Recapitulation of the results.
\r\n\t2) Human sexual disorders in males and females.
\r\n\t3) Psychological aspects of the human sexual response cycle and its disorders.
\r\n\t4) The therapeutic aspects.
\r\n\tThe human sexual response cycle and human sexual behavior are interrelated. How this inter-relationship and its association to normal sexual health need to be delineated. In a world torn between sex and sexually transmitted disease, clear-cut scientific information in the form of a monograph is required to educate.
\r\n\r\n\tHuman sexuality, gender identity, and sexuo-erotic orientation play great roles in human health and disease. Sex education is the need of the hour and a reflection will be timely.
",isbn:"978-1-80355-151-7",printIsbn:"978-1-80355-150-0",pdfIsbn:"978-1-80355-152-4",doi:null,price:0,priceEur:0,priceUsd:0,slug:null,numberOfPages:0,isOpenForSubmission:!1,isSalesforceBook:!1,hash:"13af09c4cf93ae89789a3db597972cf6",bookSignature:"Dr. Dhastagir Sultan Sheriff",publishedDate:null,coverURL:"https://cdn.intechopen.com/books/images_new/11267.jpg",keywords:"Master and Johnson's Cycle, Sex Education, Premature Ejaculation, Orgasmic Disorders, Sexual Aversion Disorders, Dyspareunia, Vaginismus, Sex Hormones, Sexually Transmitted Diseases, Impotence, Low Libido, Blood Analyses",numberOfDownloads:99,numberOfWosCitations:0,numberOfCrossrefCitations:0,numberOfDimensionsCitations:0,numberOfTotalCitations:0,isAvailableForWebshopOrdering:!0,dateEndFirstStepPublish:"August 18th 2021",dateEndSecondStepPublish:"March 3rd 2022",dateEndThirdStepPublish:"May 2nd 2022",dateEndFourthStepPublish:"July 21st 2022",dateEndFifthStepPublish:"September 19th 2022",remainingDaysToSecondStep:"3 months",secondStepPassed:!0,currentStepOfPublishingProcess:4,editedByType:null,kuFlag:!1,biosketch:"Dr. Sheriff is a life counselor, sex educationist, and researcher with over 35 years of teaching experience, five authored books, and editorials written in the British Journal of Sexology and the Journal of Royal Society of Medicine. Dr. Sheriff is a life member of the European Society for Human Reproduction, and Early Human Development, American Association of Clinical Chemistry, Association of Physiologists and Pharmacologists of India, and a member of the National Academy of Medical Sciences.",coeditorOneBiosketch:null,coeditorTwoBiosketch:null,coeditorThreeBiosketch:null,coeditorFourBiosketch:null,coeditorFiveBiosketch:null,editors:[{id:"167875",title:"Dr.",name:"Dhastagir Sultan",middleName:null,surname:"Sheriff",slug:"dhastagir-sultan-sheriff",fullName:"Dhastagir Sultan Sheriff",profilePictureURL:"https://mts.intechopen.com/storage/users/167875/images/system/167875.jpg",biography:"Dhastagir Sultan Sheriff is a life member of the European Society for Human Reproduction and Early Human Development, Association of Physiologists and Pharmacologists of India, member of the National Academy of Medical Sciences, New Delhi, and resource person for UNESCO for Medical and Bioethics. Dr. Sheriff has authored five books including a textbook on medical biochemistry with additional interest in human sexology. He had editorials written in the British Journal of Sexology, Journal of Royal Society of Medicine, Postgraduate Medicine, and Scientist. 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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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Due to creep the total strain in the material gradually increases. At the same time the microstructure can also change. For example the strength of many materials used at high temperatures is based on the presence of fine particles that slow down the deformation. There is a thermodynamic driving force for coarsening of the particles, since this will reduce the total surface area of the particles and thereby the surface energy. The deformation of the material and changes in the microstructure will decrease the strength of the material and this is referred to as the formation of creep damage. When the creep damage has reached a certain level, failure takes place.
\nPolycrystalline materials consist of regions with a specific lattice orientation called grains and the boundaries between them grain boundaries. During the creep deformation, small voids called creep cavities are formed at the grain boundaries. The size for the cavities is of the order 1 μm. The creep cavities are continuously nucleated so their number increases with time. Each individual cavity also grows so their radii increase. The driving force is the same as for coarsening of particles, that is, a reduction of the surface energy. In this way, there is a gradually increasing fraction of the grain boundaries that is cavitated. When the area fraction of cavities has reached a critical value, the cavities join and eventually form cracks that make the material fail.
\nThe fact that creep rupture is mainly controlled by the development of grain boundary cavities has created a large technical interest in cavitation. This interest increased even more in the 1980s, when it was recognised that the appearance of the cavitation could be used to estimate the residual life time of fossil fired power plants. The service time of many power plants were approaching the design life and operators were asking whether it would be safe to continue running the plants. Neubauer found that by observation of the cavitation with the help of the replica technique, the residual lifetime could be estimated [1, 2]. The cavitation was subdivided into four classes (and one for undamaged material): individual cavities to a small extent, individual cavities to a large extent, stringers of cavities and finally microcracks. Replicas were taken at welds, pipe bends and other critical positions. The basic idea was that if damage of one class was detected, the damage did at most correspond to the next class at the next inspection. The method was very successful when it was applied to low alloy steels such as 0.5Cr0.5Mo0.25V and 2.25Cr1Mo, which represented the body of materials of the plants at the time. Unfortunately the method is less applicable to today’s materials such as 9 and 12Cr steels, because cavitation appears only at a late stage of life and does not provide the necessary early warning.
\nThe successful technical use of observations of cavitation stimulated a lot of scientific work. This was dominated by empirical approaches to describe the development of the creep damage. The first and perhaps most well-known approach was set up by Kachanow and Rabotnov [3–5]. They simply assumed that the cavities represented voids that reduced the loading capacity. The most interesting feature of the method is that it is consistent with behaviour of creep strain during the tertiary creep, that is, the final stage before rupture [6, 7]. This dependence is nowadays referred to as the omega method [8].
\nWe will now concentrate on basic models for cavitation. Traditionally cavity nucleation has been modelled either as a process of rupturing atomic bonds or of atomic vacancy condensation. For the former approach the estimated threshold stress is orders of magnitude higher than the applied stress, which makes it physically unrealistic because high stresses will be reduced quickly in a creeping material [9]. The condensation of vacancies can be treated with the help of the classical nucleation theory [10]. It is shown that cavity nucleation would be a very rare event at low stresses but becomes frequent above a certain threshold stress [11]. High stress concentration can be formed at grain boundary ledges, grain boundary triple points and particles. Cavity nucleation at particles can be a result of decohesion of particles from the matrix. In practically all models that have been presented, a high stress concentration is needed. A threshold stress and an incubation time are essential to form a cavity [10, 12]. Contrary to these suggestions nucleation frequently takes place at low stresses and is controlled by strain rather than stress. In agreement with statements in the literature it can be concluded that theories of cavity nucleation have not been fully successful in earlier work [13, 14]. In both these papers excellent reviews are given.
\nFor modelling cavity growth the situation was different but not entirely unproblematic. A diffusion controlled cavity growth was formulated by Hull and Rimmer [15]. The model was later improved in particular by Beere and Speight [16]. It was soon realised that the model gave much larger growth rates than observed experimentally in many cases. Dyson proposed that the cavities should not be able to grow faster than the creep deformation of the surrounding material [17]. This is referred to as constrained cavity growth. Rice developed an explicit model for constrained growth [18]. The idea of constrained growth is now fully accepted. However, the model still tends to overestimate the growth rates. It is now believed to be due to the assumptions in Rice’s derivation. This will be analysed in the present paper.
\nIt is evident from the summary above that the modelling of formation and growth of cavities has met considerable difficulties in the past. In recent years important new developments have taken place. With the help of these developments fundamental quantitative modelling of both nucleation and growth of creep cavities has now been possible to set up. In addition some of the difficulties that have been encountered in the past can be understood. It is the purpose of this paper to review these new developments.
\nGrain boundary sliding (GBS) occurs when neighbouring grains move with respect to each other in shear. The mechanism is illustrated in \nFigure 1. During the creep deformation the two grains have moved 0.8 μm with respect to each other. To observe GBS, the specimen surface has to be scratched, for example, with a knife. When the scratches cross a sliding grain boundary, the two parts of the scratches on the different sides of the grain boundary are displaced. This displacement is a direct measure of GBS.
\nIllustration of grain boundary sliding (GBS) for a copper specimen that has been exposed to 3.3% creep strain during 307 h at 125°C [
It is generally accepted that a prerequisite for cavity nucleation is grain boundary sliding. Experiments on copper bicrystals have shown that artificially introduced GBS can dramatically increase the amount of cavitation. Chen and Machlin [20] and Intrater and Machlin [21] exposed bicrystals of copper to either tensile loading or to a combination of tensile loading and shear. The latter alternative gave much larger number of cavities. It is natural that GBS gives rice to cavitation, since any obstacle at the grain boundary such as a particle will give rise to large stress concentrations. In low alloy steels cavities have frequently been observed around manganese sulphides [22]. Since the interface between the sulphides and the matrix is weak, voids are easily formed there. Some papers also suggest that cavities can be formed at carbides, see, for example, Ref. [23].
\nThe most convincing argument concerning the central role of GBS in cavity nucleation comes from the creep strain dependence of both GBS and cavity nucleation. It has been observed many times that the displacement
\n
\n
Experiments that give the strain dependence of
Observed displacements at grain boundaries in copper as a function of strain [
The displacement
To investigate the influence of GBS on the total strain, Crossman and Ashby [31] developed a finite element model (FEM) for shear stresses. If a free grain boundary is considered, they found that the sliding rates are very high for typical creep stresses and that the grain boundaries could be considered as flaws in the material with respect to GBS. Later Ghahremani [32] transferred the model to tensile stresses, which are typically used in creep testing. In both Refs. [31, 32] a Norton equation for the creep strain rate was considered
\nσ is the applied stress and
\n\n
where
Eq. (6) is referred to the
Comparison of modelled Eq. (
For materials with particles in the grain boundaries Riedel has derived a model corresponding to Eq. (1) [33]. The sliding boundary was represented by a shear crack surrounded by creep deforming grains. The model is referred to as the
The two models (shear sliding and shear crack models) are compared with the experimental GBS displacements for different austenitic stainless steels [34–38] in \nFigure 4. The shear crack model is compared with the average of all the experimental data, Ave. 1. The shear sliding model does not work very well for large grain sizes so data for such grain sizes [38] are not included in the comparison, Ave. 2. It can be seen from \nFigure 4 that
Modelling and experimental GBS displacement as a function of creep strain for different types of austenitic stainless steels, from Ref. [
From \nFigures 3\n and \n4 it is evident that the shear sliding and shear crack models can describe the experimental data for fcc metals with reasonable precision.
\nThe mechanisms for cavitation nucleation have been a puzzle for a long time as explained in the introduction. However part of the explanation came from studies on copper. Pure copper can show extensive cavitation during creep [39], but the number of particles present is so low that they cannot explain the large number of cavities. Lim suggested that it was the substructure of the dislocations that could nucleate the cavities [40]. He also presented a model that can be used to demonstrate whether a nucleation mechanism is thermodynamically feasible or not. He assumed that pile ups of grain boundary dislocations generate the necessary high stresses for the nucleation. Since these high stresses are stationary as a result of the creep process, it avoids the problem of fast stress relaxation in many models. Lim’s model is fairly complex and details in the model will not be given here. When a cavity is formed the free energy Δ
γs and γGB are the surface and grain boundary energies per unit area.
Lim’s model has been applied to copper and austenitic stainless. As long as energy is gained when a cavity is formed, that is, Δ
Minimum stress to form cavities at cell boundaries versus temperature for oxygen free pure Cu-OF and phosphorus alloyed copper Cu-OFP. For comparison the stress that gives creep rupture after one year (10,000 h) is included. After Ref. [
These minimum stresses are compared with design stresses during creep in copper. It is clear that the stresses required for nucleation are well below the stresses that typically appear in the material. This demonstrates that nucleation based on the substructure is a viable process.
\nFrom a technical point of view it is well established that the creep ductility of oxygen free pure copper Cu-OF can be very much lower than for phosphorus alloyed copper Cu-OFP. As a consequence the latter material should be used in creep exposed components [28, 41]. It is evident from \nFigure 5\n that much lower stresses are needed in Cu-OF than in Cu-OFP, which makes the cavitation in the former material much more abundant. This is believed to be the main reason for the low creep ductility of Cu-OF.
\nIt has also been verified that the minimum nucleation stresses are below typical design stresses for the common stainless steels 304H (18Cr10Ni), 316 (17Cr12Ni2Mo), 321 (18Cr12NiTi) and 347 (18Cr12NiNb). For example this is illustrated for 347 (18Cr12NiNb) in \nFigure 6. The design stresses are 10,000 h rupture data. The minimum cavitation stress lies in the interval 35–50 MPa in the interval from 500°C to 750°C. The minimum cavitation stresses are again below the design stresses. The temperature dependence of Lim’s model is probably not fully correct. In general it is thought that the amount of cavitation will increase with temperature. However the temperature dependence of the minimum cavitation stress is weaker than that of the design stress, which suggests the opposite behaviour.
\nMinimum cavitation stress versus temperature for TP347H austenitic stainless steel. 10,000 h rupture data from ECCC [
Experimentally it has been found many times that the number of cavities is proportional to the creep strain, cf. Eq. (2). To explain this strain dependence, Sandstrom and Wu introduced the
where
The constant
In Eq. (10), Eq. (1) has been used. The factor 0.9 in Eq. (10) takes into account the averaging of different orientations [44].
\nThe model in Eq. (10) is compared with experimental data for austenitic stainless steels in \nFigure 7. For three of the experimental data sets TP347 at 550°C and 650°C and TP304 at 727°C, the model gives quite an acceptable description. For TP304XX at 750°C the deviation between model and experiment is larger.
\nModelling and experimental number of cavities per unit grain boundary area as a function of creep strain [
It has been proposed that a critical particle radius exists for nucleation [45, 46]. The radius must exceed a minimum value in order for nucleation to take place. Harris developed a model that related the critical particle size to the GBS velocity [47, 48]. His basic assumption was that particles are not able to stop GBS if the diffusion is fast enough. According to Harris this critical particle radius also represented the minimum radius that could nucleate cavities. Harris gave the following relation between the GBS velocity \n
where λ is the interpaticle spacing, γs the surface energy, δ the grain boundary width,
Comparison of experimental and modelling GBS velocity as a function of particle radius [
In \nFigure 8\n the particle parameters are taken from the experimental references. The minimum particles that nucleated cavities in the experiments are chosen for the critical particle radius. The experimental data clearly support Harris’ model.
\nFrom the particle size distributions [24] the number of nucleated cavities can be estimated if the critical particle size is known. The computed number of nuclei is compared with the observed ones for austenitic stainless steels in \nFigure 9.\n\n
\nComparison of experimental number of cavities and modelling number of particles that initiate cavities [
After the cavities have been nucleated, they start to grow if they exceed a critical size. The main mechanism for the growth is diffusion. Vacancies are transported away from the surfaces of the cavities. The grain boundaries are good sinks for the vacancies. The first model for diffusion controlled growth was presented by Hull and Rimmer [15]. A much more elegant formulation was later given by Beere and Speight [16] and this is the model that has been used since. Their growth equation can be expressed as
\nwhere
From the number of cavities per unit grain boundary area
\n
When diffusion controlled growth models were compared with experimental data, it was evident that the models often strongly exaggerated the growth rate. Dyson found that the predicted growth rate of the cavities many times exceeded the deformation rate of the surrounding material which he considered as unphysical [17]. He suggested that the cavity growth rate should not be larger than the creep rate of the material. This was referred to as constrained growth. Based on this assumption, Rice developed a quantitative model [18]. The result is that in the growth equation, the applied stress is replaced by a reduced stress
\nThe reduced stress is given by
\nwhere β is a material constant (β = 1.8 for homogeneous materials) and
Rice based his analysis on a linear viscoplastic model of an opening crack. He and Sandstrom reanalyzed the model and avoided the assumption of linearity [52]. A grain structure with a pillar of height
\n\n
In general Eq. (19) has to be solved by iteration to find the new value of σred. This new value for σred is lower than that given by Eq. (17). This is illustrated in \nFigure 10: Both the absolute and relative difference increase with time.
\nReduced stress according to Eq. (
The new constrained growth model is compared to experimental data for austenitic stainless steels in [52]. Some examples are given here in \nFigure 11. Growth data for 18Cr10Ni steel with and without Nb or Ti are shown. It can be seen that the growth data can be described with fair accuracy. The lower growth rate according Eq. (19) is important in this respect.
\nCavity radius as a function of creep time for 18Cr10Ni without or with Nb (347) or Ti (321) austenitic stainless steels. Model according to Eq. (
Creep rupture is technically very important, because it determines the life of many plants operating at high temperatures. Two main mechanisms are distinguished: ductile rupture and brittle rupture. Ductile rupture is controlled by the exhaustion of the deformation capacity of the material. In this case the usual rupture criterion is that the creep strain reaches a critical value. The deformation takes place by dislocation mechanisms. The faster the dislocations move, the faster rupture occurs. Since ductile rupture does not involve cavitation, it is not reviewed here, but full details can be found elsewhere [53].
\nRupture curves for dislocation creep are illustrated in \nFigure 12 for the austenitic stainless steel 18Cr12NiTi (321H) at temperatures between 600°C and 775°C. The experimental creep rupture data cover times up to 100,000 h (11 years). The general overall behaviour is well described by the model predictions.
\nComparison of dislocation creep model rupture curves (ductile rupture) Refs. [
The second process brittle rupture is due to grain boundary decohesion. By far the most important mechanism in this respect is the formation and growth of cavities. It is well established that when the cavitated grain boundary area reaches a certain fraction of about 0.25, brittle rupture takes place [54]. The cavitated area fraction
A continuous nucleation of cavities takes place. The number of cavities is directly proportional to the creep strain, Eq. (10). Once a cavity has nucleated it starts to grow after an incubation time
The model predictions for brittle rupture for 18Cr12NiTi (321H) are shown in \nFigure 13. The predictions are compared to the same experimental data as in \nFigure 12. Again the overall time dependence of the rupture strength at different temperatures is well represented. In fact the differences between the model predictions for ductile rupture in \nFigure 12 and brittle rupture \nFigure 13 are not very large.
\nComparison of model rupture curves based on cavitation (Eq. (
Ductile rupture is assumed to be controlling if the strain exhaustion occurs before
Comparison of model rupture curves based on both dislocation creep (ductile rupture) and cavitation (brittle rupture) with experiments [
When brittle rupture is taken into account when modelling the creep rupture curves, there is an improvement in particular at high temperatures and low stresses.
\nWith the development of the
It is assumed in general that nucleation of creep cavities is based on GBS. The new models for GBS have made it possible to set up realistic models for nucleation. Many models for nucleation developed in the past are strongly stress dependent and suggest that the amount of cavitation would increase with stress, which is clearly at variance with most observations on creep. This applies for example to models based on classical nucleation theory. Using Lim’s model for substructure induced cavitation [40], it has now been demonstrated both for commercial copper and austenitic stainless steel that the creep stresses in the substructure are sufficiently high to nucleate cavities. Since the stresses are stationary, the problem with rapid relaxation in particular at high stresses is avoided. If particles instead of subgrain corners constrain the grain boundary dislocations, the outcome of the model is essentially the same. The model is consequently applicable to cavity nucleation at particles as well.
\nWith the help of the
Harris developed a model for nucleation around particles many years ago [47, 48]. He considered the relation between particle sizes and the GBS displacement. If the particles are sufficiently large it is assumed that they will prevent GBS. He formulated a criterion for the critical particle size. If GBS is prevented significant stresses are formed at the particles. If the critical particle size is exceeded, Harris proposed that cavity nucleation can take place. With the event of the new models for GBS it has now for the first been possible to test Harris’ ideas. It turns out that both the critical particle radius and the number of cavities that can be estimated from the particle distributions are in agreement with observations for austenitic stainless steels. In this way a method for estimating the critical particle size for nucleation has been established.
\nGBS does not occur on every grain boundary. In fact only on a limited number of GBS events is observed in a material that has been creep exposed [19]. As a consequence cavity nucleation only occurs on some grain boundaries. The presence of cavities show a large statistical variation, see for example [39]. The models in the present paper represent grain boundaries where cavities will be formed. These are also the grain boundaries that control the rupture of the material. The models predict a fairly high nucleation rate that represents the most active grain boundaries and not an average over all grain boundaries.
\nModels for cavity growth have been available for a long time. Unfortunately these models in general generate growth rates that are much higher than the observed ones. This might be the reason why very few quantitative comparisons have been made between experiments and models in the literature. A major step forward was the introduction of constrained growth [17]. Then the cavities were not allowed to grow faster than the surrounding creeping material. A quantitative model for constrained growth was given by Rice [18]. Still the growth rates tended to be higher than the observed ones. Only recently it has been recognised that some minor approximations in the work of Rice were essential to correct [52]. With these new corrections satisfactory predictions for cavity growths in austenitic stainless have been achieved.
\nThe recent development has implied that quantitative models are now available for grain boundary sliding, for the thermodynamic feasibility of cavity nucleation controlled by subboundaries, the nucleation rate and constrained cavity growth, that is, for all of the involved main processes. Each model is of great significance in itself, but by using combinations of them, the development of cavities can be fully understood.
\nRecent development of processes concerning the development of creep cavities has been reviewed. Models have been covered for grain boundary sliding, cavity nucleation and cavity growth.
Based on analysis of previously presented FEM models, a model for the grain boundary displacement during sliding called the shear sliding model has been presented. The model gives a displacement that is proportional to the creep strain. The model can quantitatively reproduce the observed displacements for fcc alloys.
Using Lim’s model for subboundary assisted cavity nucleation, it has been demonstrated that this process is thermodynamically feasible for copper and for austenitic stainless steels. It gives a minimum cavitation stress that is well below stresses in creep exposed components.
According to the double ledge model, nucleation is assumed to take place when subboundaries on one side of a sliding grain boundary meet subgrain corners or particles on the other side. The model gives a nucleation rate that is proportional to the creep rate in good accordance with observations. The model can predict the measured nucleation rates in austenitic stainless steels.
Due to the development of the new models for GBS, it has for the first time been possible to test Harris’ model for cavity nucleation around particles. The model gives a relation between the critical particle radius and the GBS velocity. Data for austenitic stainless steels confirm the validity of the model.
A modified constrained growth model has been presented. It gives lower growth rates than previous models. These lower growth rates have implied that observed growth rates for austenitic stainless steels can now be reproduced.
Alloys can fail by ductile or brittle creep rupture. It is demonstrated that by considering both ductile and brittle rupture, the prediction of creep rupture curves can be improved in particular at high temperatures and low stresses.
Radio frequency identification (RFID) is a technology used mainly to identify tagged items or to track their locations. The identification technology by radio frequency (RFID) uses electromagnetic fields to automatically identify and track tags attached to objects. The tags contain electronically stored information; passive tags collect energy from a nearby RFID reader’s interrogating radio waves. Active tags have a local power source (such as a battery) and may operate hundreds of meters from the RFID reader. The first secure system identifying the friend and the foe (IFF) was the first form of RFID’s technology. In 1948, Stockman (Stockman, 1948) proposed the identification from distance. He defended that it is possible to vary the amount of reflected power (also called load modulation antenna) by the alternation of the load of the tag antenna and consequently it has a modulation. Identification by radio frequency, known as RFID, is a smart technology that is very performed, flexible, and more suitable to automatic operations. RFID is an automatic identification method using radio waves to read the data contained in the devices called tag RFID. RFID technology is used to monitor, identify, and track objects, animals, and people away. The RFID system has two key features: RFID tag (label) and RFID reader. Today, this technology finds use in access controls, vehicle safety, animal tracking and patients in hospitals, and other applications [1].
The purpose of this chapter is the design and simulation of a PIFA with a T-shaped slot. We studied the effect of changing the type of feed supply, the type of substrate, and thus the position of the connecting line between the ground plane and the radiating element. The PIFA consist of a radiating element of length equal to the quarter wave and of a short circuit of several types: plane, tongue, or wire. This structure has advantages over a traditional patch antenna: cost and ease of manufacture, reduced size, thin profile, and bandwidth.
RFID is part of automatic identification technologies; this technology makes it possible to identify an object or a person, to follow the path and to know the characteristics at a distance thanks to label emitting radio waves, attached to or incorporated into the object or person. RFID technology allows reading of labels even without direct line of sight and can cross thin layers of materials [2, 3].
RFID includes labels, readers, encoders, and middleware which allow integrating the flow of data in the information system of the company.
One of the most used identification methods is to house a serial number or a sequence of data in a chip and connect it to a small antenna. This couple (chip + antenna) is then encapsulated in a support. These “tags” can then be incorporated in objects or be glued on products, Figure 1. The format of the data on the labels is standardized at the initiative of electronic product code (EPC) Global.
Tag antenna.
The reader/recorder is constituted of a circuit that emits electromagnetic energy through an antenna and an electronics that receives and decodes the information sent by the transponder and sends them to the data collection device. Not content to read RFID tags, he is able to write their content. The RFID reader is the element responsible for reading radiofrequency labels and transmitting the information they contain (EPC code or other, status information, cryptographic key, etc.) to the next level of the system (middleware). This communication between the reader and the label takes place in four stages:
The reader transmits by radio the energy necessary for the activation of the tag.
It launches a query querying the tags nearby.
It listens to answers and eliminates duplicates or collisions between answers.
Finally, it transmits the results obtained to the applications concerned.
To exploit the information contained in these labels, it is imperative to have the appropriate reader. This one emits radio waves toward the capsule which allows to supply it with energy (electromagnetic induction feed); in other words to activate it, these chips are not able to perform dynamic treatments but only to return static data (Figure 2).
The different geometries of the inverted antennas.
Without any external power supply, they depend on the electromagnetic effect of receiving a signal emitted by the reader. It is this current that allows them to power their microcircuits. They are inexpensive to produce and are generally reserved for volume productions. They are the ones we find especially in logistics and transport. They use different radio frequency bands according to their capacity to transmit remotely more or less important and through different substances (air, water, metal). The reading distance is less than 1 m. Low and high frequencies are standardized worldwide. These chips are stuck on the products for a follow-up. They are disposable or reusable depending on the case.
These tags are similar to passive ID cards. They use similar technologies but with some important differences. They also have a small battery which works constantly, which frees the antenna for other tasks, in particular the reception of return signals. These tags are more robust and faster in reading and transmission than passive tags, but they are also more expensive.
Active tags are the most expensive because they are more complex to produce and provide transmission functions, functions of capture or processing of the captured information, and either or both. Thereby, they need an onboard power supply you have to know that these labels prove particularly well adapted to certain functions, including the creation of authentication systems, security, anti-theft, etc.
Short, they are ideal for triggering an alert or alarm. They can emit several hundred meters.
RFID systems generate and reflect electromagnetic waves. In particular, RFID systems must be careful not to disrupt the operation of other radio systems. We cannot, in principle, use only the frequency ranges specifically reserved for industrial, scientific, or medical applications. These frequency ranges are called industrial-scientific-medical (ISM). The main frequency ranges used by RFID systems are the low frequencies (125 and 134.5 kHz) and ISM frequencies: 6.78, 13.56, 27.125, 40.68, 433.92, 869.0, 915.0 MHz (not in Europe), 2.45, 5.8, and 24.125 GHz.
The advantages of radio frequency labels over the barcode are
The ability to update the content
Unlike bar code for which data are frozen once printed or marked, the content of the data stored in a radio frequency tag will be able to be modified, increased, or decreased by authorized stakeholders (read and write tags).
Greater content capacity
Certainly bar codes that can store important content data appeared these last years, two-dimensional or matrix barcodes. However their use in industrial or logistic worlds remains problematic; they require conditions printing and reading. The commonly used barcodes are limited to data contents of less than fifty characters and in these extreme cases require an A4 or A5 size label. In a radio frequency tag, a capacity of 1000 characters is easily storable on 1 and 2 mm and can easily reach 10,000 characters in a logistics label affixed to a pallet.
The marking speed
The barcode in a logistic context most often requires the printing of a paper medium. Handling and labeling are manual or mechanical operations. The radio frequency labels can be included in the handling support or in the packaging from the outset. Data concerning objects contained or transported are written in a split second at the time of the constitution of the logistics or transport unit, without further manipulation.
Security of access to the content
Like any digital medium, the radio frequency tag can be protected by password in writing or reading.
The data can be encrypted. In the same label, a part of the information can be freely accessible and the other protected. This faculty makes the RF tag, a tool adapted to the fight against theft and counterfeiting.
Longer life
In applications where the same object can be used multiple times, as the identification of handling supports, or the consignment of the container, a radio frequency tag can be reused 1,000,000 times.
Greater positioning flexibility
To enable the automation of the reading of the logistic barcode labels, standardization bodies like EAN, have defined positioning rules on logistics units. With the radio frequency tag, it is possible to abstract constraints related to optical reading; she does not need to be seen. It is enough for him to enter the field of the reader so that his presence is detected.
Better protection against environmental conditions
RFID tags do not need to be positioned outside the object to be identified. They can therefore be better protected from attacks related to storage, to the handling or transport. In addition, their operating principle does not make them susceptible to soiling or various spots that interfere with the use of the barcode.
Disturbance by the physical environment
The reading of radio frequency tags is disturbed by the presence, for example, of metals in their immediate environment. Solutions must be studied case by case to minimize these disturbances.
Disturbances induced by the labels between them
In many applications, several radio frequency tags may occur at the same time in the reader’s field voluntarily or involuntarily. This can be wanted in store, at the time of checkout or between anti-theft doors.
In this last case just detect a stolen object, a label not inhibited by the box. Technology allows it today. More complex is the need to identify and read the contents of several labels in a field without forgetting; to do this the readers use algorithms or anti-collision techniques, etc.
Sensitivity to parasitic magnetic waves
In certain circumstances, RFID reading systems are sensitive to spurious electromagnetic waves issued by computer equipment (computer screens) or lighting systems more generally by electrical equipment. Their use must be tested taking into account the environment.
The regulatory constraints related to the impact on health
This question has been debated for a few years, in particular concerning the anti-theft gates and cell phones. Passive tags themselves present no risk whatever their number is since they are active only when they are in the field of a reader. The studies therefore focus on readers and aim to define the regulatory criteria of their emission power to prevent them from creating disruptions.
RFID tag applications are already very numerous; we give some examples of the possibilities offered by this technology:
Tracking and sorting luggage
The airlines are currently studying the replacement of RFID tags.
The automatic toll
Many management companies’ toll motorways have already put in place systems subscription based on RFID tags and microwave, placed in vehicles. Subscribers benefit in special way of crossing toll gates. Payment is made without stopping the vehicle, by simply reading his identification.
Access control
RFID tags are already used for access control of buildings or car parks.
Animal tracking
More and more applications of animal traceability are growing, whether it’s ear tags on farm animals or the subcutaneous labels for horses or pets. In all cases, it’s about ensuring animal traceability for the purpose of sanitary control or the quality of herds.
Cleaning clothes
For the cleaning of work clothes, companies are putting in place systems uniform identification based on RFID tag with a diameter of 20 mm and a thickness of 2.5 mm, the frequency 13.56 MHz read/write at 20 m.
These labels are attached to the garment; they resist washing operations. They allow a follow-up of the washing operations and easy identification of the wearer of the uniform.
Waste collection
In Europe as well as in Japan and the United States, household or industrial waste collection companies are concerned with improving the load distribution of garbage collection and treatment. The principle is to equip each bin or container of an RFID tag and the collection trucks for readers and weighing system, so that each operation can automatically identify the “producer” and measure the weight of the collected material.
Supply chain management
In logistics, four levels of applications can be distinguished:
Delivery
Home
In transit
Local
At the time of shipment, labels can facilitate the collection of products and the constitution of pallets, sorted by destination and loading control. The label may contain, in addition to the product identification, or the contents of a pallet, that of the manufacturing lot number, consignee identification, order number, handling details, etc. This information collected at the time of loading can be stored in the RFID tag container or means of transport to facilitate checks during transit, customs, access, or exit authorization. Similarly, upon receipt of the goods, the data can be collected to automatically perform audits and update the inventory and make reconciliations with commercial documents or EDI messages. In transit, the label is used to trace the product at each point of loading and unloading or simply passing. Thus, the sender can be informed at any time transport stream. Locally, labels allow product inventory but also media management handling and equipment (gas bottles, etc.).
There are several types of antennas for RFID applications; among these antennas we mention that antennas of the planar inverted-F antenna (PIFA) type are the most used in portable devices for GSM, Wi-Fi, RFID applications, etc. due to their low manufacturing cost and their compactness, as it has very small dimensions compared to a half-wave antenna. The PIFA is obtained by placing the short circuit (plane, wired, or tongue-like) between the half-wave resonator and the ground plane, at the precise point where the electric field vanishes for the fundamental mode. This makes it possible to overcome one half of the resonator and thus have an X/4 resonance. This type of antenna has the advantage of presenting a desired quasi-isotropic radiation in RFID applications, since the relative orientation of the tag relative to the reader is uncertain.
The PIFA is the result of the transformation of the inverted-F antenna (IFA) from a horizontal wire element to a planar structure to compensate for his loss of maladjustment and improve its radiation characteristics. The planar inverted-F antenna (PIFA) is a quarter wave antenna integrated and miniaturized by comparing it with monopole antennas. Also, it has good advantages over a traditional patch antenna (cost and ease of manufacture, small size, and bandwidth). The inverted plane antenna F is a rectangular microstrip antenna powered by a coaxial probe. It is called an inverted-F antenna because the side view of this antenna resembles the letter F with its face down [4, 5, 6, 7, 8, 9].
The ILA consists of a short vertical monopole with the addition of a long horizontal arm at the top. Its input impedance is almost equivalent to that of the short monopole with the addition of the reactance caused by the horizontal wire above the ground plane. In general, it is difficult to match the impedance to a power supply line since its input impedance consists of low resistance and high reactance. Adding the additional inverted-L element adjusts the input impedance of the antenna. The impedance bandwidth of the IFA antenna is less than 2% on the center frequency. One way to increase the bandwidth of the IFA antenna is to replace the upper horizontal arm with a plate oriented parallel to the ground plane to form the inverted plane antenna F (PIFA). More generally called planar inverted-F antenna (PIFA) in the scientific literature, they have the advantage of being compact with a wide bandwidth. Figure 3 shows the different elements of the PIFA [4].
The PIFA.
Figure 4 shows the side view of the PIFA.
The PIFA (side view).
More generally called planar inverted-F antenna (PIFA) in the scientific literature, they have the advantage of being compact with a large bandwidth; it is mainly characterized by the presence of a plate that plays the role of a short circuit between the radiating patch and the ground plane as shown in Figure 5 where h is the height of the short circuit, W its width, and D the distance between the short circuit and the feed point of the patch antenna.
PIFA.
The resonance frequency of a PIFA is approximated by equation (Eq. (1)).
With
The antenna proposed is an antenna consisting of a rectangular patch with a width W = 20 mm and a length L = 18 mm placed on a substrate with a width W = 30 mm and a length L = 30 mm using FR4_epoxy, characterized by a relative permittivity of 4.4, a relative permeability of 1, tgδ of the dielectric losses = 0.02, and a thickness e = 0.7 mm. The antenna is connected to the ground plane through a rod with a height h = 10 mm and a width of 10 mm, Figure 6.
The structure of the PIFA on HFSS.
In contrary to a conventional PIFA, the short circuit is not realized over the entire width of the antenna but through a flat short circuit which is a metal tongue of width W. A T-slot with a width of 0.5 mm in the metal radiating element ensures a good match between the impedance of the chip and the input impedance of the PIFA. The geometry of this antenna is shown in Figure 7.
The structure of the PIFA with T-slot on HFSS. (a) side view and (b) top view.
The Ansoft high frequency structure simulator (HFSS) logger is a very high-performance microwave simulator that models and simulates 3D global fields radiated by microwave structures (antennas, filters, guides, connectors, PCBs, etc.). Characteristics for antennas such as (Gain, SAR, VSWR, Sij, etc.). It is based on the finite element model which consists in solving the equations of the field in discrete points defined in an orderly way in the complete domain of the structure. It directly solves the Maxwell equations in their differential form by replacing the differential operators by difference operators, thus realizing a discretization approximation.
The results of the both PIFA antennas with and without slot at 5.8 GHz are:
Figure 8 shows the return loss of the PIFA, S11 = −21 dB with a bandwidth equal to 200 MHz.
Return loss of the PIFA.
Figure 9 shows the reflection coefficient of the PIFA,
Reflection coefficient of the PIFA.
Figure 9 shows that our antenna is well adapted.
Another essential character for knowing the parameters of the antenna is the SWR of the antenna PIFA.
Figure 10 shows the SWR of the antenna PIFA SWR = 1.09 < 2.
The SWR of the PIFA.
The SWR parameter of the PIFA fitted with a T-slot is less than 2 (Figures 11–13).
The SWR of the antenna with T-slot.
The 3D radiation pattern of the PIFA.
The 3D radiation pattern of the PIFA with T-slot.
The appearance of Figure 14 shows the gain of the PIFA without slot equal to 2.4 dB around the resonance frequency 5.8 GHz.
Gain of the PIFA.
The appearance of Figure 15 shows the gain of the PIFA is equal to 3.4 dB around the resonance frequency 5.8 GHz (Table 1).
Gain of PIFA with slot.
PIFA without T-slot | PIFA with T-slot | |
---|---|---|
–21 dB | −33 dB | |
Gain | 2.4 dB | 3.4 dB |
SWR | 1.09 | 1.01 |
Recapitulation of the results.
From the results obtained, we notice that the T-slot has a positive effect on our PIFA: a decrease in return loss and an increase in gain.
Changing the substrate has a major effect on the antenna especially on the return loss and the resonance frequency. In this work we studied the effect of substrate change; we used three types of substrate: FR4 epoxy with a permittivity equal to 4.4, Rogers RT/Duroid 6006 with a permittivity equal to 6.15, and Rogers RT/Duroid 5880 with a permittivity equal to 2.2.
Figures 16–18 show the reflection coefficient of the PIFA for the three substrates used:
Return loss (epoxy FR4).
Return loss (Rogers RT/Duroid 6006).
Return loss (Rogers RT/Duroid 5880).
The change of substrate has a major effect on the antenna especially on the reflection coefficient and the resonant frequency used in this work. To achieve the resonance frequency 5.8 GHz, it is necessary to modify the dimensions of the radiating element, which automatically influences the reflection coefficient.
The following table summarizes the results of the three simulations:
From Figures 16–18 and Table 2, we noted that for the substrate FR4 epoxy (εr = 4.4), the antenna resonates at (5.8 GHz) with a return loss is equal to −33 dB.
RO5880 | FR4 epoxy | RO6006 | |
---|---|---|---|
Width | 32 mm | 30 mm | 29 mm |
Length | 26 mm | 26 mm | 26 mm |
5.8 GHz | 5.8 GHz | 5.78 GHz | |
−17 dB | −33 dB | −27 dB |
Recapitulation of the results.
For RO6006 (
The connecting line between the substrate and the radiating element of the PIFA can take several positions, either at the end or at the center of the radiating element.
In this study we compared the results of simulations of the PIFA with three different positions of the connection line.
Figures 19–21 present the return loss of the antenna PIFA for the three positions.
Return loss (Position 1).
Return loss (Position 2).
Return loss (Position 3).
From Figures 19–21 and Table 3, we noted that for = 10 mm the antenna resonates at (5.8 GHz) with a return loss is equal to −33 dB. For
Position | |||
---|---|---|---|
−33 dB | −20 dB | −17 dB |
Recapitulation of the results.
Based on the results we deduced that as one moves away from the end of the radiating element the return loss becomes greater.
Microstrip feed line and the coaxial cable feed are easy to implement; nevertheless this type of power supply generates of parasitic radiation, which affects the radiation pattern. In this study we chose to feed our antenna via a coaxial cable and secondly via a microstrip line. We will compare the results obtained for these two feeding modes. To use these power modes, the microstrip line or the coaxial cable is adapted. For printed antennas this is parameter
In this work, we chose to feed our antenna via a microstrip line and secondly via a coaxial cable. We will compare the results obtained for these two modes of feeding. To use these power modes, it is necessary that the microstrip line or the coaxial cable is adapted. For printed antennas it is the parameter S11 that reflects the adaptation of the antenna. Otherwise, an antenna is considered suitable and isolated when the parameter
Return loss of the antenna supplied via microstrip line.
Return loss of the antenna supplied via coaxial cable.
From Figures 22 and 23, we notice that the reflection coefficient PIFA powered by coaxial cable is equal to −33 and −22 dB for the antenna powered by a microstrip line. So feeding via a coaxial cable is the best technique to power a PIFA.
In this chapter, in the first part, we did an introduction to automatic identification technology, to define the different components of this system, then the frequencies of utilization for this application, and finally the advantages and disadvantages of this technology. In the second part, we presented the design and simulation of a PIFA adapted by a T-slot and powered by a coaxial cable. We studied the effect of changing the type of feed and the substrate type and thus the position of the connecting line between the ground plane and the radiating element. We chose as the resonance frequency of the antenna for RFID applications the frequency 5.8 GHz. We compared the results of simulations obtained by the Ansoft HFSS software. The results obtained are in perfect harmony for RFID applications, either in terms of frequency or bandwidth. Similarly, the significant maxima have been obtained for parameters S11, Gain, SWR, and radiation pattern.
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",metaTitle:"Prior Publication Policy",metaDescription:"Prior Publication Policy",metaKeywords:null,canonicalURL:"/page/prior-publication-policy",contentRaw:'[{"type":"htmlEditorComponent","content":"A significant number of working papers, early drafts, and similar work in progress are openly shared online between members of the scientific community. It has become common to announce one’s own research on a personal website or a blog to gather comments and suggestions from other researchers. Such works and online postings are, indeed, published in the sense that they are made publicly available. However, this does not mean that if submitted for publication by IntechOpen they are not original works. We differentiate between reviewed and non-reviewed works when determining whether a work is original and has been published in a scholarly sense or not.
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\\n"}]'},components:[{type:"htmlEditorComponent",content:'A significant number of working papers, early drafts, and similar work in progress are openly shared online between members of the scientific community. It has become common to announce one’s own research on a personal website or a blog to gather comments and suggestions from other researchers. Such works and online postings are, indeed, published in the sense that they are made publicly available. However, this does not mean that if submitted for publication by IntechOpen they are not original works. We differentiate between reviewed and non-reviewed works when determining whether a work is original and has been published in a scholarly sense or not.
\n\nThe significance of Peer Review cannot be overstated when it comes to defining, in our terms, what constitutes a published scientific work. Peer Review is widely considered to be the cornerstone of modern publishing processes and the key value-adding contribution to a scholarly manuscript that a publisher can make.
\n\nOther than the issue of originality, research misconduct is another major issue that all publishers have to address. IntechOpen’s Retraction & Correction Policy and various publication ethics guidelines identify both redundant publication and (self)plagiarism to fall within the definition of research misconduct, thus constituting grounds for rejection or the issue of a Retraction if the work has already been published.
\n\nIn order to facilitate the tracking of a manuscript’s publishing history and its development from its earliest draft to the manuscript submitted, we encourage Authors to disclose any instances of a manuscript’s prior publication, whether it be through a conference presentation, a newspaper article, a working paper publicly available in a repository or a blog post.
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\n\nSome basic information about the editorial treatment of different varieties of prior publication is laid out below:
\n\n1. CONFERENCE PAPERS & PRESENTATIONS
\n\nGiven that conference papers and presentations generally pass through some sort of peer or editorial review, we consider them to be published in the accepted scholarly sense, particularly if they are published as a part of conference proceedings.
\n\nAll submitted manuscripts originating from a previously published conference paper must contain at least 50% of new original content to be accepted for review and considered for publication.
\n\nAuthors are required to report any links their manuscript might have with their earlier conference papers and presentations in a note to the Academic Editor, as well as in the manuscript itself. Additionally, Authors should obtain any necessary permissions from the publisher of their conference paper if copyright transfer occurred during the publishing process. Failure to do so may prevent Us from publishing an otherwise worthy work.
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\n\nAs with the conference papers and presentations, Authors should obtain any necessary permissions from the newspaper or magazine that published the work, and indicate that they have done so in a note to the External Editor.
\n\n3. GREY LITERATURE
\n\nWhite papers, working papers, technical reports and all other forms of papers which fall within the scope of the ‘Luxembourg definition’ of grey literature do not pass through any extensive peer or editorial review and we do not consider them to be published in the scholarly sense.
\n\nAlthough such papers are regularly made publicly available via personal websites and institutional repositories, their general purpose is to gather comments and feedback from Authors’ colleagues in order to further improve a manuscript intended for future publication.
\n\nWhen submitting their work, Authors are required to disclose the existence of any publicly available earlier drafts in a note to the Academic Editor. In cases where earlier drafts of the submitted version of the manuscript are publicly available, any overlap between the versions will generally not be considered an instance of self-plagiarism.
\n\n4. SOCIAL MEDIA, BLOG & MESSAGE BOARD POSTINGS
\n\nWe feel that social media, blogs and message boards are generally used with the same intention as grey literature, to formulate ideas for a manuscript and gather early feedback from like-minded researchers in order to improve a particular piece of work before submitting it for publication. Therefore, we do not consider such internet postings to be publication in the scholarly sense.
\n\nNevertheless, Authors are encouraged to disclose the existence of any internet postings in which they outline and describe their research or posted passages of their manuscripts in a note to the Academic Editor. Please note that we will not strictly enforce this request in the same way that we would instructions we consider to be part of our conditions of acceptance for publication. We understand that it may be difficult to keep track of all one’s internet postings in which the researcher´s current work might be mentioned.
\n\nIn cases where there is any overlap between the Author´s submitted manuscript and related internet postings, we will generally not consider it to be an instance of self-plagiarism. This also holds true for any co-Author as well.
\n\nFor more information on this policy please contact permissions@intechopen.com.
\n\nPolicy last updated: 2017-03-20
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We welcome chapters presenting research on the many applications of multi-agent studies including, but not limited to, the following key areas: machine learning for multi-agent systems; modeling swarms robots and flocks of UAVs with multi-agent systems; decision science and multi-agent systems; software engineering for and with multi-agent systems; tools and technologies of multi-agent systems.",coverUrl:"https://cdn.intechopen.com/series_topics/covers/27.jpg",hasOnlineFirst:!1,hasPublishedBooks:!1,annualVolume:11423,editor:{id:"148497",title:"Dr.",name:"Mehmet",middleName:"Emin",surname:"Aydin",slug:"mehmet-aydin",fullName:"Mehmet Aydin",profilePictureURL:"https://mts.intechopen.com/storage/users/148497/images/system/148497.jpg",biography:"Dr. Mehmet Emin Aydin is a Senior Lecturer with the Department of Computer Science and Creative Technology, the University of the West of England, Bristol, UK. 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