, 3].
In veins, Virchow’s triad is traditionally invoked to explain pathophysiologic mechanisms leading to thrombosis. In fact, abnormalities in blood composition with plasma hypercoagulability, alterations in the wall components of blood vessel and changes of the blood flow with stasis, are the three components involved in the development of venous thrombosis [13]. Clinical manifestations of venous thrombosis include acute peripheral venous thrombosis (phlebitis) and deep venous thrombosis or venous thromboembolism as well as pulmonary embolism, the most serious acute complication of deep venous thrombosis. Long-term complications represented by post-thrombotic syndromes are due to damages affecting the valves in the veins. Venous thromboembolism and superficial vein thrombosis account for about 90% of venous thrombosis. Other rarer forms include retinal vein thrombosis, splanchnic vein thrombosis, cerebral venous sinus thrombosis, renal vein thrombosis, and ovarian vein thrombosis [15].
The complex thrombosis related pathways crosstalking implies hemostasis and coagulation, inflammation and immune system as well as the contributing role of Redox homeostasis and the interplay of oxidative/nitrosative stress to both inflammation and coagulation [16, 17].
Understanding, components and factors as well as steps of hemostasis and coagulation pathways, is important in defining the molecular variants related to the thrombosis pathogenesis [18].
Hemostasis encompasses the tightly regulated processes of blood clotting, platelet activation, and vascular repair. Hemostasis, which is the physiologic response to vascular endothelial injury, encompasses a series of processes to maintain blood within the vascular system through the formation of a clot. It involves three basic steps: vascular spasm, platelet clot formation, and coagulation, in which activation of the coagulation cascade clotting factors promotes the formation of a fibrin clot. Fibrinolysis is the process in which a clot is degraded [19].
Hemostasis can be divided into primary hemostasis and secondary hemostasis corresponding to the coagulation process. The fibrinolytic pathway called the tertiary hemostasis interacts to regulate fibrin deposition and removal during healing [18, 20].
Primary hemostasis consists of the formation of the platelet clot and includes the blood vessel constriction or vasoconstriction, platelet adhesion, activation and aggregation at the site of the vessel injury. Secondary hemostasis is characterized by the transformation of fibrinogen into fibrin and changes the platelet clot into a stable fibrin clot [20, 21].
During hemostasis, three distinctive pathways can be involved: intrinsic, extrinsic, and common pathways. Activation of the intrinsic pathway is promoted through exposed endothelial collagen, while activation of the extrinsic pathway is stimulated through tissue factor released by various cells in particular the endothelial cells after external damage. These pathways initiate separately at the beginning but at a specific moment with the presence of factor X, the Stuart-Prower factor, they converge, leading to common pathway with the generation of the prothrombinase complex that cleaves the prothrombin into thrombin and then fibrin activation process and platelet clot stabilization with a fibrin webbing. Coagulation cascade involving conversion of inactive coagulation factors to their active forms following a series of enzymatic reactions including multiple cofactors and that ends with the conversion of fibrinogen to fibrin, leads to the formation of the definitive fixed blood clot with scrambled blood cells. The factors II, VII, IX, X, XI and XII circulate as zymogens that are activated into serine proteases to act as catalytic agents cleaving the next zymogen into more serine proteases, whereas factors V, VIII, XIII are not serine proteases [20, 21, 22].
To look at the multiple involved factors and actors in hemostasis pathways as well as their complex interactions; we reviewed recent literature reviews detailing the physiology of hemostasis and coagulation pathways. The biologic and molecular factors, cofactors and actors of the hemostasis pathways are summarized in Table 1 and Figure 2.
Clotting factors | Aliases names | Gene | Chromosome | Exons | Gene ID |
---|---|---|---|---|---|
Factor I | Fibrinogen | FGB | 4q31.3 | 8 | 2244 |
Factor II | Prothrombin | FII | 11p11.2 | 14 | 2147 |
Factor III | Thromboplastin -Tissue Factor | FIII | 1p21.3 | 6 | 2152 |
Factor IV | Ionized calcium | ||||
Factor V | Proaccelerin | FV | 1q24.2 | 25 | 2153 |
Factor VI | Unassigned | ||||
Factor VII | Proconvertin -Stable factor | FvII | 13q34 | 10 | 2155 |
Factor VIII | Anti-hemophilic factor A | FVIII | Xq28 | 27 | 2157 |
Factor IX | Christmas factor | FIX | Xq27.1 | 8 | 2158 |
Factor X | Stuart-Prower factor | FX | 13q34 | 8 | 2159 |
Factor XI | Plasma thromboplastin | FXI | 4q35.2 | 15 | 2160 |
Factor XII | Hageman factor | FXII | 5q35.3 | 15 | 2161 |
Factor XIII | Fibrin stabilizing factor | FXIIIA1 | 6p25.1 | 15 | 2162 |
FXIIIB | 1q31.3 | 12 | 2165 |
The three distinctive pathways of hemostasis: intrinsic, extrinsic, and common pathways.
At the cellular level, hemostatic reactions involves plasma, platelet, and vascular components. After a blood vessel injury the extracellular matrix and the collagen become unprotected and in contact with the blood within an area of vasoconstriction, leading to the liberation of cytokines and inflammatory markers. Consequently, platelet adhesion, activation and aggregation at that site are sequentially mediated by interactions between various receptors including tyrosine kinase receptors, glycoprotein receptors, other G-protein receptors and proteins within the platelets [23]. Platelet degranulation induces the liberation of Adenosine diphosphate, thromboxane A2, serotonin, and multiple other activation factors. The conversion of fibrinogen to fibrin and the formation of a platelet-fibrin hemostatic clot ends by a coagulation cascade involving the formation of fibrin polymer mesh catalyzed by activated factor XIII that stimulates the lysine and the glutamic acid side chains causing the cross-linking of the fibrin molecules and the formation of a stable fibrin clot [24].
The fibrinolytic pathway called the tertiary hemostasis interacts to regulate fibrin deposition and removal during healing. The activities of thrombin and other serine proteases are modulated by the serine protease inhibitors (serpins), including antithrombin III and heparin cofactor II which are important in regulating the physiological anticoagulant action of glycosaminoglycans at the endothelium [25].
Under normal circumstances, there exists a fine balance between the procoagulant and anticoagulant pathway and hemostasis is under the inhibitory control of several inhibitors that limit clot formation, thereby avoiding thrombus propagation. This balance is disturbed whenever the procoagulant activity of the coagulation factors is increased, or the activity of naturally occurring inhibitors is decreased [14, 26]. As thrombin acts as a procoagulant, it also acts as a negative feedback by activating plasminogen (Serpine 1 Gene ID: 5054 7q22.1 with 9 exons) to plasmin and stimulating the production of antithrombin (Serpinc1 Gene ID: 462, 1q25.1 with 9 exons). Plasmin acts directly on the fibrin mesh and breaks it down. Antithrombin decreases the production of thrombin from prothrombin and decreases the amount of activated factor X. Protein C or blood coagulation factor XIV (PROC Gene ID: 5624, 2q14.3 with 8 exons) and protein S (PROS1 Gene ID: 5627 3q11.1 with 16 exons) act to prevent coagulation, mainly by inactivating factors V and VIII. The Kunitz-type protease inhibitor tissue factor pathway inhibitor (TFPI Gene ID: 7035, 2q32.1 with 13 exons) limits the diffusion of the coagulation cascade. TFPI binds to FXa or the TF-FVIIa-FXa complex to restrict coagulation function [https://www.genecards.org, https://www.ncbi.nlm.nih.gov/gene/].
Under abnormal circumstances, the formation of thrombi happens in a not breached vessel, in particular in venous thrombosis where thrombi are formed subsequently to the activation of the clotting system. However, in arterial thrombosis, thrombi are considered typically as the result of a phenomenon of atherothrombosis after rupture of atherosclerotic plaques leading to platelet activation and interactions between platelet activation, tissue factor vesicle expression from plaque macrophages, and then activation of the coagulation cascade [27].
Understanding the role of inflammation in thrombosis disorders is important in defining the molecular variants related to the thrombosis pathogenesis.
The complex pathways of inflammation and hemostasis appear to have a common evolutionary origin and interrelated pathophysiologic processes [28].
In fact, there is an inflammation-hemostasis cycle in which each activated process promotes the other, and the two systems function in a positive feedback circle. The mechanisms responsible in the relations between thrombosis and inflammation involve all components of the hemostatic system including associated cells and plasma coagulation/fibrinolysis cascades [1, 28, 29].
The first event in thrombus formation is probably the stimulation of an inflammatory response with the activation of endothelial cells, platelets, and leukocytes. Initiation of inflammation leads to the formation of microparticles that activate the coagulation system through the induction of tissue factor. In fact, throughout the inflammatory response, various inflammatory mediators, in particular proinflammatory cytokines play a central role in ever-changing the hemostatic activity towards procoagulant state by triggering endothelial cell dysfunction, increased platelet reactivity, activation of the plasma coagulation cascade, impaired function of physiologic anticoagulants and inhibited fibrinolytic activity [30].
On the other side, coagulation cascade augments inflammation by means of thrombin-induced secretion of proinflammatory cytokines and growth factors. Platelets may also trigger inflammation, in particular by activating the dendritic cells. In abnormal circumstances, other inflammatory factors are implicated such as chemokines, adhesion molecules, platelet-derived mediators linking thrombosis and atherosclerosis and thrombosis, infection and immunity [28, 31].
Recently, there is a consensus that vascular thrombosis diseases are simultaneously, triggered by biological stimuli responsible for activating coagulation and inflammatory pathways in both the arterial and the venous systems [32]. In fact, while it is commonly recognized that the pathogenesis of arterial thrombotic disease is related to the chronic lipid-driven inflammatory disease of the arterial wall characterized by the involvement of the innate and adaptive immune systems or atherosclerosis, it is only recently that inflammation has been accepted as a common pathway of venous thrombosis formation [33, 34].
The most well described pathophysiologic process, in which there are an established relation between inflammation and hemostasis is the arterial atherothrombosis generated consequently to ruptured atherosclerotic plaque. Besides, chronic inflammation may cause endothelial damage, resulting in the loss of physiologic anticoagulant, antiaggregant and vasodilatory properties of endothelium. There are, many systemic inflammatory diseases characterized by thrombotic tendency in the absence of vessel wall damage, including chronic autoimmune diseases and vasculitis, such as Behçet disease, antineutrophilic cytoplasmic antibody-associated vasculitis, Takayasu arteritis, rheumatoid arthritis, systemic lupus erythematosus, antiphosholipid syndrome, familial Mediterranean fever, thromboangiitis obliterans and inflammatory bowel diseases [28, 35, 36].
Inflammation-induced venous thrombosis developed in the absence of vessel wall damage, in particular during malignancies, is also well demonstrated. Malignant proliferation induces prothrombotic substrates such as tissue factor and production of inflammatory cytokines, including tumor necrosis factor (TNF Gene ID: 7124, 6p21.33 with 4 exons) and interleukin-1 (IL1A Gene ID: 3552, 2q14.1 with 8 exons and IL1B Gene ID: 3553, 2q14.1 with 7 exons). This leads to the shift of the hemostatic state to procoagulant state that predisposes to the development of venous thrombosis [1, 37].
On the other hand, during the coordinated intravascular coagulation response of platelets in response to various blood pathogens and consequent tissue damage recently termed immunothrombosis, the risk of thrombosis that manifests as arterial or venous thrombosis (and may contribute to atherosclerosis). During this process of immunothrombosis, inflammation-dependent activation of the coagulation system is part of the host response to pathogens, aiming to limit their systemic spread in the bloodstream [38, 39]. This response is achieved through an interplay between innate immune cells and platelets, triggering the activation of the coagulation system and the releasing of the complement system. Platelets and immune cells form, in fact, a physical barrier of confinement preventing dissemination of pathogens and potentially leading to activation of the innate and adaptive branches of the immune system [40]. Interestingly, platelets mediate the crosstalk between the hemostatic and the immune system utilizing similar pathways. The dysregulated and excessive activation of immunothrombosis results in thromboinflammation, causing tissue ischemia by microvascular and macrovascular thrombosis. Pulmonary immunothrombosis in severe COVID-19 correlating with a systemic prothrombotic phenotype provides clinical evidence for the partnership between inflammation and thrombosis [12, 41].
There is now a strong evidence for the participation of reactive oxygen and nitrogen species in the pathogenesis of thrombosis as well as solid proofs of an interplay of oxidative and nitrosative stress, inflammation and thrombosis [42].
First, it is well established that reactive oxygen species (ROS) participate in vascular cell signaling and proatherogenic gene expression by modulation of oxidation–reduction (Redox) reactions pathways [43, 44, 45].
The cellular redox state, or balance between cellular oxidation and reduction reactions, serves as a vital antioxidant defense system that is linked to all important cellular activities. Redox homeostasis is thought to be achieved by careful regulation of both ROS formation and removal from the body system [46].
Recently, redox processes in cell signaling imply, beside ROS, Reactive Nitrogen Species (RNS). In fact, ROS and RNS were identified as key players in initiating, mediating, and regulating the cellular and biochemical complexity of oxidative stress either as physiological or as pathogenic processes [47].
Oxidative stress is a term associated with both enhanced production of ROS and reduced efficacy of protection by antioxidant enzymes. Nevertheless, after the discovery of NO as a biological entity and the powerful role of superoxide radicals O2- and NO as oxidants via ONOO- formation, oxidative stress has become unavoidably related to nitrosative stress and RNS. The key species associated with oxidative and nitrosative stress as well as their interactions have been reviewed and it was suggested that ROS are the initial reactants produced from an ionization event, whereas RNS are the effectors/activators of redox-dependent cellular signal transduction pathways [48, 49].
Depending on the severity of the oxidative stress, adaptive processes occur by increasing antioxidant capacities and by growing the capacity of the oxidative damages reparation. In extreme cases, metabolic processes shift away from oxidative metabolism towards glycolytic metabolism. In the case of chronic metabolic oxidative stress along with the accumulation of oxidative damage to critical biomolecules, potentially pathological conditions can develop due to the cumulative oxidative damage interacting with proteins, lipids, and DNA [48, 50].
An excessive ROS generation or a defect in the antioxidant defense system impacts a wide variety of biological molecules, lipids in the plasma and mitochondrial membranes, causing lipid peroxidation that impairs membrane selective permeability, proteins (resulting in structural instability and damage to their enzymatic function) and nucleic acids, thus inducing pathways of apoptosis [51].
In particular, oxidative stress is responsible for the disruption of the coagulation cascade at various stages leading to anomalies in blood coagulability and platelet reactivity. Nicotinamide adenine dinucleotide phosphate (NADPH) oxidase family (NOX) enzymes appears to be the most important source for ROS involved in processes related to thrombosis [52]. On the other hand, oxidative stress contributes to the development of atherosclerosis leading to atherothrombosis [53].
Oxidative pathways of thrombosis can occur throughout endothelial apoptosis, impairment of red blood cells quality and function, endothelial dysfunction and damage of endothelial cell lining, activation of platelets and leukocytes, and consequently by affecting the clotting system. The endothelial cell lining is essential in triggering the prothrombotic events as an intact endothelial cell lining prevents platelets adherence and activation. Furthermore, endothelial injury-associated oxidative stress promotes tissue factor expression having a potent procoagulant activity. In fact, ROS increases the expression of tissue factor in endothelial cells, monocytes and vascular smooth muscle cells, with essentially the contribution of NOX enzymes [54]. Whereas TFPI, which is the only physiologic regulator of tissue factor activity, can be inhibited by oxidative stress and exerts a procoagulant effect. ROS can also directly inactivate major anticoagulant proteins such as protein C and its upstream agonist thrombomodulin (THBD Gene ID: 7056, 20p11.21 with one exon). The stimulation of protease-activated receptors (PARs) may also lead to endothelial tissue factor induction via mitochondrial ROS signaling [55].
ROS stimulates platelet reactivity and during this ROS generation/platelet reactivity, platelet ROS are mostly generated by reduced NADPH oxidase. NOX2 expressed in platelets is an important regulator of platelet activation associated thrombosis. Engagement of primary platelet receptors, GPIb-IX-V and GPVI, that initiate thrombus formation, leads to a rapid increase in intracellular ROS above basal levels, and is a key step in platelet activation following exposure to physiological ligands such as von Willebrand factor (VWF)/collagen [55, 56, 57].
Thus, in contrast to endothelial injury-associated thrombus, platelet-dependent thrombus formation may also be influenced by alteration of platelet redox state or other cells or vascular redox state. Settings and pathways that influence the formation of superoxide and nitric oxide, as well as their metabolism, may specifically influence platelet function and thrombus formation [58].
Many studies emphasis that ROS influences venous thrombus formation and resolution through the modulation of the coagulation, the fibrinolysis, the proteolysis and the complement system, as well as the regulation of effector cells such as platelets, endothelial cells, erythrocytes, neutrophils, mast cells, monocytes and fibroblasts. During antiphosholipid syndrome for example, venous thrombosis occurs in patients having alterations in their redox homeostasis [42].
Reactive free radicals are defined as any chemical species capable of independent existence that contains one or more unpaired electrons. Reactive oxygen species (ROS) and Reactive nitrogen species (RNS) are free radicals that are associated with the oxygen atom (O) and other molecules, with stronger reactivity. Other biologically important free radicals exist such as lipid hydroperoxide (ROOH), lipid peroxyl radical (ROO), and lipid alkoxyl radical (RO), which are associated with membrane lipids and thiol radical (RS), which has an unpaired electron on the sulfur atom [59].
ROS consists of radical and non-radical oxygen species formed by the partial reduction of oxygen, including superoxide anion (O2-), hydroxyl radicals (OH), singlet oxygen (1O2) and hydrogen peroxide (H2O2). Generally, ROS are generated endogenously as natural by-products of aerobic metabolism during mitochondrial oxidative metabolic rate and by the means of cytochrome p450, cyclooxygenase, lipoxygenase and NOX enzymes. ROS are, also generated in response to stimulation such as by cytokines and other inflammatory mediators [59, 60].
Imbalance between oxidative stress and antioxidant status may be the result of an up-regulation of ROS-producing enzymes, such as NADPH oxidase and myeloperoxidase, along with down-regulation of antioxidant enzymes, such as superoxide dismutase (SOD) and glutathione peroxidase (GPx). Antioxidant defenses modulate the steady state balance of ROS with the implication of other several antioxidant enzymes such as catalase, glutathione peroxidases, heme oxygenase, thioredoxin system as well as small molecule antioxidants such as glutathione, vitamins A, C and E. These enzymes are produced to scavenge ROS, thereby limiting their detrimental effects [60, 61].
For example, age-dependent increased venous thrombosis is related to age-related endothelial dysfunction involving upregulation of the NADPH oxidase and cyclooxygenases (COXs)-dependent oxidative stress pathways. On the other hand, overexpression of the antioxidant enzyme GPX-1 protects from age-dependent increased venous thrombosis. Moreover, during aging, abnormal aged red blood cells may also adhere to the endothelium or extracellular matrix, activate platelets and other cells, and enhance local thrombin generation during thrombosis [52].
Second, in nitrosative stress, RNS involve various species such as nitric oxide (NO), nitrogen dioxide (NO2) and peroxynitrite (ONOO-). NO is generated in biological tissues by specific nitric oxide synthases (NOSs) and acts as an important oxidative biological signaling molecule in defense mechanisms and immune regulation. In the extracellular milieu, NO reacts with oxygen and water to form within an enzymatic cascade more reactive products. Immune cells, including macrophages and neutrophils, simultaneously release NO and superoxide into their phagocytic vacuoles. Other inflammatory cells can also produce reactive chemicals that can result in 3-NT formation, including the peroxidases in activated neutrophils and eosinophils. 3-NT is a characteristic marker of nitrosative stress and, commonly, inflammation [47].
NO was originally discovered as a vasodilator product of the endothelium and later as a factor having important antiplatelet actions, inhibitor effects of leukocyte adhesion and migration, and other inflammatory cells adhesion. By activating guanylyl cyclase, inhibiting phosphoinositide 3-kinase, impairing capacitative calcium influx, and inhibiting Cox-1, endothelial NO limits platelet activation, adhesion, and aggregation. Platelets are also an important source of NO, and this platelet-derived NO pool limits recruitment of platelets to the platelet-rich thrombus [62, 63].
A deficiency of bioactive NO is associated with arterial thrombosis in individuals with endothelial dysfunction and patients with a deficiency of the extracellular antioxidant enzyme GPx-3. Impaired NO availability also seems to be caused by inactivation of NOS and the levels of an endogenous inhibitor of NOS such as asymmetric dimethylarginine (ADMA). On the other hand, it seems that the decline in vascular NO production may be a characteristic feature of mammalian aging [47, 64].
Low NO availability is incriminated in thrombus formation. In fact, in the presence of low NO availability, endothelium-dependent vasodilation is impaired, which leads to abnormal red blood cells adhesion, and may contribute to increased platelet activation [65].
NO is considered as having a dual role as a protective or harmful molecule depending on tissue concentration levels and interaction with oxidative stress. In the endothelium, NO has antiatherogenic actions related to the inhibition of platelet function and inflammatory cell adhesion, promotion of fibrinolysis, and attenuation of smooth muscle cell proliferation. Oxidative stress and enhanced ROS production seem to be involved in the down-regulation of the protective NO pathway [48].
Finally, ROS/RNS generated during inflammation and inflammatory response and crosstalk between cellular redox state and the ROS/RNS network during inflammation constitute an emerging field. In states of inflammation, NO production by the vasculature increases considerably and, in conjunction with other ROS, contributes to oxidative stress [47].
ROS/RNS have also emerged as important modulators of intracellular transduction signaling. These radicals interact with redox-sensitive signaling molecules including protein tyrosine phosphatases, protein kinases and ion channels, regulating cellular processes like growth factor signaling, hypoxic signal transduction, autophagy, immune responses, and stem cell proliferation and differentiation. Moreover, the level of miRNAs can be modulated at the transcription and/or processing level by stress-induced factors like p53 or NF-kB as well as the presence of intracellular hydrogen peroxide levels [43, 44, 51, 66].
Among the many important insights derived from completion of the Human Genome Project was the recognition of the abundance of single nucleotide polymorphisms (SNPs) as a major source of genetic variation. Studies over the past last years have resulted in increasing recognition of the critical role of structural genetic variation in particular of copy-number variation in modulating gene expression and disease phenotype. Recently, genome-wide surveys and association studies are being widely applied to identify genetic factors that affect complex diseases or traits. However, while for SNP-association studies there are well-developed available resources, resources for structural genetic variation identified via genome-wide association studies are still in their early phases [67, 68, 69].
Arterial and venous thrombosis, with their clinical manifestations classified as complex multi-factorial diseases are related to various genetic variations that are both deleterious mutations and disease-susceptibility sequence polymorphisms, since the last century. In fact, beyond deficits in coagulation inhibitors, which have been known for a long time, the two most known thrombogenic mutations have been discovered in 1994 and 1996 [69].
Genetic studies in thrombosis started with the conception of the term thrombophilia by Jordan and Nandorff in 1956 [70]. Nine years later, antithrombin deficiency was identified as a genetic risk factor of thrombosis [71]. In the 1990s, activated PC resistance and the causal genetic variation of factor V Leiden, the first-born thrombogenic mutation, were revealed in a family setting. Factor V Leiden risk factor was also the first prothrombotic defect in a procoagulant protein. In 1996, case–control studies revealed the common prothrombin 20210 G > A mutation [72].
Using association studies and commonly PCR-RFLP tools, many genetic variations in almost all coagulation proteins were tested. However, until the beginning of the new century, only few gene loci were significantly associated with thrombotic diseases. The majority of the genetic variations was identified in the coding genes of hemostasis and coagulation factors and was shown as important risk factors for particularly venous thrombosis [73]. In contrast, in arterial thrombosis disease commonly related to atherosclerosis, many polymorphisms were identified, with significant relationships demonstrated between genotypes and plasma phenotypes. However, the exact contribution of genotypes to clinical phenotypes remains regularly uncertain. These variants associated in majority to a small risk, if any risk at all, have a limited usefulness as relevant biomarkers of the thrombotic diseases that must be prescreened to guide prevention, prognosis and treatment [74].
Nowadays, despite the success of genome-wide association studies in identifying new genetic factors determining many thrombosis-related diseases such as coronary artery disease, results for arterial and venous thrombosis have yielded little success. One of the reasons for the limited number of loci identified is most likely the lack of power due to the small sample sizes of studied cases [75].
Since the underlying pathogenic mechanisms are only partially known, regarding the complex interplay of many pathways in thrombosis-related pathogenesis as shown in the chapter 3 and the emerging role of intricate modulators of intracellular transduction signaling, there is mounting evidence indicating the challenging struggle of the mapping disease-susceptibility genes in thrombotic disorders. Genetic variations within thrombosis related pathways involving hemostasis and coagulation, inflammation, and immune system as well as Redox homeostasis and oxidative/nitrosative stress might be potential risk factors. Subsequently, many new loci need identification as risk factors as well as characterization in the future, through studies of candidate genes and genome-wide association studies.
Thrombophilia traditionally refers to rare inherited defects leading to enhanced coagulation, especially of the venous system. Thrombophilia may be inherited or acquired. Acquired causes of thrombophilia include trauma, surgery, pregnancy, use of oral contraceptives, antiphospholipid syndrome, paroxysmal nocturnal hemoglobinuria and heparin induced thrombocytopenia. Inherited causes of thrombophilia are related to the hypercoagulability state that may arise from an excess or hyperfunction of a procoagulant or a deficiency of an anticoagulant factor [72].
In 1937, Nygaard and Brown first used the term thrombophilia, when they described sudden occlusion of large arteries, sometimes with coexistent venous thrombosis. Investigation of thrombophilia causes started by familial setting within families characterized by a predisposition to thromboembolic diseases and a strong tendency to venous thrombosis. This approach leaded to the early description of the deficiency of antithrombin causing venous thromboembolism at a young age related to thrombophilia entity in several members of a Norwegian family. Deficiencies of protein C and protein S were discovered after few years like the novel hereditary thrombophilia risk factors in other anticoagulant proteins. The inherited risk factors implying prothrombotic factors for thrombophilia were identified in following years like the underlying causes linked to venous thrombosis. They included FV Leiden variant linked to resistance to activated protein C (APC resistance) and FII 20210 G/A transition linked to elevated levels of Prothrombin (Table 2) [82, 83].
The factor V G1691A and prothrombin G20210A polymorphisms in arterial disease have been subjects of numerous reports. Many of these—some large—concerned with their association with arterial disease in young, middle-aged, and elderly populations had negative results. In contrast, some studies report positive associations, particularly when the interaction of these polymorphisms with environmental factors were formally evaluated [82, 83].
In 1988, Kang et al. [84] described a heat-labile form of MTHFR associated with mild hyperhomocysteinemia. The C677T polymorphism of the MTHFR gene has led to the identification of many more cases of thrombophilia.
Hereditary thrombophilia manifests more or less severely and early depending on the genotype, which may be heterozygous (a single affected allele), homozygous or composite heterozygous (two affected alleles) or associated with several different genetic risk factors.
Association studies between inherited thrombophilia and venous thromboembolic disease showed dominance of factor V Leiden, and factor II G20210A variant in comparison with coagulation protein deficiencies (Table 3).
The factor V gene (Gene ID: 2153) is located on the long arm of chromosome 1 at q24.2. It consists of 25 exons that span a region of approximately 80. The FV gene encodes a propeptide of 2224 amino acids containing a 28-residue signal peptide, excised after translocation into the endoplasmic reticulum. This propeptide, called proaccelerin, is a monomeric protein of 330 kDa. It is characterized by a domain structure with 3 A domains (330aa), 2 C domains (150aa) and a B domain [N-A1-A2-B-A3-C1-C2--COOH]. Proaccelerin consists of two calcium-stabilized non-covalent chains: a heavy chain (110,000) and a light chain (74,000–71000). It is highly N- and O-glycosylated (about 13–25% of the mass, i.e. 37 N-glycosylation sites: 25 at the B-domain, 9 heavy chains and 3 light chains). Factor V exists in two forms V1 and V2, related to the heterogeneity of the molecular mass of the light chain and caused by the partial glycosylation at the Asn2181 residue (3 and 2 carbohydrate chains respectively for FV1 and FV2). These 2 forms differ in their functions: FV2a would have more affinity for membrane phospholipids and thrombin generation. Factor V is synthesized by hepatocytes and megakaryocytes. Approximately 80% of pro-accelerin is circulating in plasma (with a concentration of 5-10 mg/l = 21 nM) and only 20% is stored in the α-granules of platelets (i.e. between 4600 and 14000 molecules/platelet) in association with BPM (binding protein multimerin). This platelet fraction is released during platelet activation [91, 92].
Proaccelerin has a dual function: procoagulant and anticoagulant. Procoagulant action: Factor Va is part of the prothrombinase complex (Xa;Va;PL;Ca) that converts prothrombin (FII) to thrombin (FIIa), which is responsible for thrombus formation. It is initially activated by thrombin, which eliminates the B domain, and then its Xa cofactor binds to the C2 domain. At the molecular level, factor V performs its procoagulant function after proteolysis by thrombin and FXa at three arginine residues (Arg709, Arg1018, and Arg1545). This results in the elimination of the B domain. Thus FVa is formed by a heavy chain (105 KDa) [A1-A2] and a light chain (74–71 KDa) [A3-C1-C2] stabilized by calcium [92].
Once activated, FV complexed with FXa on membrane phospholipids and in the presence of Calcium forms the prothrombinase complex that converts prothrombin to thrombin. Anticoagulant action: Factor V binds to protein S and is a synergistic cofactor for inhibition of VIIIa by activated protein C. The anticoagulant action requires the inactivation of FVa. This is mediated by protein C which successively proteolyses it at Arg506, Arg306 and Arg 679. The first cleavage at Arg506 reduces the activity of FVa (25–40%) as well as its affinity for FXa, this partial inactivation is completed after cleavage at Arg 306, however Arg 679 is less important in this process. Thus, factor V will be fragmented into FVai (composed of the A1 domain associated with the light chain) and two fragments derived from the A2 domain (A2N and A2C respectively on the N and C terminal side). Alternatively, the inactivation of FVa is mediated by thrombin, which cleaves Arg643 in the presence of endothelial cells, resulting in a reduction of affinity between the two heavy and light chains [91, 92, 93].
On the other hand, activated protein C can degrade intact FV and thus confers an anticoagulant property (FVac). Thus, the latter would be a cofactor of APC and protein S in the degradation of FVIIIa. This anticoagulant property requires cleavage at different sites (Arg306, Arg506, Arg679 and Lys994). However, only Arg 506 is required for the expression of the FV-APC cofactor activity [93]. This functional duality of FV in the coagulation process is dependent on the local concentration of procoagulant and anticoagulant enzymes such as thrombin, FXa and APC, which are responsible for the conversion of FV into a procoagulant or anticoagulant cofactor [94].
Various mutations affecting the FV gene have been described in association with a thrombotic phenotype. Among these missense mutations, the most prevalent is the Factor V Leiden mutation, initially described by Bertina et al. (Table 4) [76].
Thrombophilia risk factor | Prevalence in the general population (%) | Mode of transmission | Reference |
---|---|---|---|
FV Leiden | 2–15 | Dominant | Bertina et al. [76] |
FII G20210A | 2–3 | Dominant | Poort et al. [77] |
MTHFR C677T | 1–11 | Recessive | Frosst et al. [78] |
ATIII deficiency | 0.02–2 | Dominant | Egeberg [79] |
PC deficiency | 0.2–0.5 | Dominant | Griffin et al. [80] |
PS deficiency | 0.1–2.1 | Dominant | Comp and Esmon [81] |
Prevalence and mode of transmission of inherited thrombophilia.
Thrombophilia n/N | Absence of thrombophilia n/N | OR (CI = 95%) | |
---|---|---|---|
FV Leiden heterozygote | |||
Dilley et al. [85] | 8/9 | 32/107 | 18.75 (2.25–156.15) |
Gerhardt et al. [86] | 47/65 | 72/287 | 7.80 (4.26–14.28) |
Martinelli et al. [87] | 22/28 | 97/323 | 8.54 (3.36–21.73) |
Murphy et al. [88] | 3/16 | 29/556 | 4.19 (1.13–15.54) |
Tormene et al. [89] | 6/94 | 1/81 | 5.45 (0.64–46.29) |
TOTAL (95%) | 86/212 | 231/1354 | 8.94(2.32–50.79) |
FII G20210A HETEROZYGOTE | |||
Dilley et al. [85] | 4/4 | 36/112 | 18.86 (0.99–359.76) |
Gerhardt et al. [86] | 20/23 | 98/321 | 15.17 (4.41–52.24) |
Martinelli et al. [87] | 7/14 | 112/337 | 2.01 (0.69–5.87) |
TOTAL (95%) | 31/41 | 246/770 | 12.01(2.03–139.29) |
MTHFR C677T HOMOZYGOTE | |||
Dilley et al. [85] | 5/13 | 22/63 | 1.16 (0.34–3.99) |
Murphy et al. [88] | 1/57 | 9/223 | 0.42 (0.05–3.42) |
Ogunyemi et al. [90] | 2/12 | 28/48 | 0.14 (0.03–0.72) |
TOTAL | 8/82 | 59/334 | 0.57(0.42–2.71) |
ATIII Deficiency | |||
Gerhardt et al. [86] | 6/8 | 83/212 | 4.66 (0.92–23.65) |
Martinelli et al. [87] | 1/2 | 118/349 | 1.96 (0.12–31.58) |
TOTAL | 7/10 | 201/561 | 3.31(0.52–13.61) |
PC Deficiency | |||
Gerhardt et al. [86] | 15/24 | 91/312 | 4.05 (1.71–9.58) |
(Ogunyemi et al. [90] | 2/2 | 28/58 | 5.35 (0.25–116.31) |
TOTAL | 17/26 | 119/370 | 4.7(0.98–62.94) |
PS Deficiency | |||
Gerhardt et al. [86] | 13/24 | 92/309 | 2.79 (1.2–6.45) |
Martinelli et al. [87] | 2/3 | 117/348 | 3.95 (0.35–44.00) |
TOTAL | 15/27 | 209/657 | 3.37 (0.77–25.22) |
Association studies between inherited thrombophilia and venous thromboembolic disease.
Codon | AA | Name | Reference |
---|---|---|---|
ARG306GLY | 1090A-G | FV HONG KONG | Chan et al. [95] |
ARG306THR | 1091G-C | FV CAMBRIDGE | Williamson et al. [96] |
ILE359THR | 1250 T-C | FV LIVERPOOL | Steen et al. [97] |
Arg506Gln | 1691G-A | FV LEIDEN | Bertina et al. [76] |
Various mutations affecting the FV gene.
Many studies have focused on the pathogenicity of VF in the occurrence of thrombophilia. Since its discovery in 1994 by Bertina et al. [76], FV Leiden represents the major anomaly in thromboembolic patients. It is a 1691G-A transition in exon 10 of the FV gene resulting in an Arg506-to-Gln substitution (R506Q) (Figure 3). This mutation is responsible for resistance to activated protein C, since it affects the potential site of cleavage by activated protein C, both for FVa degradation and FV-APC cofactor activity for FVIIIa inactivation [98, 99].
Sanger sequence of the G1691A Factor V Leiden mutation in exon 10 of the FV gene.
The thrombotic risk depends on the form of expression of the FV Leiden allele: it is 5–7 times in heterozygotes, 30 times in homozygotes and intermediate in pseudo homozygotes. The latter is a particular form, where the FVL allele is associated with another deficient or null allele [98].
Different mutations have been described in association with FV Leiden. The first mutation is a A4070G transition at exon 13 of the FV gene, resulting in a His1299Arg substitution, described in 1997 [100]. This mutation is an allelic form characterized by a moderate deficiency in Factor V not counterbalanced by FV Leiden; hence the occurrence of thrombosis.
In 1998, it was identified a null mutation that consists of a C2308T transition, at exon 13 of the FV gene affecting codon Arg 712(CGA), and producing a stop codon (TGA) resulting in a truncated protein at the level of its light chain (A3, C1, and C2 domains) unable to perform its anticoagulant function. As a result, only FV Leiden molecules are present and thus responsible for thrombosis [101].
The geographic distribution of FVL is extremely heterogeneous: it is absent in Asians, Africans, Americans, and Australians; however, it is prevalent in the Caucasian population. The existence of a single haplotype of FV Leiden worldwide suggests a single mutational event that occurred about 30,000 years ago, after the migration from Africa and the segregation of Asians from Europe. The age of factor V Leiden is estimated at 21,340 years [102].
FV Leiden is a remarkable genetic anomaly in more ways than one. It is common in the general population (2–15%) and affects 20–25% of patients with at least one episode of venous thromboembolism. Carriers of the anomaly are heterozygous in the vast majority of cases, which increases their risk of thrombosis by a factor of 5. However, homozygotes are not rare (0.05 to 0.25%) in the general population. They have a significant risk of venous thromboembolism (RR in the range of 20–30), but generally have no thrombotic events in childhood. They may remain asymptomatic, even in the homozygous state as the Factor V Leiden mutation has incomplete penetrance [103].
In the Chinese population, it was identified a 1090A-G substitution in exon 7 of the FV gene resulting in an Arg306Gly (R306G) substitution and the mutation is named Factor V Hong Kong. It is one of the sites of cleavage by activated protein C that is affected, leading to a loss of the procoagulant activity of FVa. However, no predisposition to thrombosis was detected [95].
In 1998, at Addenbrooke’s Hospital (Cambridge, England), Williamson et al. [96] identified a new mutation of the FV gene in a thrombophilic patient. It is a G to C transversion that results in an Arg306Thr (R306T) substitution. This mutation affects the APC cleavage site and is responsible for a loss of procoagulant activity of FVa. Unlike FV Hong Kong, FV Cambridge is associated with resistance to activated protein C.
In 2004, Steen et al. [97] identified a new mutation affecting the FV gene, called FV Liverpool. It is a 1250 T-C transition resulting from an Ile359Thr substitution (I359T). This mutation reduces the susceptibility of FVa to proteolysis by APC, since it alters the N- glycosylation at the asn357 residue of the A2 domain. Thus, the anticoagulant activity of FV is decreased and resistance to protein C is observed.
The factor II gene (Gene ID: 2147) is about 21 Kb long. It is located on chromosome 11, near the centromere (band 11p11.2). It has 20,241 bp, 14 exons of 25 to 315 bp and 13 introns of 84 and 9447 bp.
Factor II protein or prothrombin is one of the coagulation factors whose hepatocyte synthesis depends on vitamin K. It is a globular protein of about 72 kDa. It consists of a polypeptide chain of 579 amino acids, formed by functional domains found in several coagulation factors. The propeptide (residues −43 to −1), encoded by exons 1 and 2, is cleaved before secretion of the protein by hepatocytes. The Gla domain (residues 1 to 37), encoded by exon 2, is characteristic of vitamin K-dependent proteins: it contains 10 glutamic acid (Glu) residues that are converted to c-carboxy-glutamic acid (Gla) post-translationally by a vitamin K-dependent carboxylase present in the endoplasmic reticulum of the hepatocyte. Gla residues are involved in binding to anionic membrane phospholipids (mainly phosphatidylserine) in the presence of calcium. Two “Kringle” domains (Kringle 1: residues 65–143; Kringle 2: residues 170–248) are encoded by exons 5–6 and exon 7 respectively. Kringle 2 is involved in the binding of prothrombin to factor Va. The C-terminal part of prothrombin carries the serine protease domain, encoded by exons 8–14 [104].
Thrombin is the active form of factor II. It is composed of two polypeptide chains joined by a disulfide bridge: an A chain (residues 284–320) encoded by exons 8 and 9 and a B chain (residues 321–579) encoded by exons 9 to 14. Prothrombin synthesized in hepatocytes is found in the bloodstream. Prothrombin is activated by the prothrombinase complex into thrombin, a potential factor in the coagulation cascade. The prothrombinase complex consists of an enzyme (factor Xa, or FXa), a protein cofactor (factor Va, or FVa) and anionic phospholipids. FXa performs two cleavages at the Arg271/Thr272 and Arg320/Ile321 peptide bonds, giving rise to thrombin and activation peptides (F1, F2, F3) [104, 105].
Thrombin, a serine protease, is both multifunctional and highly selective. It has procoagulant properties, converting fibrinogen to fibrin, activating factor XIII, and amplifying its own formation (activation of platelets and factors V, VIII, XI). It is also anticoagulant, since by binding to thrombomodulin, it becomes capable of activating protein C, the negative regulator of coagulation. It activates not only platelets but almost all cell types (blood, vascular and non-vascular cells), thus intervening in many processes other than hemostasis (inflammation, angiogenesis, tissue remodeling, etc.…) [106].
Various mutations have been described associated with the occurrence of thrombophilia (Table 5). These mutations affect both the regulatory and the splicing system and lead to thrombosis and hyperprothrombinemia respectively. Nevertheless, the G 20210A polymorphism first described by Poort et al. [77] is the most incriminated in thrombophilia.
Localization | AA | Reference | Phenotype |
---|---|---|---|
3’UTR | C20209T | Warshawsky et al. [107] | Thrombosis |
3’UTR | C20221T | Wylenzek et al. [108] | Thrombosis |
3’UTR | G20210A | Poort et al. [77] | Thrombosis |
A19911G | Ceelie et al. [109] | Hyperprothrombinemia |
Various mutations affecting the FII gene.
The G20210A mutation affects the 3’UTR region of the FII gene. It leads to transcriptional efficiency through facilitated polyadenylation, resulting in increased prothrombin synthesis (https://www.ncbi.nlm.nih.gov/gene/2147).
The geographic distribution is due to a founder effect that dates back to 23,720 years [102]. The G20210A prothrombin mutation is quite common in the general population (2–3%). It is found in about 10% of patients with venous thrombosis, with carriers having a 3–4 fold increased risk. Homozygotes are rare and are likely to have a higher risk [103].
In 2001, Ceelie et al. [109] focused on the genetic causes of hyperprothrombinemia by analyzing variations in the prothrombin sequence in homozygous 20210-GG subjects. A homozygous 19911-G mutation is associated with an elevated prothrombin level. However, it does not affect thrombotic risk. On the other hand, this risk is potentially increased in association with the G20210A mutation (OR = 1.6 for 19911A versus 4.7 for 19911G). In the same year, Wylenzek et al. [108] detected a new mutational point in a Lebanese family: a C20221T substitution in the 3’UTR region of the F2 gene. In addition, in 2002, Warshawsky et al. [107] identified a mutation in four patients of African American origin presenting venous thrombosis. It is a C20209T substitution of the 3’UTR region of the FII gene [110].
The MTHFR gene (Gene ID: 4524) is located on chromosome 1 (1p36.22) and consists of 12 exons (https://www.ncbi.nlm.nih.gov/gene/4524). Several transcriptional start sites, alternative splicing and polyadenylation sites have been observed for MTHFR. Transcription start sites are located in two regions, and two promoters have been characterized. The latter contain multiple binding sites for transcription factors [111].
5,10-methylenetetrahydrofolate reductase (MTHFR) is a 150 kDa dimer comprising two isoforms of varying sizes: 77 kDa and 70 kDa. It consists of 656 AA and has two domains: catalytic on the N-terminal side and regulatory on the C-terminal side. The MTHFR protein is a homodimer with a βα structure. Each monomer is formed by 8 alpha helices and 8 beta sheets. It is the cofactor of the flavine adenine dinucleotide (FAD) [111].
MTHFR is a cytoplasmic enzyme found in the spleen, lymph nodes and bone marrow. Dimeric flavoprotein 5,10-methylenetetrahydrofolate reductase (MTHFR) is an NADPH-dependent enzyme that catalyzes the reduction of 5,10-MTHFR, the major carbon donor in nucleotide biosynthesis, to 5-MTHFR, which is the predominant form of folate and the donor of the methyl radical in the reaction of homo-cysteine remethylation to methionine [111].
Indeed, homocysteine is a sulfur-containing amino acid formed during the conversion of methionine to cysteine (demethylation). The catabolism of homocysteine follows two pathways: on one hand, transsulfuration (conversion to cystathionine and then to cysteine) involving cystathionine betasynthase (CBS) and, on the other hand, remethylation (regeneration of methionine) involving methionine synthase (MS) and methylene tetrahydrofolate reductase (MTHFR). These enzymes have as enzymatic cofactors certain vitamins of the B group (B6, folic acid, B12) [112].
The 5,10-methylene tetrahydrofolate reductase (MTHFR) catalyzes the irreversible reduction of 5,10-methylene tetrahydrofolate (CH2THF) to 5-methyltetrahydrofolate (CH3THF). MTHFR activity thus affects the availability of CH2THF, which influences RNA and DNA synthesis. CH3THF is required for the remethylation of homocysteine to methionine (MET), which in turn is involved in protein synthesis and methylation of DNA and other compounds (CH3-X) [113].
Hyperhomocysteinemia may be both a genetic and acquired abnormality. Homocystinuria and hyperhomocysteinemia can be caused by rare inborn errors of metabolism that result in marked elevations of plasma and urine homocysteine concentrations [114].
Genetic polymorphisms result from common mutations that are usually ignored because they are often benign. However, some polymorphisms are not without health consequences. Two SNPs are described for MTHFR: C677T polymorphism and A1298C polymorphism of the MTHFR. Recently, rare variants in MTHFR have been detected by whole exome sequencing in association with the occurrence and the recurrence of pulmonary embolism [115].
In 1995, Frosst et al. [78] identified a C to T substitution of nucleotide 677 that converts an alanine to a valine in 222. This mutation affects the catalytic domain of the MTHFR protein responsible for the generation of a thermolabile enzyme whose enzymatic activity is reduced by half at 37°C and absent at 46°C. This thermolability depends on the transmitted form: in homozygotes, the residual activity is only 18–22% while it is 56% in heterozygotes. On the other hand, the presence of the mutation in the homozygous state alters the metabolism of folates and induces a moderate increase in plasma homocysteine concentrations. The study of the biochemical characteristics of this thermolabile factor revealed a tendency to segregate into monomers as well as the dissociation of its cofactor FAD in solution [116].
The C677T mutation of MTHFR is a common polymorphism in the general population (allelic frequency is 0.38). Its frequency in the homozygous state varies between 1 and 21% with a significant heterogeneous distribution among different ethnic groups [117]. The homozygous TT genotype is particularly prevalent in northern China (18%), eastern Italy (18%) and California (21%). In addition, there is a geographical gradient in Europe (increase from north to south) and China (decrease from north to south). Furthermore, the genotypic frequency is low in African ancestors, intermediate in Europeans and prevalent in Americans [111].
In 1998, Van der Put et al. [118] identified another SNP less frequent than C677T (allelic frequency is 0.33): it is a 1298A-C substitution that converts Glu429 to Ala (E429A) and thus destroys the restriction site for MboII. This mutation affects the regulatory domain of the protein and is associated with a more pronounced reduction in MTHFR enzymatic activity in homozygotes than in heterozygotes. However, the E429A protein is biochemically similar to the normal protein [116].
Protein C (PROC), protein S (PROS1), and antithrombin (Serpinc1) have been demonstrated to play important roles in the anticoagulation process and thrombophilia [69, 72, 119].
PROC gene is located on chromosome 2 (2q14.3) and consists of 8 exons. Gene ontology annotations related to this gene include calcium ion binding and peptidase activity. An important paralog of this gene is PROZ (https://www.ncbi.nlm.nih.gov/gene/5624).
This gene encodes a vitamin K-dependent plasma glycoprotein, produced and secreted by hepatic cells as a zymogen. Along with its cofactor protein S (PS), activated protein C plays the role of an inactivator of the coagulation factors and an important factor of the regulation of the blood clotting pathway. It has a proteolytic effect on of the activated forms of coagulation factors V and VIII (Va and VIIIa). Protein C is a multi-domain glycoprotein composed of a non-catalytic light chain linked to the catalytic heavy chain by a single disulfide bond. The light chain harbors the vitamin K-dependent N-terminal g-carboxyglutamic acid (Gla) domain followed by two epidermal growth factor (EGF)-like domains. The C-terminal catalytic heavy chain with a trypsin-like substrate specificity is preceeded by an activation peptide, which is removed during the activation of protein C by the thrombin- thrombomodulin complex. The encoded protein C is cleaved to its activated form or APC by the thrombin-thrombomodulin complex. APC with the serine protease domain leads to the degradation of the coagulation factors Va and VIIIa in the presence of PS acting as a non-enzymatic cofactor, calcium ions and phospholipids. Protein C exerts also a protective effect on the endothelial cell barrier function [119, 120, 121].
Various conditions have been shown to cause acquired protein C deficiency. These conditions include vitamin K deficiency, warfarin therapy, severe liver disease, disseminated intravascular coagulation, severe bacterial infections in the young, and some chemotherapy drugs [122].
In contrast, inherited protein C deficiency is caused by genetic variations in the PROC gene. Prevalence of hereditary PROC deficiency is estimated at 0.2–0.5%. The milder form is caused by an alteration in one PROC gene and is inherited in an autosomal dominant manner. The severe form is caused by an alteration in both PROC genes (homozygous or compound heterozygotes) and is inherited in an autosomal recessive manner. In the other hand, heterozygous mutations in many adults may be asymptomatic for life but other heterozygous protein C deficiencies are characterized by recurrent venous thrombosis. Individuals with decreased amounts of protein C are classically referred to as having type I deficiency and those with normal amounts of a functionally defective protein as having type II deficiency [123].
PC deficiency is found in 3% of patients with primary venous thromboembolic disease. However, regarding the complex forms of inherited PC deficiency, studies of thrombophilic patients have shown that the prevalence of PC deficiency associated with thrombosis is between 1/16,000 and 1/36,000 [124]. A much higher prevalence of asymptomatic PC deficiency has been shown in a healthy blood donor population (1/200 to 1/700) [125].
Mutations in PROC gene have been long associated with thrombophilia with an increased tendency toward thromboembolic disease risk. In 1981, it was first described by Griffin et al. [80] that hereditary PROC deficiency was responsible of an hypercoagulability state. Hereditary PROC deficiency considered as autosomal dominant by familial studies arises from several distinct mutations in the PROC gene. PROC mutations leading to homozygous deficiency are detected during neonatal purpura fulminans [126].
Protein C database analysis suggests that there are about 380 mutations of PROC gene and that the mutations are scattered on both light and heavy chains and involve all functional domains of the protein (Gla, EGF1, EGF2 and catalytic domains), and recurrent venous thrombosis [127]. ClinVar database records that mention thrombosis and PROC showed 200 genetic variations. PROC variants occurring as the result of these genetic changes can lead to severe intracellular impairments and ineffective PROC release or non-functional PROC release.
PROC gene neighboring sequence contains several transcriptional regulatory regions. Distinct polymorphic loci were identified on promoter region of the human PROC gene. It was shown that polymorphic regions of the PROC gene: -1654C > T, -1641A > G and -1476A > T were associated with deep venous thromboembolism in some countries. Pulmonary embolism incidence in Chinese population seems to be associated with TT phenotype of -1654C > T polymorphism of PROC gene [128].
Recently, it was shown that PC as well as its PS cofactor are not only partners in the anticoagulant system, but also proteins closely involved in the mechanisms of inflammation, apoptosis, and in vascular permeability [129].
PROS1 gene is located on chromosome 3 at 3q11.1 with 16 exons. There are two genes with 98% homology: an active gene with 15 exons spanning more than 80 kb and a non-coding pseudogene b, which is very close to the PSa gene (https://www.ncbi.nlm.nih.gov/gene/5627). This gene encodes Protein S (PS), the major cofactor of PC. It is a single-stranded, vitamin K-dependent glycoprotein of 69 kDa. PS is produced by the liver, but has also been localized in the endothelial cell, the megakaryocyte and the Leydig cell. It is synthesized as a 676 AA precursor comprising a leader sequence eliminated before secretion, a hydrophobic signal peptide, and a propeptide with the carboxylase recognition site analogous to that of other vitamin K-dependent factors. The mature form of PS (635 AA) consists of a GLA domain with 11 GLA residues, a binding peptide, a thrombin-sensitive loop (TSL), four EGF domains, and a carboxyterminal region with areas of homology to the hormone-binding globulin (SHBG) [130, 131, 132, 133].
PS acts to prevent coagulation, mainly by inactivating factors V and VIII. PS increases the affinity of PCa for negatively charged phospholipids, forming a membrane-bound PCa-PS complex that makes factors Va and VIIIa more accessible to cleavage by PCa. PS circulates in the plasma partly under the influence of PCa. Free form (40% of circulating PS) is active in the coagulation system. Whereas, 60% is in the complexed form with C4b-binding protein (C4bBP), a protein of the complement system that binds PS at the SHBG domain. C4bBP-bound PS has no cofactor effect on PCa [131].
Other mechanisms of action independent of PC have been suggested for PS but their physiological importance is not firmly established; in particular, PS may have direct anticoagulant activity through its ability to bind and inhibit factors Xa, Va, and VIIIa and to compete with procoagulant factors for binding to phospholipids. It may also stimulate inhibition of the tissue factor pathway inhibitor or TFPI.
PS deficiency is found in 2–3% of thrombophilic patients. The prevalence in the general population may be in the range of 0.05% to 0.1% [130].
Antithrombin belongs to the serine protease inhibitor superfamily: the serpins. It exerts its physiological function by inhibiting procoagulation factors, such as thrombin, factor Xa, factor IIa, and other factors of the blood coagulation system. It contributes to the regulation of clot formation both by inhibiting thrombin activity directly and by interfering with earlier stages of the clotting cascade [134].
Antithrombin (AT) is a single-stranded plasma glycoprotein with a molecular weight of 58 kDa and 432 amino acids (AA) and four oligosaccharide side chains. AT is synthesized by the liver. It mainly inactivates thrombin and activated factor Xa, but also, in the presence of heparin, factors VIIa, XIa and XIIa [135].
Inactivation of the protease involves the formation of an irreversible bond between the active site of the enzyme and the reactive site of the inhibitor, formed by Arg 393 and Ser 394 (P1-P1’). The AT acts as a pseudosubstrate for the enzyme. Indeed, cleavage of the P1-P1’ linkage induces a major conformational change in the AT, which can then form a stable complex with the target protease by incorporation of the AAs located upstream of Arg 393 into a b-sheet structure consisting of five strands in the uncleaved form and six strands in the cleaved form, with the sixth strand being the P1-P14 segment [136].
Inhibition of the enzyme by AT is catalyzed by heparin and proteoglycans of the vascular endothelium. This interaction accelerates thrombin inhibition by a factor of approximately 2000. In the presence of heparin, the AT reactive site loop is more exposed at the protein surface and more readily fits the catalytic site of certain activated factors such as factor Xa [137]. In the case of thrombin, which like AT has binding sites for heparin, a ternary complex is formed that brings the enzyme closer to its inhibitor. The heparin-binding domain of AT comprises the region of AA 41–49 on the one hand and AA 107–156 on the other. Both regions are rich in basic AAs that can interact with the sulfate groups of heparin. They are similar in the tertiary structure of the protein [138].
SERPINC1 is the gene encoding antithrombin. It is located on chromosome 1 at 1q25.1 with 9 exons. There are ten Alu sequences in the introns, representing 22% of the intronic sequences, four times more than in the entire human genome. These repetitive elements may contribute to the occurrence of many mutations and deletions in the gene (https://www.ncbi.nlm.nih.gov/gene/462).
Antithrombin deficiency, a rare autosomal dominant disorder (MIM#107300), is caused by rare genetic variations of SERPINC1 gene. There are two types of antithrombin deficiency. In type I antithrombin deficiency, functional and antigenic levels are proportionally decreased. In type II antithrombin deficiency, antigenic levels are normal while the functional activity is abnormal. In around 0.02–0.25% of a healthy population with antithrombin deficiency, there is a 5- to 50-fold increased risk of developing venous. AT deficiency is found in 1–2% of patients with primary venous thromboembolic disease. The prevalence of symptomatic AT deficiency in the general population is between 1:2000 and 1:5000 [139].
The first variation linked to antithrombin deficiency was characterized in 1983 and, to date, more than 200 variants have been reported to be associated with the risk of thrombosis. The homozygous variant (Phe229Leu) of SERPINC1 leading to spontaneous antithrombin polymerization in vivo has been shown to be associated with severe childhood thrombosis [140]. The heterozygous variant is mainly associated with a high risk of venous thrombosis [141].
However, most of SERPINC1 genetic variants (currently 399 different mutations reported) are rare, usually found in a single family baptized as private or orphan and occasionally discovered in more than one population. For example, in a Dutch population, Bezemer et al. [142] reported the 5301G > A polymorphism of SERPINC1 gene, to be associated with the risk of venous thrombosis. The frequencies of this rs2227589 polymorphism were around 0.10 and 0.329 in the East Asian population. In Spanish Caucasian population, it was shown the presence of a functional effect of the 5301G > A on antithrombin levels [143]. All of these conclusions were debated in different other studies [139].
Although thrombophilia can be identified in about half of all patients presenting with venous thrombosis, genetic testing or screening for hereditary thrombophilia is indicated only in selected cases [144, 145].
This chapter has focused on thrombosis-related genetic polymorphisms, particularly the variations of hemostatic genes involved in classical inherited thrombophilia diseases. They are the earliest and the most studied polymorphisms in the field.
Despite the increasing knowledge about thrombosis-related genetic polymorphisms, genetic testing for inherited thrombophilia remains considered, most often, not helpful to guide clinical decisions and not recognized on a routine basis.
The current knowledge of the contribution of thrombosis-related genetic polymorphisms showed an accumulation of understanding over the years for more than half a century that has led to robust results regarding their roles in thrombotic disorders and their potential clinical consideration, particularly as genetic markers of the diseases.
Despite their recognition as risk factors with well-established frequencies and sufficiently convincing associations, the implementation of the genetic testing as diagnosis/prognosis tools failed to attain an international consensus for clinical application. In fact, even though, genetic and genomic testing and screening are expected to have a greatly increased role in healthcare with a gradually likely to be ordered in routine for many diseases, genetic test reports in thrombosis miss the ability to deliver with the results, their clinical implications clearly and unambiguously. Guidelines and recommendations on thrombosis related genetic polymorphisms laboratory analysis remained limited to a narrow range of specific clinical situations and patients and are not uniform worldwide. The conditions under which genetic testing for thrombophilia have been in fact defined, were engaged, validated and published by some working groups and medical associations [144, 145, 146, 147, 148, 149, 150, 151, 152, 153].
Furthermore, literature review showed that the AT, PC and, PS deficiencies, as well as FV Leiden, prothrombin mutation and MTHFR polymorphisms mentioned above, are considered as having an increased risk for venous thrombosis but have little or no effect on arterial thrombosis. In fact, the available evidence indicates that Leiden FV variant is not a major risk factor of any sort in arterial thrombosis and micro thrombosis, including myocardial infarction and strokes. The same conclusions were demonstrated for the other thrombophilia polymorphisms [154, 155, 156]. However, hyperhomocysteinaemia is still considered as a mixed risk factor for both arterial and venous thrombosis [1, 154].
Additionally, analysis of the literature revealed the description of several other polymorphisms that predisposes to the development of thrombosis, mainly those involving the hemostatic pathway factors like fibrinogen, factors VIII and VII, factor XIII, activated protein C receptor, thrombomodulin, plasminogen activator inhibitor, tissue plasminogen activator, Thrombin-activatable fibrinolysis inhibitor and platelet receptors (GPIIb-IIIa, GPIb-IX-V, GPIa-IIa, GPVI and others) etc… Two exhaustive reviews reporting these polymorphisms and especially their clinical significance were identified [146, 157].
In contrast, there is little clarity in relation to arterial thrombotic disease and the initial promise that genetic risk factors might contribute appreciably to an explanation of the development of arterial thromboses has largely been unfulfilled. As well, the expectations raised by early reports of positive associations have been tempered by inconsistent results with almost the majority of the studied hemostatic genes. In reality, the most consistent associations that have been found involve fibrinogen and the factor XIII [146]. Recently, most association studies of arterial thrombosis-related genetic polymorphisms are focused more much towards genes and factors involved in the other pathogenic pathways leading to thrombosis, i.e., inflammatory, immune and oxidative pathways.
Interrogation of the NCBI ClinVar database with an inquiry linking polymorphism and thrombosis revealed more than 3500 variations. The pathogenicity and the cause-and-effect relationship of these genetic variations was not strongly validated in the majority of cases. Most of related studies involved limited number of patients with untested statistical associations on a large scale. Additionally, some of the problems in identifying causal genetic markers are related to difficulties associated with the precise definition of the clinical phenotype under study. The sampling of patients in the studies was characterized by obvious heterogeneity both in terms of pathologies and in terms of the physiopathogenic origins of considered thrombosis. Indeed, there are many problematical uses of the terminology and other difficulties regarding the disorders stratification and the thrombosis typology. These difficulties of clinical and biological heterogeneity limit fundamentally the statistical homogeneity of the studied subgroups and the comparative effectiveness during the associative relationship approaches.
To overcome these shortcomings and to reach effective associations, several other technical and biological obstacles must be considered and defeated.
Translational medicine and research findings in the field of polymorphisms during thrombotic disorders are promising by the use of omics approaches and genome-wide association analysis, which will permit the identification of new risk loci. They will provide mechanistic insights into the genetic pathogenesis of thrombotic entities and put on view greater overlap among venous, arterial and microvascular thrombotic disorders than previously thought. The next step will be at the interactomic level to disclose binary and complex interactions between genes, factors and actors of thrombosis pathways. Indeed, it has been evident through this review that there are permanent interactions between the different pathogenic factors at the origin of thrombosis and almost permanent functional dualities for each factor under the influence of the dynamic homeostatic states of the organism and of the cells facing various situations to establish adaptive equilibriums. The importance of environmental influences and the complexity of the processes involved in vascular thrombotic disease suggest another myriad of other interacting metabolic factors. This understanding further increases the importance of lifelong risk interactions and may suggest an explanation for some of the inconsistencies in case–control studies. It is also important to consider that studies of population genetics of polygenic disorders, such as thrombotic disease, would ideally require prior knowledge of the relationship between the protein level/receptor density and disease, the degree of heritability of variance in the plasma levels of the protein/receptor density, and the genetic determinants of heritability.
It should be emphasized that despite the difficulties delaying the approval of genetic polymorphisms as reliable markers of thrombotic disorders, some of them have already been integrated into the preventive approaches of precision medicine, while others could be adopted in the near future in the predictive approaches of precision medicine.
Finally, it is important to mention that the most advantageous achievements of the studies on the associated thrombosis genetic variations are perceived through the pharmaceutical and biotechnological industries discovers in the field of thrombosis. These progresses on drug discoveries during the past, the present and the future are closely related to the deep understanding of the pathogenic mechanisms of thrombosis as well as their complex interplay.
Nouha Bouayed Abdelmoula and Balkiss Abdelmoula declare they have no conflict of interest.
With the increasing demand for herbal medicinal products, nutraceuticals, and natural products for primary healthcare worldwide, medicinal plant extract manufacturers and essential oil producers have started using the most appropriate extraction techniques. Different methods are used to produce extracts and essential oil of defined quality with the least variations.
Herbs and medicinal plants have been used for centuries as source of a wide variety of biologically active compounds. The plant crude material or its pure compounds are extensively used to treat diverse ailments by generations of indigenous practitioners [1, 2]. They are currently the subject of much research interest, but their extraction as part of phytochemical and biological investigations presents specific challenges that must be addressed throughout the solvent extraction [3]. Natural products provide unlimited opportunities for new drug discovery because of the unmatched availability of chemical diversity [4]. Thanks to two drugs derived from alkaloids of Madagascar’s rosy periwinkle (
Natural products are currently of considerable significance due to their unique attributes as a significant source of therapeutic phytochemicals and their efficacy, safety, and minimal side effects [2, 8]. Bioactive compounds in plants include alkaloids, terpenoids, coumarins, flavonoids, nitrogen-containing compounds, organosulfur compounds, phenolics, etc. A wide spectrum of bioactivities is exhibited by these compounds such as anti-inflammatory, immunostimulatory, anticancer, antioxidant, antimicrobial, etc.
Research on medicinal plants is particularly important as that on conventional drugs due to the beneficial phytochemicals from plants and the shift towards natural products in pharmaceutical and cosmeceutical industries. Chemical structures of a few essential bioactive compounds isolated from plants are presented in Figure 1 [9, 10, 11, 12, 13, 14].
Chemical structures of a few important bioactive compounds isolated from plants.
Extraction of the bioactive constituents from plants has always been challenging for researchers [15]. As the target compounds may be non-polar to polar and thermally labile, the suitability of the extraction methods must be considered. The study on medicinal plants starts with extraction procedures that play a critical role in the extraction outcomes and the consequent assays.
Hence, this chapter aims to provide an overview of the process of plant extraction, describe, and compare extraction methods based on their principle, the effect of solvent on extraction procedures, strength, limitations, and economic feasibility, with their advantages and disadvantages. This chapter shall also emphasize the common problems encountered and methods for reducing or eliminating these problems. Since millions of natural products derived from plants are known, only selected groups and compounds are presented.
The term “medicinal” as applied to a plant indicates that it contains a substance or substances which modulate beneficially the physiology of sick mammals, and man has used it for healthful purpose [16]. Medicinal plants were described by Farnsworth and Soejarto as: “all higher plants with medicinal effects that relate to health, or which are proven as drugs by Western standards, or which contain constituents that are defined as hits.” [17].
Medicinal plant (MP) refers to any plant which, in one or more of its organs, contains substances that can be used for therapeutic purposes or which are precursors of the synthesis of valuable drugs. A whole plant or plant parts may be medicinally active [18, 19, 20, 21, 22]. Medicinal plants (MPs) are becoming very important due to their uses mainly as a source of therapeutic compounds that may lead to novel drugs. MPs are plants that are used for healthcare purposes in both allopathic and traditional medicine systems. MPs cover various species used including condiments, food aromatic and cosmetics [23, 24, 25, 26].
Herbs may be defined as the dried leaves of aromatic plants used to impart flavor and odor to foods with, sometimes, the addition of color. The leaves are commonly traded separately from the plant stems and leaf stalks [27].
Herbal medicine is referred to as medicinal preparations comprising active ingredients obtained from the herbal plant. The product can be made from the whole plant or any part. Preparations from by-product herbal plants such as oil, gum, and other secretions are also considered herbal medicines [18, 19, 22].
Metabolites are intermediate processes in nature and are small molecules. Primary metabolites are known vital or essential compounds and are directly involved in the average growth, development, and reproduction of plants [28]. Primary metabolites include cell constituents (e.g. carbohydrates, polysaccharides, amino acids, sugars, proteins, and lipids) and fermentation products (ethanol, acetic acid, citric acid, and lactic acid), and are mainly used during their growth and development stages [19, 22, 29, 30].
Secondary metabolites are not directly involved in those processes and usually have a function but are not that important for the organism (e.g. phenolic, steroids, lignans, etc.). They are found only in specific organisms or groups of organisms, and express of the individuality of species [19, 30, 31]. They are not necessarily produced under all conditions, and most often, the function of these compounds and their benefit to the organism is not yet known. Some are undoubtedly made for readily appreciated reasons, e.g., as toxic material providing defense against predators, as volatile attractants towards the same or other species, but it is logical to assume that all do not play some vital role for the well-being of the producer [27, 30]. Secondary metabolites are produced after the growing stage and are used to increase the ability of plants to survive and overcome their local challenges. Bioactive compounds are classified as terpenoids, alkaloids, nitrogen-containing compounds, organosulfur compounds, and phenolic compounds [29].
Bioactive compounds are reported to possess diverse bioactivities such as antioxidant, anticancer, antimalarial, antiulcer, antimicrobial, anti-inflammatory activity [32, 33, 34, 35, 36].
The definition of bioactive compounds remained ambiguous and unclear for a long time. Very few references describe the term “bioactive”. It is composed of two words
A plant extract is a substance or an active substance with desirable properties removed from the tissues of a plant, frequently by treating it with a solvent, to be used for a particular purpose. The term “bioactive compounds” is generally referred to as biologically significant chemicals but not established as essential nutrients [43]. Bioactive compounds are essential (e.g., vitamins) and non-essential (e.g., polyphenols, alkaloids, etc.) compounds that occur in nature, are part of the food chain, and can affect human health [44]. They are derived from various natural sources such as plants, animals, microorganisms (e.g., fungi) and marine organisms (e.g., lichens) [2]. The amount of bioactive natural products in natural sources is always fairly low [45, 46]. Plant active compounds are usually contained inside plant matrixes. Active compounds are synthesized in small quantities and different concentrations in all plant organs or parts such as leaves, roots, barks, tubers, woods, gums or oleoresin exudations, fruits, figs, flowers, rhizomes, berries, twigs, as well as the whole plant. Further processes may be required after extraction to purify or isolate the desired compounds.
Fresh and dried samples are used and are reported in the literature in the preparation of medicinal remedies. Ideally, fresh plant tissues should be used for phytochemical analysis, and the material should be plunged into boiling alcohol within minutes of its collection. Alternatively, plants may be dried before extraction [47]. In most reported cases, dried materials are preferred considering their long conservation time compared to fresh samples. Furthermore, fresh specimens are fragile and tend to deteriorate faster than dried ones. Phytoconstituents such as Essential Oils (EOs) are found in fewer dried samples than in fresh samples. In case of fresh plant material extraction using organic solvents such as methanol or ethanol, is required to deactivate enzymes present in the plant sample. The extractive might contain a substantial portion of water; hence it can be partitioned using specific immiscible organic solvents [3].
Drying is the most common method to preserve the plant material from enzymatic degradation, such as hydrolysis of glucoside, etc. It should be dried as quickly as possible in the open room under primitive conditions at ambient room temperature with air circulation around the plant material to avoid heat and moisture [47]. However, they placed in shallow trays with good atmospheric air-up dryness either in the sunshine or in shade depending on nature of the indicated or identified constituents. However, direct sunlight is usually avoided to reduce the possibility of chemical reactions, responsible for forming of the artifact that may result from chemical transformations after exposure to ultraviolet radiation. Alternatively, plant materials should be dried under optimum temperature conditions between 40 and 50°C, or they can be dried in the oven if needed. Generally, plant material is dried at temperatures below 30°C to avoid the decomposition of thermolabile compounds [3]. Plants containing volatile or thermolabile components may be lyophilized (freeze-dried). In freeze-drying the frozen material is placed in an evacuated apparatus with a cold surface maintained at −60 to −80°C. Water vapors from the frozen material then pass rapidly to the cold surface to yield the dry material [8, 48].
Lowering particle sizes increase surface contact between samples and extraction solvents and therefore, increase the yield rate and yield. Grinding resulted in coarse smaller samples, meanwhile, powdered samples gave a more homogenized and smaller particle, leading to better surface contact with solvents used for extraction. Before the extraction, pretreatments such as drying and grinding of plant materials are usually conducted to increase the extraction efficiency [48]. It is essential that the particles are of as uniform size as possible because larger particles take a longer time to complete the extraction process [49]. Usually, solvent molecules most contact the larger analytes, and particle size smaller than 05 mm is ideal for efficient extraction [8]. Conventional methods are usually used to reduce the particle size of dried plant samples viz. mortar and pestle or electric blenders and mills, etc.
Extraction is separating the medicinally active mixture of many naturally active compounds usually contained inside plant materials (tissues) using selective solvents through the standard procedure [50]. It can also be defined as the treatment of the plant material with solvent, whereby the medicinally active constituents are dissolved and most of the inert matter remains undissolved. Thus, the purpose of all extraction is to separate the soluble plant metabolites, leaving behind the insoluble cellular marc known as residue [8]. The obtained product is a relatively complex mixture of metabolites, in liquid or semisolid state or (after removing water) in dried powder form, and are intended for oral and/or external uses. Extraction is based on the difference in solubility between the solute, other compounds in the matrix, and the solvent used to stabilize [29].
In general, there are three common type of extractions: liquid/solid, liquid/liquid and acid/base [51]. The extraction of these active compounds needs appropriate extraction methods that consider the plant parts used as starting material, the solvent used, extraction time, particle size and the stirring during extraction [52, 53]. Extraction methods include solvent extraction, distillation method, pressing, and sublimation according to the extraction principle. Solvent extraction is the most widely used method [47].
The solvent used, the plant part used as starting material and the extraction procedure are three basic parameters reported that influence the quality of an extract [15]. Proper extraction procure is the first step towards isolating and identifying the specific compounds in crude herbal material. It plays a significant and crucial role in the outcome. Successful extraction begins with careful selection and preparation of plant sample and thorough review of the appropriate literature for indications of which protocols are suitable for a particular class of compounds or plant species [3]. For instance, if the components are volatile or prone to degradation, they can first be frozen and homogenized with liquid nitrogen [29]. The extraction, in most cases, involves soaking the plant material in solvent for some specific time. Reported properties on an excellent extraction solvent include low toxicity, preservative action, ease of evaporation at low heat, promotion of rapid physiologic absorption of the extract, and inability to cause the extract to be complex or dissociate.
The principle of solid–liquid extraction is that when a solid material comes in contact with the solvent, the soluble components in the solid material are dissolved in, and move to the solvent. In solvent extraction, the mass transfer of soluble ingredients to the solvent takes place in a concentration gradient. The mass transfer rate depends on the concentration of ingredients, until equilibrium is reached. After that, there will no longer be a mass transfer from plant material to the solvent. In addition, heating the solvent can also enhance the mass transfer because of better solubility.
Moreover, the concentration gradient changes if fresh solvent replace the solvent equilibrium with the plant material [50]. Properties required for an excellent extracting solvent (or a mixture of solvents) include removal, inert, non-toxic, free from plasticizers, not easily inflammable, and no or less chemical interaction [53]. The selection of solvent is therefore crucial for solvent extraction. Solubility, selectivity, cost, and safety should be taken into account in selecting solvent [47]. The factors affecting the choice of solvent are quality of phytochemicals to be extracted, rate of extraction, diversity of metabolites extracted, the toxicity of the solvent in the bioassay process, and the potential health hazard of the extractants and ease of subsequent handling of the extract. Obtaining maximum yield and the highest quality of the targeted compounds is the central goal of the extraction process [29]. Extraction methods are usually chosen per the properties of targeted active compounds, the water content of the plant material, and the objectives of extraction. Initially, natural bioactive compounds are extracted using various extraction techniques, and their bioactivities are identified using
Various conventional (classical) and non-conventional (innovative) methods can extract plant materials. Variation in extraction procedures usually depends on key factors as extraction time, the temperature used, the particle size of tissues, the solvent-to-sample ratio, the pH of the solvent.
The commonly employed extraction methods (long been used) are primarily based on liquid–solid extraction. They are ordinarily easy to operate and are based on heat and/or solvents with different polarities.
This process is conducted by soaking the plant materials (coarse or powered) in a closed stoppered container in a solvent allowed to stand at room temperature for 2–3 days with frequent stirring to obtain plant extracts. A sealed extractor is used to avoid solvent evaporation at atmospheric pressure. The process is intended to soften and break the plant’s cell walls to release the soluble phytoconstituents. The mixture is then pressed or strained by filtration or decantation after a specific time [8, 54]. Maceration is the simplest and still widely used procedure. The extraction procedure in this stationary process works on principle of molecular diffusion, which is a time-consuming process. Maceration ensures dispersal of the concentrated solution accumulation around the particles’ surface and brings fresh solvent to the surface of particles for further extraction [46].
This is a kind of maceration in which gentle heat is applied during the maceration extraction process. The temperature does not alter the active ingredients of plant material, so there is greater efficiency in the use of menstruum (solvent or mixture of solvent used for extraction). It is used when the moderately elevated temperature is not objectionable and the solvent efficiency of the menstruum is increased thereby [15]. The most used temperatures are between 35 and 40°C, although it can rise to no higher than 50°C. The plant part to be extracted is placed in a container with the pre-heated liquid to the indicated temperatures, is maintained for a period that may vary between half an hour to 24 hours, shaking the container regularly. This process is used for the herbal material or plant parts that contain poorly soluble substances or polyphenolic compounds [49].
Infusion is a simple chemical process used to extract plant material that is volatile and dissolves readily or release its active ingredients easily in organic solvents [49]. Infusion and decoction use the same principle as maceration; both involve soaking the plant material in boiled or cold water which is then allowed to steep in the liquid. The maceration time for infusion is, however shorter. The liquid may then be separated and concentrated under a vacuum using a rotary evaporator.
Infusion finds its application in tea preparation and consumption prescribed in psychophysical asthenia, diarrhea, bronchitis, asthma, etc. In Tropical Africa, the infusion of the bark of
The word “lixiviation” (comes from the Latin lixivium, “lessive”.) The extraction is carried out with cold or boiled, fresh and new solvent, always. Extraction of components is done using water as solvent.
The current process involves boiling the plant material in water to obtain plant extracts. Heat is transferred through convection and conduction, and the choice of solvents will determine the type of compound extracted from the plant material [8]. The sample is boiled in a specified volume of water for a defined time (15 to 60 minutes.) It is then cooled, strained, filtered, and added enough water through the drug to obtain the desired volume. This method is suitable for extracting thermostable (that does not modify with temperature) and water soluble compounds, hard plant materials and commonly resulted in more oil-soluble compounds than maceration.
It is the extraction of plant material in alcohol. Usually, the plant material (fresh) and ethyl alcohol are taken at the ratio of 1:5. Because of the alcohol content, the tinctures can be stored at room temperatures without decomposing [55].
It is conducted by passing the boiled solvent through the plant material at a controlled and moderate rate (e.g. 5–7 drops per min) until the extraction is complete before evaporation. The concentrated plant extracts are commonly collected at the bottom of the vessel. To obtain a significant amount of extract, successive percolations can be performed by refilling the percolator with fresh solvent and pooling all extracts together. This procedure is mostly used to extract active compounds in the preparation of tinctures and fluid extracts. Its major disadvantage is that large volumes of solvents are required, and the procedure can be time-consuming and may require skilled persons [49].
Steam and hydrodistillation methods are usually used to extract volatile compounds, including essential oil, insoluble in water, from various aromatic and medicinal plants. This is conducted by boiling the plant materials in water to obtain EOs after vapor condensation. Steam distillation occurs at a temperature lower than the boiling point of the ingredients. The method is useful for thermos-sensitive bioactive compounds e.g., natural aromatic compounds. The heat leads to breakage in the sample’s pores and then enables the release of the target compound from a matrix. As Raoult’s law states that while mixing two immiscible liquids, the boiling point will be reduced. Therefore, in the mixture of volatile compounds having a boiling point between 150 and 300°C and water having a boiling point at about 100°C (at atmospheric pressure), the mixture evaporation will be getting closer to that of the water [29, 56].
There are similarities between the hydrodistillation and the steam distillation principles. In brief, plant material is immersed in water or a proper solvent followed by heating to boiling under atmospheric pressure in the alembic. In a condenser, EOs vapors and water undergo a liquefaction process, and EOS are then separates from water/solvent after collection of the condensate in the decanter. The principle of extraction is based on isotropic distillation. Hydrodistillation with water immersion, direct vapor injection, and water immersion and vapor injection are the three main types of hydrodistillation. The distillation time depends on the plant material being processed [56].
In this method, finely ground sample is placed in a porous bag or “thimble” made from a strong filter paper or cellulose, set in the thimble chamber of the Soxhlet apparatus. The first Soxhlet apparatus was developed in 1879 by Franz von Soxhlet (Figure 2) [58]. Extraction solvents are heated in a round bottom flask, vaporized into the sample thimble, condensed in the condenser, and dripped back. When the liquid content reaches the siphon arm, the liquid content is emptied into the bottom flask again, and the process is continued [8]. The disadvantages include no possibility of stirring, and a large amount of solvent is required. This method is unsuitable for thermolabile compounds as prolonged exposure (long extraction time) to heat may lead to their degradation. It constitutes an official classical method used to determine different foods’ fat content [15, 29, 57].
Experimental Soxhlet extraction apparatus [
Exposure to hazardous and flammable liquid organic solvents are the most noticed disadvantages in this method, and the high purity of extraction solvents needed may add to the cost. Also, shaking or stirring cannot be provided in the Soxhlet device to accelerate the process [57].
However, it requires a smaller quantity of solvent as compared to maceration. Besides, instead of many portions of warm solvent passing through the sample, just one batch of solvent is recycled. Other advantages of this technique include its simple operational mode, its applicability to a higher temperature that increases the kinetics process, its low capital cost, the absence of filtration, and the continuous contact of the solvent and the sample. It maintains a relatively high extraction temperature with heat from the distillation flask [29, 57, 59].
It is a standard extraction procedure that involves successive extraction with various solvents of increasing polarity from non-polar to polar ones. The aim is to ensure that a broad polarity range of compounds could be extracted [15].
Some medicinal preparations adopt the technique of fermentation for extracting the active principles. The extraction procedure involves soaking the crude drug, either a powder or a decoction, for a specified period. Alcohol is generating
Hydrodistillation and steam distillation, hydrolytic maceration followed by distillation, expression and effleurage (cold fat extraction) may be employed for aromatic plants. Some of the latest extraction methods for aromatic plants include headspace trapping, solid phase micro extraction, protoplast extraction, micro distillation [15].
These techniques are the easiest and simplest methods. Despite the establishment of advanced extraction methods, the potential of conventional solid–liquid extractions is still being used to obtain active compounds from plants. These methods are criticized due to large solvent consumption and long extraction times that can destroy some metabolites. Solvents used in these techniques for soaking play a critical role. Many other advanced extraction methods that incorporate various technologies have been developed [8, 48].
There is steady progress in the development of extraction technology in recent years. They are also known as advanced techniques with the most recently developed.
Microwaves are part of the electromagnetic spectrum of light with a range of 300 MHz to 300 GHz, and wavelengths of these waves range from 1 cm−1 to 1 m−1 [60]. These waves are made up of two perpendicular oscillating fields which are used as energy and information carriers.
In this extraction process, the use of microwave energy results in faster heating. Due to the exposure of each molecule to the microwave field, its direct effects include, thermal gradients reduction, volume generation due to heat, equipment size reduction, because of the higher process rates, and thus increase in productivity, through better usage of the same equipment process volume [61]. MAE is a feasible green solvent extraction procedure as it uses water or alcohol at elevated temperature and controlled pressure conditions (Figure 3).
Schematic representation of microwave-assisted extraction equipment [
This procedure has demonstrated various benefits like ease to handle and understand steadiness. Many studies reported that MAE has higher yields and is significantly faster than conventional methods for extracting active substances from plant materials [48, 54, 62]. MAE can be presented as a potential alternative to the traditional soli-liquid extraction techniques. A few of the potential advantages are as follow:
a lesser amount of solvent is required (few milliliters of solvent can be used);
shorter extraction time, from few seconds to few minutes (15–20 min);
improved extraction yield;
favorable for thermolabile constituents;
heavy metals and pesticides residue which is present in the trace can be extracted from a few milligrams of plant sample;
during extraction, it provides a stirring, by which the mass transfer phenomenon is improved [54, 60, 62, 63].
MAE intensification needs special equipment to be functional, and electricity produces waves, leading to higher investments and higher operating costs than conventional methods [64]. Banar and collaborators extracted the bioactive compounds from
This extraction method involves using ultrasound with frequencies ranging from 20 to 2000 KHz; this increases the permeability of cell walls and produce cavitation. Although the process is helpful in some cases, its large-scale application is limited due to its high cost. The most noticeable disadvantage of the procedure is the occasional but known deleterious effect of ultrasound energy on the active components of the medicinal plants through the formation of free radicals and consequently undesirable changes on the drug molecules [50]. The schematic representation of the equipment is given below (Figure 4).
Schematic representation of an ultrasound-assisted extraction equipment.
Factors that affect the efficiency of UAE are extraction time, power, solvent, Liquid/Solid (L/S) ratio, plant material, frequency, amplitude, and intensity. UAE more advantageous than other advanced extraction methods and provided the best mass and heat transfer efficiency, lowest energy consumption and carbon emission. It was reported to yield high total phenolic content, antioxidant activity, or specific active compounds [62, 66].
Pressurized liquid extraction (PLE) also known as pressurized fluid extraction (PFE), accelerated solvent extraction (ASE), and pressurized solvent extraction (PSE), or as enhanced solvent extraction system (ESE) [67].
Dionex Corporation introduced PLE in 1995 as an alternative to maceration, percolation, sonication, Soxhlet extraction, etc. It is an automated technique for extracting solid samples with liquid solvents (either aqueous or organic, single or mixtures) above their boiling point, combine high pressures (4–12 MPa) and moderate to high temperatures (50–300°C) [68]. When water is the extraction solvent, different terms are used to define the method, that includes hot water extraction (HWE), subcritical water extraction (SWE), high-temperature water extraction (HTWE), hot water extract pressurized (PHWE), liquid water extraction or superheated water extraction [67]. Sample size, solvent, pressure, temperature, pH, flow rate, extraction time are the standard parameters influencing the PLE process, with temperature and solvent type being the most significant ones [69, 70, 71].
In this process, for a short period of time (5–10 min), a cartridge in which the ample has been placed is filled with an extracting solvent and used to statically extract the sample under elevated temperature and pressure. To purge the sample extract from the extraction cell into a collector flask pressurized gas is used (Figure 5) [68].
Scheme of pressurized liquid extraction equipment [
To increase the efficiency of this extraction process, environmentally friendly liquid solvents are used at moderate to elevated temperature and pressure [72]. The increased temperature causes dramatic changes in the physical–chemical properties of water, enhances the analytes’ solubility, breaks matrix-analyte interactions achieving a higher diffusion rate, and accelerates the extraction process by increasing the diffusivity of the solvent. The increased pressure in contrast, keeps the solvent in a liquid state without boiling and forces the solvent to penetrate the matrix pores [55, 73, 74, 75].
The main advantages of this technique are: (i) faster extraction from 15 to 50 min, (ii) low quantity of solvents (15–40 mL), and no filtration is required. However, costly equipment and the need for a throughout optimization of variables to avoid a matrix-dependent efficiency are the main demerits [72, 73, 74].
SFE is used for separating components from the matrix with the application of supercritical fluids as the extracting solvent (Figure 6) [30].
Schematic diagram of supercritical fluid extraction (SFE) set-up [
Using CO2 as the extracting fluid has many advantages. Besides, its lower boiling point (31°C) and its critical pressure (74 bar). Moreover, carbon dioxide is abundant in nature, safe and inexpensive. But while carbon dioxide is the preferred fluid for SFE, it possesses several polarity limitations. When extracting polar solutes and when strong analyte-matrix interactions are present solvent polarity is crucial. Carbon dioxide fluid is usually mixed with organic solvents to alleviate the polarity limitations (Figure 7) [2].
Schematic representation of a supercritical fluid extraction (SFE) system [
The SFE extraction procedure possesses distinct advantages:
the extraction of constituents is carried out at a low temperature, strictly avoiding damage from heat and some organic solvents. SFE offers gentle treatment for heat-sensitive material;
fragrances and aroma remain unchanged;
CO2 is an inexpensive solvent;
No solvent residues are left behind;
possibility of direct coupling with analytical chromatographic techniques such as gas chromatography (GC) or supercritical fluid chromatography (SFC);
environmentally friendly extraction procedure. CO2 as the solvent does not cause environmental problems and is physiologically harmless, germicidal, and non-flammable.
Some specific disadvantages of this method are:
high investment cost;
the use of high pressures leads to capital costs for the plant, and operating costs may also be high, so the number of commercial processes utilizing supercritical fluid extraction is relatively small, due mainly to the existence of more economical methods;
high polar substances (sugars, amino acids, inorganic salts, proteins, etc.) are soluble;
phase equilibrium of the solvent/solute system is complex and making design of extraction conditions is difficult.
SFE finds extensive application in extracting pesticides, environmental samples, foods and fragrances, essential oils, polymers, and natural products [50, 77]. Conde-Hernández and collaborators extracted the essential oil of rosemary (
Pulsed electric field extraction is a technique based on the exposure of vegetable matrix to an electrical potential. A transformer generates an electric pulse, increasing voltages from 140 or 220 V to 1000 V, or even greater than that (25000 V). A capacitor transforms this high voltage in a closed chamber with metallic electrodes. The general scheme of PEF equipment is presented in Figure 8 [80].
General scheme of a PEF equipment process.
This “cold” extraction assisted by PEF prevent the degradation of the cell and the extraction of components from the intracellular vacuoles [81]. It considerably increases the yield and decreases the time because it can increase mass transfer by destroying membrane structures during the extraction process.
Specific energy input, treatment temperature and field strength are considered among parameters that can influence the treatment efficacy of the PEF extraction. It is known as a non-thermal method which reduces the decomposition of the thermolabile components [47].
The EAE is an enzymatic pre-treatment that is carried out by the addition of specific hydrolyzing enzymes during the extraction step. In the cell membrane and cell wall structure, micelles are formed by macromolecules such as polysaccharides and protein. The coagulation and denaturation of proteins at high temperatures during extraction are the main barriers to extracting natural products. EAE enhance the extraction efficiency due to the hydrolytic action of the enzymes on the components of the cell wall and membrane and the macromolecules inside the cell, which facilitate the release of the natural products. Cellulose, α-amylase, and pectinase are hydrolyzing enzymes usually employed in EAE [47, 82]. This procedure is suitable for extracting various bioactive substances from plant matrices, but after filtration the obtained fraction is rich in small water-soluble molecules that include polyphenols and flavonoids [82].
Turbo-distillation was patented in 1983 by Martel, and has been used in several companies as an industrial purpose for extracting EOs from hard matrixes (such as wood, bark, and seeds) [83]. The extraction process is similar to hydrodistillation with slight modifications [84]. The turbo-extraction or turbolysis is based on extraction with stirring and simultaneous reduction of particle size. Due to of high shearing force, cells disruption leads to rapid dissolution of the active constituents. It results in an extraction time of the order of minutes and the plant content is almost completely depleted [85]. Compare to hydrodistillation, turbo-distillation minimize extraction time and energy consumption and prevents the degradation of volatile constituents (Figure 9) [84].
Laboratory turbo-Clevenger: (a) schematic, (b) bench apparatus. The vessel (1); the rotor (2); the turbo shredder (3); the thermometer (4); the distillation column (5); the condenser (6); the receiver-cum separator (7) [
In 2017, Martins and collaborators studied the turbo-extraction of stevioside and rebaudosideo A from
In this procedure, the wet raw material is pulverized to produce a fine slurry. The target material is moved in one direction (usually as a fine slurry) within a cylindrical extractor where it comes in contact with extracting solvent. Further, the starting material moves making more concentrated extract. Thus, complete extraction is possible when the amounts of material and the flow rate of solvent are optimized the complete extraction is possible. The process is extremely efficient, takes little time and poses no danger when high temperature is applied. Lastly, the extracts come out sufficiently concentrated at one end of the extractor, while the residue falls on the other end [50]. This extraction procedure has great advantages:
compared to other methods such as maceration, decoction, percolation a unit amount of the plant material cab be extracted with a much smaller volume of solvent;
CCE is usually performed at room temperature, which avoids the thermolabile constituents from being exposed to heat which is used in most other techniques;
Since the drug is pulverized under wet conditions, the heat generated during comminution is neutralized by water. This once more avoids the thermal degradation of components from heat exposure;
Compare to continuous hot extraction, CCE is rated to be more efficient and effective.
Solid-phase extraction (SPE) is a sample preparation technology using chromatographic packing material, solid particle, commonly found in a cartridge-type device, to chemically separate the different components. Samples are almost constantly in the liquid state (although special applications can be run with some samples in the gas phase). In this method, the dissolved or suspended compounds in a liquid mixture are separated from other compounds depending on their physical and chemical properties. The technically correct name for this technology is “Liquid–Solid Phase Extraction”, since the chromatographic particles are solid and the sample is in the liquid state [87].
SPE has many benefits, but four significant benefits deserve special attention:
simplification of complex sample matrix along with compound purification;
reduce ion suppression or enhancement in MS applications;
capability to fractionate sample matrix to analyze compounds by class;
trace concentration (enrichment) of very low-level compounds.
This rapid, economical and sensitive technique uses different types of cartridges and disks, with various sorbents, where the solute molecules are preferentially attached over the stationary phase.
The principle of this equipment is similar to PEF, with the difference that electrical discharge is made through a small point. For this, a needle electrode is used from which the release is made in a plate ground electrode.
These methods are known as greener methods, are often better than conventional ones in terms of high yields, high selectivity, lower solvent consumption and shorter extraction time. They are also found to be environmentally ecofriendly since energy, and organic solvent consumption are reduced. The combination of extraction methods to obtain high purity extracts or high overall yields are described in the literature [40, 88, 89, 90]. Its main advantage is the operability in continuous mode, which is very important from an industrial and economic point of view [80].
A new solvent-based on hydrofluorocarbon-134a and a new technology to optimize its remarkable properties in the extraction of plant material offer significant environmental advantages and health and safety benefits over traditional processes to produce advanced quality natural fragrant oil, flavors and biological extracts.
The technology known as “phytonics process” was developed and patented by Advanced Phytonics Limited (Manchester, UK). Fragrant components of EOs and biological or phytopharmacological extracts that can be used straightly without additional chemical or physical treatment are the products frequently extracted by this process. The properties of the new generation of fluorocarbon solvents have been applied to the extraction of plant material. The core of the solvent is 1,1,2,2-tetrafluoroethane, better known as hydrofluorocarbon-134a (HFC-134a) with a boiling point of – 25°C; a vapor pressure of 5.6 bar at ambient temperature. It is flammable and non-toxic. This product was developed as a replacement for chlorofluorocarbons and more importantly, it does not deplete the ozone layer. By most standards this is a poor solvent that is unable to break up (dissolve) plant waste.
The process is advantageous because the solvents can be customized: by using modified solvents with HFC-134a, the process can be made highly selective in extracting a specific class of phytoconstituents. Likewise, to withdraw a broader spectrum of constituents other modified solvents can be employed. The biological products obtained by this process contain extremely low residual solvent. Residuals are constantly below the levels of detection and are fewer than 20 parts per billion. Therefore, selected solvents have minimal potential reaction effects on the botanical material, and are neither acidic nor alkaline. At the end of each production cycle, the processing plant is sealed so that solvents are constantly recycled and totally recovered. Electricity is the unique utility required to perform these systems and, even then, they consume little energy. There is no scope for the escape of the solvents, and even if some solvents come to escape, they pose no threat to the ozone layer because they do not contain chlorine. The waste product (biomass) from these plants is dry and “ecofriendly” to handle.
As the benefits of this procedure, we have the following:
the phytonic process is soft and its products are never damaged by exposure to temperatures over ambient because relatively low temperatures are employed;
vacuum stripping is necessary which, in other processes, leads to the loss of precious volatiles;
the process is performed completely at neutral pH, and in without oxygen, the products never suffer acid hydrolysis damage or oxidation;
the procedure is extremely selective, and offer a choice of operating conditions end products;
it requires a minimum amount of electrical energy;
it is less threatening to the environment;
no harmful emission in the atmosphere and the subsequent waste products (spent biomass) are inoffensive and pose no effluent disposal problems;
the solvents employed are neither toxic, nor flammable, or ozone-depleting;
the solvents are entirely recycled within the system.
In biotechnology, the utilization of the phytonics process is frequently employed to extract (e.g., for the production of antibiotics), herbal drug, food, EOs and flavor industries, and pharmacologically active products. It is particularly used to produce top-quality pharmaceutical-grade extracts, pharmacologically active intermediates, antibiotic extracts, and phytopharmaceuticals. However, the fact that it is used in all these areas prevents its use in other areas. The technique is being used to extract high-quality essential oils, oleoresins, natural food colors, flavors and aromatic oils from all types of plant material. The technique is also used in refining crude products obtained from other extraction processes. It provides extraction without wax or other contaminants. It helps in the removal of many biocides from contaminated biomass [50].
Upon extraction of the solids and release of desired organics into the extraction solvent, the most common next step is a liquid–liquid extraction, taking advantage of mixing two (or sometimes three or even more that can establish two phases) non miscible solvents, for example, water and ether. The standard rule of thumb is that polar compounds go into polar solvents (e.g., amino acids, sugars, and proteins remain in water). To the contrary, the nonpolar components usually remain in the organic phase (e.g., steroids, terpenoids, waxes, and carotenoids are typically extracted into a solvent such as ethyl acetate).
It is important to minimize interference from compounds that may coextract with the target compounds during the extraction of plant material by conventional or by advanced methods. It is also needed to avoid contamination of the extract and to prevent decomposition of important metabolites or artifact formation as a result of extraction conditions or solvent impurities [3]. Regardless of the extracting procedure employed, the resulting solution should be filtered to withdraw whatever particulate matter. Due to the accompanying increased risk of formation of artifact and decomposition or isomerization of extract components plant extract should not be stored in the solvent for a long time at room temperature or in sunlight because [3].
The chemical investigation profile of a plant extract, fractionation of a crude extract is suitable to isolate the major classes of compounds from each other before further chromatographic analysis. One procedure based on varying polarity that might be used on an alkaloids-containing plant is indicated in Figure 10. The type and quantity of components to be separate into different fractions will, vary from plant to plant. Such procedure can be modified when labile substances are investigated [47].
A general procedure for extracting fresh plant tissues and fractionating into different classes according to polarity.
Essential oils (EOs) are concentrated aromatic hydrophobic oily volatile liquids characterized by a strong odor and produced by all plant organs [91]. They are obtained from raw material by several extraction techniques such as water or steam distillation, hydrodiffusion, solvent extraction, Soxhlet extraction, expression under pressure or cold pressing method, also known as scarification method, microwave-assisted extraction, microwave hydrodiffusion and gravity, supercritical fluid or subcritical water extractions. The best extraction method to use depends on the ease of evaporating (volatility) and the hydrophilicity or hydrophobicity (polarity) of the desired components [92, 93, 94, 95, 96]. However, the three most commonly applied techniques to extract EOs are Soxhlet, hydrodistillation, and SFE [97]. The extraction method chosen significantly affects the chemical composition of EOs [91]. Benmoussa and collaborators have recently found that the microwave hydrodiffusion and gravity (MHG) appeared like a rapid process, a green technology, and a desirable alternative protocol to enhance both the quality and the quantity of the EOs extracted from medicinal and aromatic plants [92].
Lipids contain a broad category of non-polar molecules that are barely soluble or completely insoluble in water, but soluble in an organic solvent such as
Extraction process of edible oils may have negative effects on taste, stability, appearance or nutritional value, preserve tocopherols, and prevent chemical changes in the triacylglycerol. Fats and oil can be extracted from plants using conventional and advanced techniques that include hot water extraction, cold pressing, solvent extraction, high-pressure solvent extraction, microwave –assisted extraction, and supercritical fluid extraction [99]. Extraction of oil involves several mechanisms for removing a liquid from a solid such as leaching, washing, diffusion and dialysis [98]. In the case of palm oil (seeds of
The main side reactions reported during oil processing are (i)
Volatile organic compounds (VOCs) are odorant compounds emitted from plant tissues. Plants can produce a high diversity of VOCs. They are responsible for the distinct aroma of certain dried plants, including the tea,
Hydro-distillation (HD), steam distillation (SD), simultaneous distillation solvent extraction (SDE), microwave-assisted hydro-distillation (MWHD), supercritical fluid extraction (SFE), purge and trap, and solid phase microextraction (SPME), are used to extract VOCs [110].
Verde and collaborators conducted a work to optimize the MAE of the volatile oil terpenes from
The alkaloids are low molecular weight nitrogen-containing compounds found mainly in plants and a lesser extent in microorganisms and animals. They contain one or more nitrogen atoms, typically as primary, secondary, or tertiary amines, which usually confers basicity on the alkaloids. If the free electron pair on the nitrogen atom is not involve in mesomerism, the salt formation can occur mineral acids. This fundamental property of alkaloids is used in their extraction and further clan-up. According to the nature of the nitrogen-containing structure, alkaloids are classified as pyrrolidine, piperidine, quinoline, isoquinoline, indole, etc. [27].
Two methods may be used for alkaloids extraction. One is to basify the plant material using diethylamine or ammonia and extract with an organic solvent [112, 113]. Alkaloids are substances with a basic character and their solubility is a function of pH. They are soluble in low polar organic solvents in basic medium, while in acidic medium, they are soluble in water.
Alkaloids containing basic amines can be selectively extracted using a modified version of the classical “acid–base shake-out” method (Figure 11).
General procedure to obtain alkaloidal extracts from crude plant material [
As recommendations, mineral acids and strong bases should be avoided in extracting alkaloids (and plant material in general) because of the risk of artifact formation [3, 114, 115].
Caffeine is a natural product found in Coffee, cocoa beans, kola nuts, and tea leaves in a substantial amount. Its efficient extraction from Coffee relies heavily on the properties of caffeine and other components present in Coffee. One of the most popular species of the genus whose seeds contains caffeine is
Chemical structure and a few data of caffeine.
There are several ways to remove caffeine from coffee. Here are few reported procedures:
Coffee seeds are firstly grounded and refluxed in an aqueous sodium carbonate solution for about 20 minutes under constant stirring. After filtration of the resulted mixture to filtrate is allowed for cooling at room temperature. The DCM is use to perform the partition of the aqueous filtrate. The process is repeated several times to extract more caffeine. The DCM fractions are then mixed with anhydrous sodium sulfate to remove water traces, the DCM-caffeine solution is filtered through reverse-phase filter paper, which will trap any water and residual matter. The DCM solution is allowed to evaporate and the white amorphous powder of caffeine is obtained [118].
The addition of sodium carbonate converts the protonated form of caffeine, which is naturally present in coffee, to its free caffeine form. During the extraction of caffeine, tannins being soluble in water and organic solvents can interfere with extraction. A weak base such as calcium carbonate or sodium sulphate can be added to break down tannins esters bonds into glucose and calcium or sodium salts of gallic acid, both of which will not be extracted into the organic solvent.
Some benefits are reported when using this method: caffeine is easily extracted from the final product after avoiding the use of flammable and toxic solvents. In this process, caffeine diffuses into supercritical CO2 with water. Coffee beans are introduced at the top while fresh CO2 is introducing at the bottom of an extractor vessel in a continuous extraction to remove caffeine. The recovery is accomplished in a separate absorption chamber containing water. Higher temperature and pressure are mandatory to obtain great yields. A pretreatment step is needed in this process. The addition of polar cosolvents affects cosolvent solute specific chemical or physical interactions. The extraction rate is accelerated by the solvent–cosolvent interaction and makes the extraction easier. The material is humidified with ultrapure water for prewetting, this will destroy the hydrogen bonds that link the caffeine to its natural matrix. Cell membrane swelling enhances solute diffusion. Subsequently, the quality of caffeine extracted can reach a purity >94%, which is generally the standard criteria for use in the soft drink and drug companies [119].
There are some benefits to use charcoal: it is cheaper, “green,” and ease to regenerate by heat and steam. The choice of active charcoal with the appropriate number of micropores and a specific area up to 1000 m2/gram is mandatory for good absorption performance.
Cleaned green coffee beans are firstly soak in water, and the caffeine and other soluble content transferred to the aqueous phase. During the filtration through the activated charcoal, solely caffeine will continue to migrate in water. The recovered and dried coffee beans are now decaffeinated [30].
The poppy straw (
Cold water is used to treat the opium and the obtained aqueous solution concentrated until syrupy consistence. Powered sodium carbonate is added to precipitate hot and heated as long as ammonia given off; it is recommended that the solution remain alkaline to phenolphthalein and left aside four 24 hours at room temperature. After standing, the precipitate is filtered and cold water is use to wash several times until the wash-water become colorless. The precipitate is dissolved in alcohol at 85°C and the alcoholic solution is allowed for evaporation until dryness, and the residue is exhausted after neutralization with little amount of acetic acid. Decolorizing charcoal is used to treat the acidic solution and afterward precipitated with ammonia, avoiding excess is important. After filtration, the precipitate is washed and purified by crystallization in alcohol; concentration of the alcoholic mother-liquor yields a further quantity of morphine. This procedure was reported to be impossible to be consider for industrial scale because of the slight solubility of morphine is alcohol [120].
The gummy opium in divide into thin slices and treated with hot water thrice of its weight until obtain a homogeneous paste. After filtration the residue is pressed and treated again with thrice its weight in water. The resulted solutions are combined and allowed to evaporation until half their volume and poured into boiling milk of lime. One part of lime in ten parts of water should be used for four parts of opium; it is then filtered off again. The lime solutions are united and concentrated to a quantity twice the weight of the opium used. The solution is filtered, heated to boiling, and morphine is precipitated by adding ammonium chloride. The solution is filtrated after cooling at room temperature, and the precipitate is washed, then purified by solution in hydrochloric acid and crystallization of the morphine hydrochloride. It is an attractive process since there are no technical difficulties and the morphine is well separated from the secondary alkaloids. The morphine solutions are relatively clean; however, the yield might be bad. The contributory factors may be the oxidation of morphine in alkaline solution, and the fact that the lime always retains morphine [120].
Five to ten times its weight of cold distilled water is used to completely exhaust the opium. The resultant solution is evaporated to the consistency of a soft extract. The process is repeated with cold distilled water. This aqueous re-extraction causes impurities to precipitate, they are filtered off and the solution obtained is evaporated until its density is 10° Baumé. For each kilogram of opium, one hundred and twenty grams of calcium chloride are added to the boiling liquor, which is further diluted with an amount of cold water equal to its volume. A mixture of a precipitate of meconate and sulfate of calcium is thus formed and is filtered off. After filtration, the filtrate is once more concentrated to produce a new deposit which consist almost entirely of calcium meconate. After removal of the residue by filtration, the filtrate is left to stand for few days until it becomes a crystalline mass called “Gregory’s salt”. It is a mixture of hydrochloride and codeine hydrochloride. The crystals obtained are drained and then placed in a cloth and squeezed out in the presser. Successive crystallization is employed and each time animal charcoal is used to decolorize the solutions. To separate morphine to codeine, sufficiently pure crystals are dissolve in water and ammonia is therefore added to precipitate morphine while codeine remains in aqueous solution.
The first disadvantage of this procedure is that 20 to 25% of the morphine is left with the secondary alkaloids in the brown and viscous mother-liquids after filtration of the Gregory’s salt. The second drawback is that the hydrochloride of morphine and codeine crystallize in furry needles retains the mother-liquids in which the crystallization occurred. Several successive crystallization and subsequent recoveries are required for purification, which is a time-consuming process [120].
Later in 1957, an efficient method of extraction of morphine from poppy straw was developed by Mehltretter and Weakley. Water-saturated isobutanol containing 0.23% ammonia was used to extract morphine. Almost all the alkaloid was absorbed by passing off the raw opium through a cation exchange ions resin bed. Quantitative elution of morphine from the bed was achieved with dilute aqueous alkali. After neutralization and concentration, the crude morphine is obtained, and the eluate can be converted to hydrochloride pharmaceutical grade without difficulty. The general recovery of morphine was 90% [121].
Cooper and Nicola have reported recently a straightforward process for extraction of morphine with a good overall yield (Figures 11 and 13). Morphine and related alkaloids can be purified from opium resin and crude extracts by extraction in the following manner: first, soaking the resin with diluted sulfuric aci