Open access peer-reviewed chapter

Digital Sorting of Optical Vortices in Perturbed Singular Beams

Written By

Alexander Volyar, Mikhail Bretsko, Yana Akimova and Yuriy Egorov

Submitted: October 11th, 2019 Reviewed: January 29th, 2020 Published: February 20th, 2020

DOI: 10.5772/intechopen.91419

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Abstract

The chapter provides a brief overview of shaping and measuring techniques of the vortex spectra (squared amplitudes and initial phases of vortex modes) including radial indices. The main physical mechanisms causing the formation of laser beams with a complex vortex composition, in particular, in biological media, are indicated, and the need for a digital analysis of vortex spectra is substantiated. It is the analysis of vortex spectra that allows us to find the orbital angular momentum and informational entropy (Shannon’s entropy) of perturbed laser beams in real time. In the main part of the chapter, we consider in detail a new approach for measuring vortex spectra without cuts and gluing of the wavefront, based on digital analyzing high-order intensity moments of complex beams and sorting the vortex beam in computer memory sells. It is shown that certain types of weak local inhomogeneities cause a vortex avalanche causing a sharp dips and bursts of the orbital angular momentum spectra and quick ups and downs of the informational entropy. An important object of analysis is also the vortex spectra of beams scattered by simple opaque obstacles such as a hole, a disk, and a sector aperture.

Keywords

  • optical vortex
  • moment’s intensity
  • orbital angular momentum
  • medical optics

1. Introduction

As is well known, optical vortices [1] accompany light scattering processes due to both simple and complex medium inhomogeneities (see, e.g., [2] and references therein). Scattered light carries a huge array of information, both on the composition and structure of scattering (diffraction) centers, and on the structure of the initial light beam. At the same time, optical information can be read off both by analyzing the frequency spectrum [3, 4, 5] and the spectrum of optical vortices [6, 7]. An important aspect of this problem is the study of biomedical objects [8, 9], for example, the composition of the blood or the reflection of a vortex beam from the skin surface [10] for express diagnostics of skin diseases. The fact is that a vortex beam scattered by the skin is transformed into a speckle-like structure resembling one that occurs when light passes through a medium with weak turbulence [11, 12]. At the same time, the speckle structure is formed by the skeleton of optical vortex array [13, 14, 15]. In turn, the analysis of such a complex vortex structure is conveniently carried out on the basis of vortex fractal techniques [16] (see also [17] and references therein). There are a variety of approaches for the fractal vortex models of laser beams scattered by biological tissues [18, 19] based on the light scattering by nonspherical particles [20] that involves the representation of the wave field in terms of Legendre polynomials. However, a real optical experiment for measuring the vortex spectrum requires the use of particular approaches to the orthogonal basis for the scattered beam expansion in terms of special functions, which can differ significantly from the corresponding theoretical models.

The problem of using the properties of optical vortices in various areas of science and technology requires the development of reliable but simple techniques for measuring the spectrum of optical vortices in complex beams scattered by various objects. Therefore, the attention of many researchers is drawn to measuring the orbital angular momentum (OAM) of vortex beams [7, 21, 22, 23, 24, 25, 26, 27, 28, 29, 30] that is directly related to the spectrum of optical vortices. Really, the complex amplitude Ψxyz of a composite paraxial beam can be written in the form of a superposition of the orthogonal vortex modes ψmxyz

Ψxyz=m=NNCmΨmx.yz,E1

where Cm=Ψψm stands for the mode amplitudes specified by the normalizing condition m=NNCm2=1, and 2N is a total number of vortex modes, Then the average on photon OAM of the composite beam is found by the formula [31].

z=m=NNmCm2.E2

The basis of this expression is an implicit connection between the topological charge m and the OAM zm of a single mode in the beam. However, expression (2) includes the squared modulus Cm2 of a complex number while we are talking about measuring the complex number Cm itself, i.e., its amplitude and the initial phase. The known for us approaches to measuring OAM sorting modes can be divided into four groups according to the methods used. All known for us approaches to measuring OAM spectrum and mode sorting can be conditionally divided into four groups according to the methods used and the effect on the internal beam structure. The most widely used method of holographic spatial filtering of the Laguerre-Gaussian, Hermite-Gaussian, Bessel-Gaussian, Airy-Gaussian and other mode types [22, 23, 24, 30]. At that, this method allows modes sorting, both by topological charge (azimuthal numbers m) and by radial numbers n. The holographic mode sorting resembles the effect of a “white light” decomposition into a color spectrum by means of a prism or diffraction grating. The second type of measurements requires the use of a so-called log-polar transparency and diaphragms [6, 7, 24] placed along the path of a complex beam. Such a structured transparency converts the beam into a set of horizontal or vertical fringes, the pattern analysis of which allows one to obtain the OAM spectrum. The direct application of digital processing of interference patterns of a composite vortex beam [32] and a collinear phase-shifting holography [33] can be considered as the third interference technique. However, measurements in the listed above approaches lead to complete or partial damage of the combined beam and losses of useful information. At the same time, an original approach presented in the papers [26, 27, 34] to measuring the OAM in the vortex beams with a fractional topological charge enables one to avoid the beam damage in the result of employing cylindrical lenses and analyzing the second order intensity moments [35]. Unfortunately, such a simple approach is not applicable for both sorting and measuring the spectrum of vortex modes. In [26, 27], the technique analyzes a fractional OAM [36] of the combined beam as a whole at the focal plane of the cylindrical lens without cutting and gluing the wavefront while the first two techniques distorts radically the initial beam structure. In the technique [26], the measurement of second-order intensity matrix elements was used that enables the authors to devoid breaking down the beam structure. However, it makes sense to use such an approach only if the modes of a complex beam have axial symmetry. The authors of [34] improved the technique by using two cylindrical lenses whose axes are rotated by the angle π/2 relative to each other. This made it possible to measure the fractional OAM for any type of the mode beam symmetry.

At the same time, the measurement of the fractional OAM does not give complete information about the combined beam content. As can be seen from expression (2), the same value of the OAM can correspond to a different composition of vortex modes with squared amplitudes Cm2. For example, in a weakly turbulent medium [37] or optical fibers [38], there is an intense energy exchange between the vortex modes of the singular beam. It makes to change both the magnitude and the spectrum of the vortex modes including their initial phases. To measure the vortex spectrum, a special technique was developed based on the analysis of higher-order intensity moments [25] at the focal plane of a spherical lens. A characteristic feature of this technique is the ability to measure not only amplitudes but also the initial phases of the vortex modes. The point is that the intensity moments at the focal plane of the spherical lens are degenerate with respect to the sign of the vortex topological charge. Therefore, the authors of [25] note that the technique is applicable only for nondegenerate spectra of combined singular beams. In [39], the authors expanded the possibilities of measuring the vortex spectrum, also covering optical vortices with different signs of topological charges due to additional transformations of the Laguerre-Gauss beams (LG) into Hermite-Gauss ones (HG) via astigmatic conversions at a cylindrical lens [40]. However, the method of measuring optical vortices in LG beams of higher orders remained uncovered.

In this chapter, we consider in detail the technique of measuring the vortex spectrum based on the analysis of high-order intensity moments that excludes cuts and gluing of the beam without losses of information on initial mode phases. Unlike the method of holographic gratings that transforms a combined beam into vortex modes with different propagation directions, just as a prism converts “white” light into a spatial frequency spectrum, we will try to demonstrate how a perturbed singular beam can be sorted into vortex modes sited in computer memory cells and then reproduce the beam main characteristics: OAM, information entropy, and initial topological charge in real time. Moreover, knowing the digital spectrum, the beam can be recovered again, and by adjusting the spectral vortex amplitudes we can improve the structure of the transmitted field.

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2. Preliminary remarks

As far as we know, the first theoretical and experimental studies of optical vortex arrays refer to 1991, when the authors of [41] succeeded in reproducing holographically individual letters and words due to ordering optical vortex array in typical phase skeleton on the base of the technique that had been developed back in the early 1980s [29]. However, only after the article [42] by Berry did the studies of the vortex array properties become widespread. As a result, it was shown that the diffracted beam turns into a combined beam containing a large number of optical vortices with integer topological charges. These are sometimes called the beams with fractional topological charges. Using Eq. (2), we can verify that beams with a fractional topological charge also have fractional OAM z. However, in the process of shaping such beams, Eq. (2) requires careful use. Indeed, it is assumed that the functions Ψm of mode beams in Eq. (2) are normalized; otherwise, misunderstandings arise. For example, in [43] considers a Bessel beam diffracted by a holographic grating with a fractional topological charge (see the callout in Figure 1).

Figure 1.

(a) Dependence of the OAM z on the fractional topological charge p: curve 1 is calculated according to Eq. (3) with K=2104m1, curve 2 presents Eq. (5), leader—diffraction grating for p=5/2. (b and c) Computer modeling of the OAM curves zm related with combined beams in Eq. (4): (b) total value of the OAM curves at Ω=10; (c) the characteristic spectral bursts of OAM; curve 1—the OAM bursts Ω=0.4, curve 2—dips of the OAM Ω=14.

If the Bessel beam is represented in the form of a conical beam of plane waves with fractional phase bypath p, then after the inverse Fourier transform we get the non-normalized superposition of Bessel-Gauss modes, including vortices with both positive and negative topological charges:

Ψ=2NGeipπsinm=imJmKReimφ/pm,E3

where Jmx stands for a Bessel function of the first kind and m order, R=r/w0, r and φ are polar coordinates, N=expiK2/2kZ,G=expikr2/2Z, Z=ziz0,w0 is a beam waist at z=0, K is a scale parameter, k is a wavenumber. After the corresponding transformations, we find the OAM of the perturbed beam

z=m=mImK2w02/4/pm2/m=ImK2w02/4/pm2.E4

The result of the plotting is represented by the curve 1 in Figure 1(a). The OAM oscillates at large values of the topological charge p. The integer values of the topological charge p correspond to sharp bursts of the OAM z. However, a small deviation of the parameter p from the integer value causes sharp OAM dips. A completely different situation occurs if the elementary beams in Eq. (3) are normalized, as the authors of [44] do, the OAM oscillations disappear (see Figure 1(b) and curve 2 in Figure 1(c)). In this case, OAM zp obeys a simple relation (see also [45])

z=psin2πp/π.E5

The OAM oscillations disappear (see Figure 1(c), curve 2). As the authors of [45] revealed, a gradual increase in OAM is observed only at small values of the fractional topological charge. In fact, we are dealing with different beams, although the basis for their shaping is the same physical process. As we will see later, the choice of the normalization of vortex modes endows the combined beam with special properties.

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3. Theoretical background of the digital vortex sorting and experimental results

3.1 Nondegenerate case

For a simplest model for our studies, we choose a scalar field of wave in the form of superposition LGnm of the lowest order with the N monochromatic beams, where m>0 and n=0 are the azimuthal and radial indices, respectively, so that all the vortex modes in superposition have the same waist radius w0 at z=0. Let us consider the wave field in the waist plane z=0 in the form [25].

Ψrφz=0=m=0N1CmLGn=0m=m=0N1Cmrmeimφ+βmGrz/Nm,E6

where Nm=2m1m!π stands for the normalization factor, Cm is the mode amplitude, βm is the initial mode phase. We consider the nondegenerate case of the field representationm0orm0 due to the axial symmetry; combined beams with different topological signs ±m are indistinguishable in intensity moments.

Our goal is to analyze the distribution of the wave field intensity rφz=0 in such a way as to express the squared amplitudes and the initial phases of the vortex modes in terms of physically measured quantities in the region of the beam waist. For this, we make use of the intensity moments approach [35] in the form

Jp,q=SMp,qrφrφrdr/Srφrdr,E7

where the intensity distribution is written as

=ΨΨ=m=0N1Cm2Nm2r2mGr2+2m,m=0,m>m`N1CmCmNmNmrm+mcosmmφcosβm,mGr22m,m=0,m>m`N1CmCmNmNmrm+msinmmφsinβm,mGr2,E8

Mp,qrφ stands for the intensity moments function, p,q=0,1,2,. Now the problem is to choose a combination of intensity moments Jp,q in such a way as to exclude all terms of the last two sums and leave only the first one in Eq. (7). The equations for the squared amplitudes and the initial phases are separated if the moment function is written as Mprφ=rp. Then the equations for the squared amplitudes take the form

m=0N1N1+m!m!Cm2=j=0pjpJ2j,2pj,pN2,m=0N1m+1/242m!Γm+1/2Cm2=J2,0+J0,2.E9

The right-hand sides of the linear Eq. (9) are easy to calculate, and the left-hand sides are directly measured experimentally using the Eq. (7) that gives the desired values of the squared amplitudes Сm2.

As intensity of array of the beams depends only on the difference of phase between two pairs of modes, in computation of the initial phases we will assume that one of beams phase is given (let us say β0=0). Now it is important to select the combination of moments of intensity Jp,q that so either the second or the third sum in Eq. (2) is considered in the calculation. It is natural to calculate not all differences of phase βm,m, but only β0,m. However, we did not find such combinations Jp,q that could filter out only terms with β0,m. Generally speaking, to calculate the phase difference βm,m it is required to find the M equations for variables Xm,m=CmCmcosβmm and Ym,m=CmCmsinβm,m in Eq. (2) the second and third sum, number of which is equal to the number of 2-combinations of N elements. It turns out that the number of equations can be significantly decreased if using the moments J2p+1,1 for Xm,m variables and J1,2p+1 for Ym.m variables. The system of linear equations for the phase difference are written in the form

J2p+1,1=122p+1m=0,N1k=0p2pkMm,n1NnNn1Xm,n1+Mm,n2NmNn2Xm,n2,E10
J1,2p+1=122p+1m=0,N1k=0p1pk2pkMm,n1NmNn1Ym,n1+Mm,n2NmNn2Ym,n2.E11

where n1=m2pk±3,n2=m2pk±1, Mm,n1,2=0rm+n1,2+1G2dr. The number of linear equations in each system Eqs. (10) and (11) is K=3N3,N6. It is noteworthy that Eqs. (10) and (11) contain only the terms with an odd difference of indices, including β0,m, so that a finite solution enables us to obtain all phases of the partial beams in the form tanβm,m=Ym,m/Xm,m.

A key element of the experimental setup in Figure 2(a) was a spatial light modulator SLM (Thorlabs EXULUS-4K1), which converted the fundamental TEM00 mode of the He-Ne laser (wavelength λ=0.6328mcm and power 1 mW) into a composite beam with mode amplitudes Cm and initial phases βm. To make this possible, the laser beam was additionally filtered by the system FF. The beam splitter BS formed two working arms of the experimental setup. The beam in the first arm projected by a spherical lens onto the input pupil of the CCD1 camera (Thorlabs DCC1645) is subjected to the image computer processing. The result of the computer processing is a digitization of the beam intensity distribution and calculations of high-order intensity moments Jpq. Additional computer software made it possible to compose a system of linear Eqs. (9)(11) and calculate both the mode amplitudes Cm and their initial phases βm in real time. The second arm was in use for the control measurement of the OAM of the composite beam. For this purpose, the beam was focused by a cylindrical lens CL onto the input pupil of the second CCD2 camera (Thorlabs DCC1645) then the second-order intensity moment Jxy was measured and the average OAM per photon was calculated in accordance with the technique described in detail in the paper [26].

Figure 2.

(a) Model of experimental setup for real-time vortex measurement and value of the OAM, P—polarizer, FF—light filter of space, SLM—space light modulator, L1, L2—spherical lenses with focal length fsh, BS—beam splitter, CL—cylindrical lens with a focal length fcyl, CCD1,2—CCD-color cameras; (b and c) the vortex spectrum of the beam array with N=10: (b) Сm2m, (c) βmm the OAM: theory z=0.39, experiment z=0.42; callout: the intensity distribution and corresponding diffraction grating.

Before proceeding to the current measurements, it was necessary to adjust the experimental setup. For this, a number of calibration measurements were carried out. The digitization of the intensity distribution xy required normalization of the transverse coordinates x,y in units of the Gaussian beam waist at the plane of the CCD camera. To measure the initial beam waist radius w0, the second-order intensity moments J12 were used in accordance with the beam quality measurement method [46]. In order to ensure calibration measurements, a special computer program was developed that assigned random values of the amplitudes and initial phases of the vortex modes in Eq. (1) due to the random-number generator. Then, an appropriate diffraction grating was formed on the liquid crystal element of the SLM modulator and the calibration beam was restored. A typical intensity distribution of the calibration beam is shown in the callout of Figure 2(c). The corresponding spectra of the squared amplitudes Сm2 and initial phases βm are presented in Figure 2(b) and (c). Red and blue colors in Figure 2(a) and (b) present experimental and theoretical data, respectively. Note that the OAM measured in the second arm was z=4.2 and the first arm calculated according to Eq. (2) was z=4.5, while the theory gives z=4.9. The measurement error for N=10 beams did not exceed 3–4% for amplitudes and 5–6% for phases. The most interesting effect is observed in the region of OAM oscillations in Figure 1(a) with a characteristic perturbation of the holographic grating in Figure 2(c). This effect is accompanied by a sharp restructuring of the vortex spectrum. For small perturbations of the singular beam, additional vortex modes arise only near the initial value of the topological charge m=M (see [47]). However, in general case of the hologram perturbation, vortex modes with opposite signs of topological charges appear. Such a vortex spectrum reconstruction cannot be detected using the above approach. It is required to expand the measurement technique.

3.2 Degenerate case and vortex avalanche

We consider the case when the initial LG beam with a zero radial index n=0,m0 is subjected to local perturbation at the central region of the holographic grating. As a result of the perturbation, vortex modes with various types of topological charges appear in the beam. The method of the beam expansion in a series over the vortex modes depends on the type of the grating perturbation. We suppose (and then prove) that the chosen perturbation does not excite LG modes with radial indices n=0, but only modes with different topological charges m appear [39]. Then we write the complex amplitude of the perturbed beam in the form

ΨRφz=m=NNCmRmeimφGRMmσm+1z,E12

where Mm is a normalized factor and σz=1iz/z0.

It is important to notice the intensity moments Jp.q are degenerate with respect to the sign of the vortex topological charge m in the case of axial symmetry of the modes in Eq. (12). To remove degeneracy of the intensity moments, it is important to change symmetry of singular beams, but without destroying of structure beams so that the vortex modes with opposite topological charges in sign have distinct geometric contours. Such a requirement provides by the astigmatic transformation with a cylindrical lens of the Laguerre-Gauss beam, which was considered detail in [34] (the general theory of paraxial astigmatic transformations can be found in [41]). We suppose that the cylindrical lens with a focal length f is located at the plane z=0. A paraxial beam with complex amplitude (12) is projected at the lens input. The plane of the beam waist is matched with the plane of the lens. Besides, we restrict our study to zero initial phases of mode beams, i.e., amplitudes Cm are real values. Then, following [34], we write the complex amplitude of a combined beam at the wave diffraction zone as

ΨCLxyz=m=NNAmHmFexpΦ,E13

where Am=iz0z1qq0w0q0m1q02q2,Φ=ik2zx2+y2z0zw0q2x2z0zw0q02y2,F=z0w0ziq0qxqq0yq2q02,q02=1iz0z,q2=1+iz0z1,z1=zfzf..

Let us consider new normalized coordinates so that the beam axes are directed by an angle π/4 relative to the axes of the cylindrical lens: u=x+y/w0,v=xy/w0, we will consider field of paraxial beam in double focus plane z=2f, and also require that z0/2f=1. Then distribution of the beam intensity is written as

=ΨCL2=m,n=0NCnСmAm,nNm,nHnu2Hmu2+m,n=1NCnСmAm,nNm,nHnv2Hmv2+n=0,m=1NCnСmAm,nNm,nHnu2Hmv2+n=1,m=0NCnСmAm,nNm,nHnv2Hmu2expu2+v22E14

where Hnx is Hermite polynomials, Am,n=1n+meimn4π, Nn,m2=π4wo2n+m2n+m+1n!m!. As can be seen from Eq. (14), the terms corresponding to optical vortices with positive and negative topological charges are only partially divided. The last two terms characterize the cross terms CnСm and CnСm. Besides, the first two terms also contain cross amplitudes CnСm and CnСmnm. On the other hand, our task is to measure only the squared amplitudes Cm2. It is important to note, that the factors Am,n=An,m=i with the difference of the indices mn=2 in Eq. (14) are imaginary, therefore the cross terms of the beam intensity distribution with such indices difference disappear.

It seems that for solving this problem it is reasonable to choose intensity moment functions in the form of Hermite polynomials Eq. (14) as Mp,0u=Hpu/2 and M0,qv=Hqv/2. Next, one can use the orthogonality condition of the HG beams and write a system of linear equations, the number of which is equal to the number of variables, as was done above for a non-degenerate vortex array. However, as shown by the assessed computations, as the indices p and q increase along with the 2N variables Cm2, the 2N6 cross terms C±nС±m and C±nСm are also added. The system of Eq. (14) cannot be closed. However, one can act otherwise. First, we make two Fourier transforms of the intensity distribution xy in the form

ξ=cosξu2x.ydxdy,η=cosηv2x.ydxdy.E15

In particular, the terms m.n in the intensity distribution are

m.nξ=cosξu2x.ydxdy=n=0NCn22n+1/2Nn,nξ2nLnξ22eξ24+m,n=0,mn0,2NCnСn+2m1n+2m2n+1/2Nm,nξ2mLn2mξ22eξ24,E16

Thus, after the Fourier transform the distribution of intensity ξη contains all the squared amplitudes, and, also, the cross terms with the difference mn=±4. The cross terms т,m and m,n refer to vortices with positive and negative charges. Besides, the terms т,n+2mξ includes amplitudes Сn2 with the similar coefficients, and the member т,n+2mξ includes amplitudes Сn2 with only different coefficients. The expressions are received for the terms, that т,n+2mη and т,n+2mη, if we swap the signs of the indices.

The equations for squared amplitudes С±n2 will be found, if we will make use the full basis of the Laguerre-Gaussian modes for expansion of the intensity moments:

Jp,2q+=ξLp2qξ22ξ/J00,Jp,2q=ηLp2qη22η/J00,E17

where J00 is a total beam intensity and Lpqx is Laguerre polynomials. Then, using [39], we find a system of linear equations

Jp,q=n=1NCn2+2q+p!1/2pp!42q+p+1m,n=1N2m+n!1/2nn!42m+n+1NnmC±nCm/J00,E18

The system of Eq. (18) enables us to find the values of the squared amplitudes via the measured values of the intensity moments Jp,q±. Each equation contains 2N terms for amplitudes Cm2 and N3 cross terms CmCn. Increasing the value of the indices p and q does not change the number of variables, so the system of Eq. (18) can be closed. Note that each of the Eq. (18) can be solved independently of each other and find the amplitudes Cm2 and Cm2. The total number of linear equations is relative to signs ±, so that the systems can be easy solved for finding the squared amplitudes in real time using modern computer software.

For measurements, the experimental setup shown in Figure 2(a) was used. However, in contrast to the non-degenerate case, the main experimental data were measured in the second arm, provided that the detection plane was located at the double focus region of the cylindrical lens, while the first arm was used for general adjustment [39].

We will implement the above technique for a new type of combined beams with conspicuous dips and bursts in the OAM spectrum similar to that shown in Figure 1(a) and (b). Let us write the complex amplitude of the combined vortex beam in the form

Ψrφz=sineim=NNcosmπ/2sinmπ/2Ωmm!Mm+δpRmeimφσzm+1expR2,E19

where Ω is a scale parameter, δp stands for the perturbation of the holographic grating responsible for shaping the beam, M is a topological charge of the non-perturbed forked grating. Factors cosmπ/2 or sinmπ/2 thin out the vortex spectrum remaining the modes with either even or odd m indices. This makes the dips in the OAM spectrum more distinct. The complex amplitude (12) corresponds to the OAM in the form

z=m=NNmcos2mπ/2sin2mπ/2Ω2mm!2Mm+δp2/m=NNcos2mπ/2sin2mπ/2Ω2mm!2Mm+δp2.E20

Figure 1(b) and (c) displays the case of even vortices beams in the curves of zp. The spectrum of OAM in Figure 1(b) characterizes the general view of resonant bursts and dips. The Ω parameter of scale admits displace along the axis of the resonant regions p=M+δp. Figure 1(c) (curves 1 and 2) describes their characteristic features. In the even vortex modes of integer topological charge are located resonant dips. Swaps of the cosine with the sine in Eq. (19) displaces along the axis p of the resonant regions by one. Increase of the topological charge M is accompanied by resonances compression, until their depth gets become approximately equal to M at Ω=18 and p<6. For large parameters Ω>>20, the OAM is doubled z=2M in range of the initial topological charges M. As was shown in [47, 48], a perturbation δp causes a local distortion of the forked grating defect for the large values parameter p shown in Figure 3(a).

Figure 3.

Forked defect perturbations of the holographic gratings with (a and b) M=20, Ω=2.1, (c and d) M=4, Ω=14: (а) δp=103, (b) δp=0.1, (c) δp=103 (d) δp=0.5, callouts: intensity distributions of the beams restored by the perturbed holograms.

As the perturbation grows the area of the hologram defect increases (Figure 3(b)). Small variations in the holographic grating structure lead to a cardinal reconstruction of the vortex spectrum (Figure 4(a)). Weak perturbations δp102 of the grating cause an avalanche of optical vortices. The satellites appear in the OAM spectrum, the maxima of which has topological charges less than the initial M. The energy of the basic mode M flows partially into the spectral satellites, that are generated both in the region of positive m>0 and negative m>0 topological charges.

Figure 4.

Experimental vortex spectra Cm2m for perturbed singular beams with (a) M=20, Ω=3.5 and (b) Ω=18,M=4; callouts: intensity distributions at the beam waist after spherical (sph) with focal length f=0.1m and cylindrical (cyl) lens with fcyl=0.5m; red color—an initial mode.

For large perturbations δp0.1, a vortex avalanche picks almost all the energy out of the basic mode. The vortex avalanche at small deviations δp of the topological charge from integer values M immediately causes a resonance dip in the OAM spectrum (Figure 5(a)). With increasing M the depth of the dip decreases while its shape is distorted (see Figure 5(b)).

Figure 5.

Dips and bursts in the OAM spectrum zp at various beam parameters Ω and M,p=M+δp: (a and b) M=20, (c and d) M=4; solid lines—theory, circles—experiment.

Absolutely other situation arises when the holographic grating with M>10 and a forked defect is subjected to a small perturbation. As shown in Figure 3(c), even a weak perturbation δp=0.001 changes drastically the entire relief of the holographic grating although the intensity distribution. In the result, even small differences in the grating relief affects inevitably the shape of the vortex spectrum Cmm2 and Ω>10 induce the vortex avalanche (see Figure 4(b)). However, the avalanche type differs significantly from that in the previous case. Indeed, as well as in the above case, the perturbation provokes appearing resonance satellites with both positive and negative topological charges (TC). However, their values are always greater than those of the initial TC. In this case, energy is also pumped from the basic mode to the satellites but with higher topological charges under the condition of the resonance m=p. In the OAM spectrum, it looks like the OAM burst at the resonance as shown in Figure 5(c) and (d) but the maxima z are at the region of fractional values p. As the scale parameter increases, the height of the flash decreases, and the resonance circuit broadens (Figure 5(d)).

Further increasing the parameter p (Ω=const) is accompanied by smoothing the curve zp so that zmax2p except for the OAM dips at the integer values m=p.

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4. OAM, informational entropy and topological charge of truncated vortex beams

A special case is represented by natural changes of the vortex spectrum due to external influences on the laser beam (diffraction by opaque obstacles, external interference in the beam, etc.). The simplest opaque obstacles are the sector, circular and annular apertures where we stop our attention using a simple technique of the vortex digital sorting.

4.1 Sector aperture

Let us consider propagation a scalar beam of Laguerre-Gaussian LG0m with a zero radial index p=0 and an azimuthal index (a topological charge) m through the rough regular sector aperture obstacle, that an angle shown in Figure 1. The edge of sector touches axis of the beam. The field of beam at the initial plane z=0 can be represented as [49].

Ψmrφα=ρ/wmeimφeρ2/w2=rmeimφer2,α<φ<2πα,E21

where r=ρ/w. w is a beam waist radius at the plane z=0, ρ and φ represent polar coordinates. We rewrite the beam field (1) formed by the rigid-edges aperture with the half angle α as a sum of non-normalized Laguerre-Gauss beams LGpm in the form

Ψmrφα=n=Cm,nαLG0nrφ=n=Cm,nαrneinφer2,E22

where the beam amplitudes are

Сm,nα=1mnΓm+n2+1sinmnπαmn/π2mn2n!,E23

where Γx is a Gamma function. The terms in the series (23) with radial indices p0 disappear due to orthogonality of the LG modes.

The complex amplitude (22) can describe the spatial evolution of the perturbed beam if we replace rr/σ and multiply the sum by σ where σ=1iz/z0. Figure 6(b) and (c) shows a computer simulation (Figure 6(b)) and experiment (Figure 6(c)) of the intensity distribution rφz=ΨΨ along the vortex beam length with m=15 modulated by the sector aperture with α=π/4. It is important to note, that the cut out dark sector from the beam intensity distribution does not lead to its self-healing. When the beam propagates, the dark sector rotates synchronously. We showed, both theoretically and experimentally, that beam self-healing does not occur at any beam length z even at a very small sector angle α.

Figure 6.

(a) Sketch of the hard-edged aperture (D) installed at the cylindrical lens plane (CL). Images LG and HG beams illustrate the astigmatic transformation of a single vortex beam. (b and c) Intensity distribution rφz of the vortex beam with m=15 along length Z=z/z0 perturbed by a hard-edged sector diaphragm with α=π/4: (b) theory, (c) experiment.

4.1.1 The vortex spectrum

We consider vortex beams spectra for topological charge that most clearly reflect properties of the sector perturbation. Computer simulation and experimental data of typical vortex spectra is shown in Figure 7. We revealed a clear maximum of vortex mode intensity Сm,n2 for the initial topological charges n=m=5 with α=45°. The short part of the beam intensity redistributed symmetric at the neighboring vortices orders. But, if we increase the angle α, we see a violation of the symmetric distribution of intensity among the vortex modes. There formed a second maximum in the spectrum range of negative topological charges n<0. It is important to note, that the authors of Ref. [50], taking into consideration the optical uncertainty principle, also plotted the vortex spectrum for a topologically neutral beam m=0 and a beam with a small topological charge m=2 at the angle of aperture α=45°. The authors did not detect a maximum of spectra in the negative region of topological charges. As we presented above, the emergence of the second intensity maximum is possible only at sufficiently large angles of overlap of beam α and also large topological charges m of the initial singular beam.

Figure 7.

Distribution of vortex beams spectrum Cm,n2 with charges m=5 perturbed by the hard-edged aperture with the sector adjacent angle β=πα, the solid line is spectrum outline.

4.1.2 The orbital angular momentum

The OAM per photon of a complex perturbed beam can be calculated in accordance with Eq. (23). The mode amplitudes are given by the normalized field Ψm of the Laguerre-Gauss beams so that the squared amplitudes Сm,n2 and С¯m,n2 are obeyed a simple relation С¯m,n2=2n2n!Сm,n2. The changes of OAM zαm after increasing the aperture angle α (decreasing the adjacent angle β=πα) is presented by Figure 7(a) for topological charges m=5,m=10 and m=15 of the initial vortex beam.

The OAM is practically unchanged a wide range of angles and remains almost equal to the initial OAM, despite the rapid increase in the number of vortex states (see Figure 8(a)). After the second spectral maximum is formed in the negative region of topological charges Figure 7, there is a sharp decrease of the OAM. The OAM is equal to zero already at the angle β2°.

Figure 8.

Computer simulation of (a) the OAM zαm and (b) information entropy HIαm for the initial topological charges, m=5,10,15; (c) transformation of the vortex TC Mof the perturbed beam via variation TC of the initial beam; (d) maximal TC mmax of the spectral vortex satellites via perturbation Ω of the perturbed holographic gratings; (solid lines); crosslets ×, circlets and squares (□) are correspondent experimental data.

4.1.3 Informational entropy (Shannon’s entropy)

The normalized squared amplitude Сn201 in the Eq. (23) can be treated as a conditional probability Pn/m of finding out a vortex beam in the state n among of 2N states (see, e.g., [51] and references therein). This approach to counting a number of vortex states can be used for the Shannon Entropy [51] and is written as

HI=n=0NPn/mlog2Pn/m=n=0NCn2αmlog2Cn2αm>0.E24

The Shannon entropy (24) characterizes the amount of uncertainty (randomness) that arises when a perturbation acts on a vortex beam. For example, in the case of the same amplitudes of the mode beams, the Shannon entropy of HI=2 means that to remove the uncertainty it is necessary to expend 1 bit of information.

In Figure 8(b) presents the dependence of the Shannon Entropy HI on the angle α for various of number topological charges m. In a broad range of aperture angles 0<α<7π/8, the informational entropy HI increases equally for any topological charges m while the OAM z does not change (see Figure 8(a)) which corresponds to the same changes in the spectrum of vortex states in Figure 7.

4.1.4 The topological charge

According to Berry [42], the topological charge of the vortex array is defined as the difference of the fluxes of vortex trajectories through the beam cross section taking into account vortex directions and “weights,” and is calculated as

M=12πImlimr02πφΨm/Ψm.E25

Berry showed [42] that the vortex beam TC has always integer values when the spiral phase plate is perturbed equal to the integer value of the unperturbed plate step. We investigated the changes of the TC under the beam sector perturbations [52] and perturbation of the holographic grating [47]. Note that all further calculations are based on the requirement that the perturbation does not introduce changes in the mode phases. We performed a series of computer TC estimations of the perturbed beam (20) for various initial TC. The following restrictions were used. As the spectra of vortices in Figure 7 show, the squared mode amplitudes quickly tend to zero as their TC increases. Therefore, we can restrict ourselves to a finite mode numbers Сmn2103. The half-width beam radius can be estimated at the maximum intensity of the initial vortex beam rM=m/2. Therefore, in Eq. (25) we replaced the limit r by r3rN. The results of computer simulation are shown in Figure 8(c). It can be seen from the figure that the total topological charge M at α=3π.4 remains equal to the initial TC of the unperturbed beam M=m. Computer calculations for sector aperture angles α=π/4,π/2,30π/31 show similar results. Therefore, we assume that, in the general case of arbitrary angles, the initial TC will be preserved under sector perturbations. We also examined the constancy condition TC under the perturbation of the holographic grating considered above and made sure that this condition is strictly satisfied. Moreover, we traced the maxima displacement of the spectral satellites in the vortex avalanche in Figure 4 [47] and convinced (see Figure 8(d)) that their TC cannot take fractional values.

4.2 Circular and annular apertures

The problem of the birth and annihilation of phase singularities has been considered as far back as at the beginning of the last century in connection with the peculiarities of light diffraction at the edges of the half-plane or lenses and micro-objectives of telescopes and microscopes (see [53] and references therein). As a rule, the discussion came down to the technique of suppressing the corresponding aberrations. In this section, we focus on the digital vortex sorting after beam diffraction by the circular and annular apertures addressing the Shannon entropy problem of the diffracted combined vortex beams.

Note also that recently, special attention has been paid to studies on increasing the information capacity of optical channels due to LGnm modes with various radial indices n, but a constant topological charge m [54]. Such modes are sorted using the holographic grating techniques and a single phase screen [55]. In this section, we will focus on the digital sorting of LG modes with various radial indices.

We consider the perturbation of the vortex LG0m beam at the z=0 plane with a ring aperture so that its complex amplitude is written in the form (see also Figure 10a)

Ψm=rmeimφexpr2,R<r<R+h.E26

If the axis of the annular aperture coincides with the beam axis then the perturbation excites only LG beams with the same TC (m=const) but different radial indices n (this follows from the condition of orthogonally of LG beams). The perturbed beam field can be represented as an expansion over LG beams

Ψm=n=0Cm,nrmLnm2r2eier2.E27

The LG vortex modes amplitudes restricted by the ring of thickness h, we find for the field difference the beams passing simultaneously through the circular aperture of radius R+h and the opaque disk of radius R. As a result we obtain

Сm,nR=0ΨmLGnmrdr=2R+h2m+1e2R+h21F11nm+22R+h2/m+1m!2R2m+1e2R21F11nm+22R2/m+1m!,E28

where 1F1 is a confluent hypergeometric function and we used the integrals from [56]. The expression (28) together with Eq. (27) allows covering three cases: (1) a circular aperture, R=0,h=R0; (2) an opaque disk R=R0,h=0; and (3) an annular aperture R,h0. An important property of mode amplitudes (28) is that the perturbation of a singular beam with a defined TC via these types of axial apertures does not excite vortex modes with other TC. This means that the OAM z does not change due to such a perturbation process. Does this mean that the perturbed vortex beam completely restores its initial properties during propagation, i.e., possesses the self-healing effect? We will peer into this process carefully.

Recall that under the action of axial perturbation, vortex modes with new topological charges do not appear in the perturbed beam. Therefore, the digital sorting of vortex modes in a perturbed beam can be carried out in accordance with Eq. (15) for the nondegenerate case (see Section 3.1). In this case, as a function of moments Mp,qrφ should choose the forms Mp,q=sinrLpk2r2 or Mp,q=cosrLpk2r2 while in the intensity distribution rφ use the complex amplitude (26). Variation of the indices p and k enables us to obtain a closed system of linear equations for the squared amplitudes Cm,n2.

The experimental results of measuring the vortex spectra are shown in Figure 9, where the average values of the squared amplitudes are plotted along the ordinate axis. A characteristic feature of the dependences Cm,n2n is long spectral tails, which are omitted in the figures, but which make a significant contribution to the calculation of information entropy. Truncation of a topologically neutral beam (m=0) with a circular aperture in Figure 9(Ia) leads to overlapping many side rings, resulting in a wave-like form of the spectral tail. In the perturbed vortex beams shown in Figure 9(Ibc), a broadening of the vortex spectrum and a decrease in the tail amplitudes are observed. Such characteristic features of the vortex spectra insert significant uncertainty into information carried by the vortex beam, which is represented as the dependence of information entropy HI on the aperture radius R0 in Figure 9(Id). It is noteworthy that even small variations in the aperture radius lead to changes in the entropy HI that grow with increasing TC. Similar changes in the entropy HIh shown in Figure 9(IId) occur when a vortex beam is perturbed by a annular aperture, which are the result of transformations in the vortex spectra in Figure 9(a–c). The presented results show that any external interference in the beam immediately affects the uncertainty of the vortex beam state, the magnitude of which can be estimated by measuring informational entropy.

Figure 9.

The vortex spectra Cm,n2 and the Shannon entropy HIh of the perturbed singular beams with different TC m: (I) the circular aperture; (II) the annular aperture; (Id) the Shannon entropy HI via the aperture radius R0; (IIh) the Shannon entropy HI via the annular width, curves 1 and 3 correspond to the TC m=0,m=2,m=4, respectively; callouts: corresponding intensity distributions.

Another interesting feature of the axial aperture action is manifested under the combined vortex beam perturbation consisting of two vortex beams with the same values but different TC signs (m and m). If the amplitudes of the beams are the same, then the complex amplitude of such a combined beam is described by Eq. (28) when replacing the phase factor expi2cos. Figure 10(b–d) illustrates the intensity distribution of such perturbed beams at the measurement plane. Each of these beams receives the same perturbations, regardless of the sign of their TC. Even if the beam amplitudes are different, they receive the same amount of the vortex state uncertainty. However, this apparent indistinguishability of the modes can be easily detected experimentally due to opposite phase circulation of the fields, and the modes can be sorted out in different memory cells.

Figure 10.

(a) Sketch of the annular aperture. (b–d) Intensity distributions of the singular beams with TC m=5 and m=5 perturbed by the circular aperture with the radius (b) R0=0.5, (c) R0=0.1 and (d) the annular aperture with R0=0.5,h=0.2.

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5. Conclusions

We examined the technique of digital sorting of vortex modes that makes it possible to measure in real time the vortex spectrum (squared amplitudes and initial phases) including radial indices, OAM, and informational entropy of perturbed singular beams. The considered approach is based on the measurement of intensity moments of higher orders and a digital solution of a linear equations system that eliminates the cuts and gluing of the beam wavefront without losing information on the modes initial phases. Moreover, the digital vortex spectrum also enables us to restore the initial combined beam and, correcting parameters of the spectral modes, to improve its characteristics.

The digital approach has been tested on vortex beams free of wave defects perturbed both by local defects of holographic gratings responsible for the beam generation and by the sectorial, circular and annular aperture. We revealed that a local perturbation of the holographic grating near the central forked defect causes bursts and dips in the OAM spectrum. The depth and height of the spectral dips and bursts are controlled by the parameters of the holographic grating and can vary over a wide range. The perturbation inserted by the sector aperture is regulated by the sector angle. Over a wide range of sector angles, the beam OAM remains almost unchanged. However, when the sector angle is relatively large, so that most of the light flux is cut off by the aperture, the optical uncertainty principle begins to act, and the OAM sharply decreases to almost zero that is accompanied by a rapid growth of the Shannon entropy. At the same time, the beam topological charge remains unchanged for any sectorial perturbations. The axial perturbation via a circular and annular aperture does not change either the OAM or topological charge. However, a wide range of Laguerre-Gauss modes with the same topological charges but different radial indices leads to a rapid increase in information entropy as the pupil of the circular aperture or the ring thickness of the annular aperture decreases. This allows not only to estimate the noise level in the optical information transmission line, but also to record external interference in the information flow. We also note that the digital sorting of optical vortices in a perturbed light flux opens up broad prospects for its employment for medical express-diagnostics of skin diseases, since, for example, this allows us to detect slight changes in the vortex spectrum of a laser beam scattered by inflamed or dehydrated skin areas.

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Acknowledgments

The authors are grateful to E. Abramochkin (Samara Branch of the Lebedev Physical Institute, Russian Academy of Sciences, Samara, Russia) for a useful discussion of the mathematical approach. The reported study was funded by RFBR according to the research project № 19-29-01233.

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Written By

Alexander Volyar, Mikhail Bretsko, Yana Akimova and Yuriy Egorov

Submitted: October 11th, 2019 Reviewed: January 29th, 2020 Published: February 20th, 2020