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Depth multiplexing in an orbital angular momentum holography based on random phase encoding

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Abstract

The orbital angular momentum (OAM) holography has been identified as a vital approach for achieving ultrahigh-capacity in 3D displays, digital holographic microscopy, data storage and so on. However, depth has not been widely applied as a multiplexing dimension in the OAM holography mainly because of the serious coherence crosstalk between different image layers. The multi-layered depth multiplexing OAM holography is proposed and investigated. To suppress the coherence crosstalk between different image channels, random phases are used for encoding different image layers separately. An image can be reconstructed with high quality at a specific depth from an appropriate OAM mode. It is demonstrated that the depth multiplexing of up to 5 layers can be achieved. This work can increase the information capacity and enhance the application of the OAM holography.

© 2022 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement

1. Introduction

The OAM holography proposed by Gu. et. al is identified as a vital approach for achieving ultrahigh-capacity multiplexing [1,2]. Owing to the theoretically unlimited helical mode index of an OAM beam, a large number of OAM-dependent information channels could be multiplexed in a single hologram, which holds great promise for ultrahigh-capacity holographic devices and systems. After that, complex-amplitude metasurface-based OAM holography [3], polarization-encrypted OAM holography [4], modulated OAM holography [5,6], perfect OAM holography [7], ellipticity-encrypted OAM holography [8], and high-dimensional nonlinear OAM holography [9,10] have been proposed in recent years. In addition, combining the deep learning or optical diffractive neural network with OAM holography has been investigated as well [11,12], which paves a way for optical communication, ultrahigh-security optical encryption and optical storage.

Depth is another possible multiplexing dimension for further increasing the information capacity. A relevant method is the ultra-dense perfect optical OAM multiplexed holography [7], in which the OAM modes are discriminated both radially and angularly by utilizing the “cone phase” degree of freedom. Another is the complex-amplitude metasurface-based OAM holography in the momentum space [3]. It is capable of multiplexing up to 200 independent channels on two depth planes, allowing holographic videos to be displayed. However, depth has not been widely applied as a multiplexing dimension mainly because of the serious coherence crosstalk between different image layers.

By utilizing the depth degree of freedom, we investigate the multi-layered depth multiplexing OAM holography (DM-OAMH). The rest of the paper is organized as follows. The DM-OAMH is introduced in Section 2. The method of suppressing the coherence crosstalk is presented in Section 3. Then simulation and experimental implementation are presented in Section 4, and the paper is summarized in Section 5.

2. Depth multiplexing OAM holography

In the OAM holography, the electric field on the hologram plane H(ξ, η) and that on the image plane E(x, y) form a Fourier pair, where x and y represent the abscissa coordinates on the image plane, and ξ and η denote those on the hologram plane. Given a target image E(x,y), the relationship can be expressed as

$$H({\xi ,\eta } )= \int\!\!\!\int {E({x,y} )} \textrm{exp} [{i({\xi x + \eta y} )} ]\textrm{d}x\textrm{d}y$$

Here, a depth multiplexing OAM hologram can be generated by combining multiple OAM holograms and a Fresnel zone plate [1], where the Fresnel zone plate is used to control the reconstruction depth. A hologram encoded by multiple image channels can be expressed as

$${H^{mul}}({\xi ,\eta } )\textrm{ = }\sum\limits_{n = 1}^N {{H_n}({\xi ,\eta } ){e^{i{l_n}\varphi }}Q\left( { - \frac{1}{{{f_n}}}} \right)}, $$
where N presents the number of image channels, φ=atan(η/ξ) is the azimuth angle, Hn(ξ,η) is the n-th OAM hologram obtained by the inverse Fourier transform of the sampled target image. The sampling period of the image is determined by the spatial frequency of the OAM mode [6]. The term Q(-1/fn) is the encoded Fresnel zone plate, where fn is the focal length used to control the reconstruction depth, and $Q(b )= \textrm{exp} [{i\pi b({{\xi^2} + {\eta^2}} )/\lambda } ]$ is a quadratic phase function.

In order to decode the m-th channel image channel Hm, an OAM beam with a helical mode index l=-lm should be used to illuminate the hologram. The resulting electric-field distribution after the hologram can be expressed as

$${H^{rec}} = {H_m}Q\left( { - \frac{1}{{{f_m}}}} \right) + \sum\limits_{n = 1\atop n \ne m}^N {{H_n}{e^{i({{l_n} - {l_m}} )\varphi }}\textrm{exp} Q\left( { - \frac{1}{{{f_n}}}} \right)} ,$$

The reconstructed electric-field distribution at z = fm can be calculated by the Fresnel diffraction [13]

$${E^{rec}}({x^{\prime},y^{\prime}} )= \frac{{\textrm{exp} ({ik{f_m}} )}}{{i\lambda {f_m}}}\int {\int {{H^{rec}}({\xi ,\eta } )\textrm{exp} \left( {\frac{{ik}}{{2{f_m}}}[{{{({x^{\prime} - \xi } )}^2} + {{({y^{\prime} - \eta } )}^2}} ]} \right)\textrm{d}\xi \textrm{d}\eta } } ,$$
where x’ and y’ are the abscissa coordinates on the reconstruction plane. Combining Eq. (3) and Eq. (4), the reconstructed image can be expressed as
$$\begin{aligned} {E^{rec}}({x^{\prime},y^{\prime}} ) &= \frac{{\textrm{exp}({ik{f_m}} )}}{{i{f_m}\lambda }}\textrm{exp}\left[ {\frac{{ik}}{{2{f_m}}}({x{^{\prime}{^2}} + y{^{\prime}{^2}}} )} \right]{E_m}({x^{\prime},y^{\prime}} )\\ &+ \sum\limits_{n = 1\atop n \ne m}^N {\frac{{\textrm{exp}({ik{f_n}} )}}{{i{f_n}\lambda }}\textrm{exp}\left[ {\frac{{ik}}{{2{f_n}}}({x{^{\prime}{^2}} + y{^{\prime}{^2}}} )} \right]{F_n}({x^{\prime},y^{\prime}} )} \end{aligned}$$
where Fn(x’, y’) is the crosstalk term caused by other image channels, which can be expressed as
$${F_n}({x^{\prime},y^{\prime}} )= {E_n}({x^{\prime},y^{\prime}} )\otimes \cal {F}\{{\textrm{exp} [{i({{l_n} - {l_m}} )\varphi } ]} \}\otimes Q^{\prime}\left( {\frac{1}{{{f_m} - {f_n}}}} \right). $$

Here ${\otimes}$ denotes convolution and $\cal {F}$ denotes the Fourier transform, $Q^{\prime}(b )= \frac{{\textrm{exp} [{ik({{f_m} - {f_n}} )} ]}}{{i({{f_m} - {f_n}} )\lambda }}$ $\textrm{exp} [{i\pi b({{{x^{\prime}}^2} + {{y^{\prime}}^2}} )/\lambda } ]$. $\cal {F}\{{\textrm{exp} [{i({{l_n} - {l_m}} )\varphi } ]} \}$ is the doughnut-shaped intensity structure. The terms $\frac{{\textrm{exp}({ik{f_m}} )}}{{i{f_m}\lambda }}$ and $\frac{{\textrm{exp}({ik{f_n}} )}}{{i{f_n}\lambda }}$ in Eq. (5) have a relatively insignificant effect. Meantime, the terms $\textrm{exp}\left[ {\frac{{ik}}{{2{f_n}}}({x{^{\prime}{^2}} + y{^{\prime}{^2}}} )} \right]$ and $\textrm{exp}\left[ {\frac{{ik}}{{2{f_m}}}({x{^{\prime}{^2}} + y{^{\prime}{^2}}} )} \right]$ play as a low-pass filter [14], which are ignored here. As a result, Eq. (5) can be simplified as

$${E^{rec}}({x^{\prime},y^{\prime}} )\propto {E_m}({x^{\prime},y^{\prime}} )+ \sum\limits_{n = 1\atop n \ne m}^N {{F_n}({x^{\prime},y^{\prime}} )}$$

The reconstruction intensity can thus be expressed as

$$\begin{aligned} {I^{rec}} &= {E^{rec}}({x^{\prime},y^{\prime}} ){E^{rec}}{({x^{\prime},y^{\prime}} )^ \ast } = {|{{E_m}({x^{\prime},y^{\prime}} )} |^2} + \sum\limits_{n = 1\atop n \ne m}^N {{{|{{F_n}({x^{\prime},y^{\prime}} )} |}^2}} \\ &+ {E_m}({x^{\prime},y^{\prime}} )\sum\limits_{n = 1\atop n \ne m}^N {{F_n}{{({x^{\prime},y^{\prime}} )}^\ast }} + {E_m}^\ast ({x^{\prime},y^{\prime}} )\sum\limits_{n = 1\atop n \ne m}^N {{F_n}({x^{\prime},y^{\prime}} )} \end{aligned}$$

The first term is the desired image with a pattern of Gaussian-shaped spots, while the last two terms are small due to the doughnut-shaped intensity structure of Fn. Each Gaussian spot in Em corresponds to a doughnut-shaped spot in Fn. The inner projects of their complementary intensity distributions are close to zero. As a result, the last two terms can be ignored. The second term is the main coherence crosstalk resulting from other image channels, which can cause dramatic intensity oscillation and reduce the reconstruction quality.

3. Suppressing crosstalk by encoding random phases

For suppressing the coherence crosstalk, random phases Φn(x,y) are augmented into the target image, i.e, the target image En(x,y) is encoded as En(x,y)exp(iΦn) with -π<Φnπ. According to the derivation in Section 2, the crosstalk term in Eq. (6) becomes

$${F_n}({x^{\prime},y^{\prime}} )= {E_n}({x^{\prime},y^{\prime}} )\textrm{exp} [{i{\Phi _n}({x^{\prime},y^{\prime}} )} ]\otimes \cal {F}\{{\textrm{exp} [{i({{l_n} - {l_m}} )\varphi } ]} \}\otimes Q^{\prime}\left( {\frac{1}{{{f_m} - {f_n}}}} \right)$$

Meanwhile, the reconstructed intensity in Eq. (8) can be converted into

$$\begin{aligned} {I^{rec}} &= {E^{rec}}({x^{\prime},y^{\prime}} ){E^{rec}}{({x^{\prime},y^{\prime}} )^ \ast } = {|{{E_m}({x^{\prime},y^{\prime}} )} |^2} + \sum\limits_{n = 1\atop n \ne m}^N {{{|{{F_n}({x^{\prime},y^{\prime}} )} |}^2}} \\ &+ {E_m}({x^{\prime},y^{\prime}} )\textrm{exp} [{i{\Phi _m}({x^{\prime},y^{\prime}} )} ]\sum\limits_{n = 1\atop n \ne m}^N {{F_n}{{({x^{\prime},y^{\prime}} )}^\ast }} + {E_m}^\ast ({x^{\prime},y^{\prime}} )\textrm{exp} [{ - i{\Phi _m}({x^{\prime},y^{\prime}} )} ]\sum\limits_{n = 1\atop n \ne m}^N {{F_n}({x^{\prime},y^{\prime}} )} \end{aligned}$$

In Eq. (10), the first term is the desired image. The second term is composed of other image channels. Usually, the random phase has no effect on the image intensity, but Q’[1/(fm-fn)] plays an important role. It can disturb the amplitude, resulting in random crosstalk noise in the image [15]. To future explain this, as an example, a checkerboard diagram with random phases is designed, as shown in Fig. 1(a). As the diffraction distance increases, the diffraction pattern will be blurred. In contrast, when a random phase is not applied, the diffraction pattern will remain clear [Fig. 1(a)]. In addition, the last two terms in Eq. (11) have little effects on the image, and they almost vanish due to the orthogonality of random vectors [15].

 figure: Fig. 1.

Fig. 1. Principle of depth multiplexing OAM holography with random phase. (a) The role of random phase; (b) The normalized inner product of two random vectors; (c) The normalized inner product of two complementary chequerboard images as a function of the number of elements.

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Notably, the random phase technique has no significant effect on a single image, and it works well for an image with a large number of pixels. The orthogonality of two random images is affected by the pixel number Num of the images. As an example, the normalized inner product of two complementary chequerboard images is numerically evaluated, as shown in Fig. 1(c). As the pixel number increases, the normalized inner product will decrease gradually according to the central limit theorem, which is approximately 1/sqrt(Num) [Fig. 1(b-c)]. When the number of pixels approaches infinity, the normalized inner product will converge to zero, leading to coherence cancellation between any two reconstructed electric fields. Therefore, the reason for coherence crosstalk suppression can be simply explained as: when the depth image is reconstructed, the total energy of the other layer image channels remains constant, but it will sprinkle dispersedly in the reconstructed image. The coherence crosstalk from other image channels is converted into white noise.

The implementation of the DM-OAMH with random phases is shown in Fig. 2. A target image with random phases is sampled by a discrete array, where the sampling period is determined by the doughnut-shaped intensity distribution [1,2]. Here, the sampling spacing is adopted according to the diameter d of the main ring of the doughnut-shaped spots. Usually, the diameter d and the helical mode index l have a linear relationship, which is approximated as d = ks|l|+d0 µm, with a linear coefficient ks = 20/3 µm and d0 = 20 µm. Notably, the size of the doughnut-shaped feature is affected by the numerical aperture (NA) of the holographic system [6]. Different holographic systems lead to different doughnut-shaped spot sizes and different linear relationships. When an image layer is sampled, an OAM preserving hologram with a discrete spatial-frequency distribution is obtained via the iterative Fourier transform algorithm with about 500 times [16]. A helical phase mode is added to the OAM-preserving hologram to create an OAM-selective hologram. Then a Fresnel zone plate is encoded onto the hologram to obtain an OAM depth selective hologram [Fig. 2(a)]. Finally, the holograms of all the layers are superimposed to obtain a depth multiplexing OAM hologram [Fig. 2(b)].

 figure: Fig. 2.

Fig. 2. The design of a depth multiplexing OAM hologram with random phases. (a) The generation of OAM depth selective hologram. (b) Generation of the OAM depth multiplexing hologram.

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4. Simulation and experimental implementation

As an example, 11 layers of a depth image are designed for numerical validation, as shown in Fig. 3. The target images are all cars [Fig. 3(a)] with 1024×1024 pixels and a pixel size of 8 µm. The sampling constant is 10 pixels and the depth range is 0.2 m. The encoding helical phase indexes are −10, −8, −6, −4, −2, 0, 2, 4, 6, 8, and 10, respectively. The 11 reconstructed layers have deviations of −0.1 m, −0.08 m, −0.06 m, …, 0.08 m, and 0.1 m, respectively from the central one. Comparison of the DM-OAMH is numerically conducted, as shown in Table 1. RMS (Root-Mean-Square), PV (Peak-to-Valley), PSNR (Peak Signal-to-Noise Ratio), and CCOEFF (cross-correlation coefficient) are used to evaluate the reconstruction quality. The RMS is defined as $RMS = \sqrt {\frac{1}{N}\sum\limits_{n = 1}^N {{\textrm{C}_n}^2} }$, where Cn is the n-th component of the background noise in Fig. 3(d-e). CCOEFF is defined as

$$CCOEFF = \displaystyle{{\sum\limits_m {\sum\limits_n {\left( {X_{mn}-\bar{X}} \right)\left( {Y_{mn}-\bar{Y}} \right)} } } \over {\sqrt {\left[ {\sum\limits_m {\sum\limits_n {{\left( {X_{mn}-\bar{X}} \right)}^2} } } \right]\left[ {\sum\limits_m {\sum\limits_n {{\left( {Y_{mn}-\bar{Y}} \right)}^2} } } \right]} }},$$
where, X is the reconstruction image and Y is the origin image, $\bar{X}$ and $\bar{Y}$ are the averages of X and Y, respectively. Xmn represents the value of the element in m rows and n columns of the reconstruction image, and Ymn is the value of the original image. Compared with the case without using random phases, the RMS of the background noise can be reduced by about 2 times and the PV by about 2.3 times. In addition, the PSNR can be improved by about 2.9 dB, and the CCOEFF can improve by about 13.3%, proving the superiority of the proposed method. In contrast, when random phases are not used, the crosstalk shows much greater peak intensity and severe intense oscillations [Fig. 3(e)].

 figure: Fig. 3.

Fig. 3. Comparisons of DM-OAMH with and without random phases. (a) Schematic diagram of the sampled target image. (b) The total crosstalk of 10 background layers with random phases. (c) The total crosstalk of 10 background layers without random phases. (d) A profile in (b). (e) A profile in (c).

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Tables Icon

Table 1. Comparisons of DM-OAMH with and without random phases

Then, an experimental system is built as shown in Fig. 4(a). A He-Ne laser with a wavelength of 632.8 nm is applied as the light source. The laser passes through a polarizer and beam expander and arrives at a spatial light modulator (SLM) Holoeye PLUTO-NIR-011. The SLM has 1080×1920 pixels with a pixel size of 8 µm. Modulated by the SLM and passing through a polarizer, the beam arrives at a CCD with 2048×2048 pixels and a pixel size of 5.5 µm. The polarizer in the experiment can filter out unwanted polarized light except the modulating one.

 figure: Fig. 4.

Fig. 4. Reconstruction result of OAM hologram with 2 layers. (a) Optical setup. (b) Reconstruction results. (b1-b2) Reconstruction result at z=0.200 m and 0.213 m, when decoded by the OAM mode with l=-10. (c1-c2) Reconstruction result at z=0.200 m and 0.213 m, when decoded by the OAM mode with l=10. (d1-d2) Reconstruction result at z=0.200 m and 0.213 m, when simultaneously decoded by the OAM mode with l=10 and OAM mode with l=-10.

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First, a two-layered depth multiplexing OAM hologram is designed, where the target images are a car and a plane, respectively. The pixel number is 1080×1080 and the pixel size of 8 µm. The encoding helical phase modes are l1=−10 and l2 = 10 and the focal lengths of the Fresnel zone plates are f1 = 0.200 m and f2 = 0.213 m, respectively. The sampling constant of the target is adopted as 20 pixels. PSNR =20log(255/RMSE) is selected to measure the reconstructed image. When the OAM mode l1 = 10 is used to decode the hologram, only the car image can be selectively reconstructed at a depth of 0.2 m with PSNR = 24.9 dB and RMSE = 14.5, while the plane cannot be reconstructed at 0.213 m depth [Fig. 4(b1-b2)]. On the contrary, when decoded with the OAM mode l2=−10, only the plane image can be reconstructed at a depth of 0.213 m, [Fig. 4(c1-c2)]. Interestingly, both can be reconstructed when two decoding modes are simultaneously used [Fig. 4(d1-d2)]. Henceforth, the method has a better reconstruction quality. Notably, DM-OAMH provides an option to select a particular image layer by choosing an appropriate decoding pattern, which is almost infeasible in the conventional holography.

Then, 5 images are adopted, where the encoded helical phase indexes are −15, −10, −5, 5, and 10, respectively. The sampling constant is 20 pixels and the depth range is from 0.21 m to 0.28 m. When the depth multiplexing OAM hologram is separately decoded by each OAM mode, 5 number or letter images can be sequentially reconstructed with high quality at different depths, as shown in Fig. 5. It is found the coherence noise is not significant in the reconstructed image and reconstruction image show well quality [Fig. 5(a-b)]. Notably, the resulting image size will gradually increase as the reconstruction length increases. The image size D is determined by the wavelength λ, pixel size of the hologram p, hologram width H, and reconstruction length z, D≈λz/p-H.

 figure: Fig. 5.

Fig. 5. Reconstruction results of OAM holograms with 5 layers. (a) The reconstruction results of 5 image layers “A”, “B”, “C”, “D” and “E”. (b) The reconstruction results of 5 images “1”, “2”, “3”, “4” and “5”.

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5. Summary

In summary, the depth multiplexing OAM holography is proposed based on random phase encoding. The method has three advantages:

  • (1) Depth multiplexing

    This work provides a new multiplexing degree of freedom in depth, which will increase the information capacity greatly.

  • (2) Layer-selective reconstruction

    Multiple images can be reconstructed layer-by-layer or simultaneously, depending on the decoding OAM mode utilized.

  • (3) Coherent noise suppression

    By encoding random phases, the coherence crosstalk can be suppressed due to the orthogonality of random vectors.

As a result, this work can promote the development of OAM holography and may find widespread applications in dynamic OAM holography, optical stage, optical encryption and so on.

Funding

National Natural Science Foundation of China (51875107); Jiangsu Provincial Key Research and Development Program (BE2021035); Shanghai Academy of Spaceflight Technology (2019-086).

Disclosures

The authors declare no conflicts of interest.

Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

References

1. X. Fang, H. Ren, and M. Gu, “Orbital angular momentum holography for high-security encryption,” Nat. Photonics 14(2), 102–108 (2020). [CrossRef]  

2. H. Ren, G. Briere, X. Fang, P. Ni, R. Sawant, S. Héron, S. Chenot, S. Vézian, B. Damilano, V. Brändli, S. A. Maier, and P. Genevet, “Metasurface orbital angular momentum holography,” Nat. Commun. 10(1), 1–8 (2019). [CrossRef]  

3. H. Ren, X. Fang, J. Jang, J. Bürger, J. Rho, and S. A. Maier, “Complex-amplitude metasurface-based orbital angular momentum holography in momentum space,” Nat. Nanotechnol. 15(11), 948–955 (2020). [CrossRef]  

4. H. Zhou, B. Sain, Y. Wang, C. Schlickriede, R. Zhao, X. Zhang, Q. Wei, X. Li, L. Huang, and T. Zentgraf, “Polarization-Encrypted Orbital Angular Momentum Multiplexed Metasurface Holography,” ACS Nano 14(5), 5553–5559 (2020). [CrossRef]  

5. F. Wang, X. Zhang, H. Yuan, R. Xiong, and X. Jiang, “Enhancing the information capacity with modulated orbital angular momentum holography,” IEEE Photonics J. 14(1), 1–5 (2022). [CrossRef]  

6. F. Wang, X. Zhang, R. Xiong, X. Ma, and X. Jiang, “Angular multiplexation of partial helical phase modes in orbital angular momentum holography,” Opt. Express 30(7), 11110–11119 (2022). [CrossRef]  

7. G. Zhu, Z. Bai, J. Chen, C. Huang, L. Wu, C. Fu, and Y. Wang, “Ultra-dense perfect optical orbital angular momentum multiplexed holography,” Opt. Express 29(18), 28452–28460 (2021). [CrossRef]  

8. P. Cheng, S. Huang, and C. Yan, “Ellipticity-encrypted orbital angular momentum multiplexed holography,” J. Opt. Soc. Am. A 38(12), 1875 (2021). [CrossRef]  

9. X. Fang, H. Wang, H. Yang, Z. Ye, Y. Wang, Y. Zhang, X. Hu, S. Zhu, and M. Xiao, “Multichannel nonlinear holography in a two-dimensional nonlinear photonic crystal,” Phys. Rev. A 102(4), 043506 (2020). [CrossRef]  

10. X. Fang, H. Yang, W. Yao, T. Wang, Y. Zhang, M. Gu, and M. Xiao, “High-dimensional orbital angular momentum multiplexing nonlinear holography,” Adv Photonics 3(01), 1–7 (2021). [CrossRef]  

11. H. Zhou, Y. Wang, X. Li, Z. Xu, X. Li, and L. Huang, “A deep learning approach for trustworthy high-fidelity computational holographic orbital angular momentum communication,” Appl. Phys. Lett. 119(4), 044104 (2021). [CrossRef]  

12. H. Zebin, Y. He, P. Wang, W. Xiong, H. Wu, J. Liu, Y. Li, D. Fan, and S. Chen, “Orbital angular momentum deep multiplexing holography via an optical diffractive neural network,” Opt. Express 30(4), 5569–5584 (2022). [CrossRef]  

13. G. Ruffato, R. Rossi, M. Massari, E. Mafakheri, P. Capaldo, and F. Romanato, “Design, fabrication and characterization of Computer Generated Holograms for anti-counterfeiting applications using OAM beams as light decoders,” Sci. Rep. 7(1), 18011 (2017). [CrossRef]  

14. D. G. Voelz and M. C. Roggemann, “Digital simulation of scalar optical diffraction: Revisiting chirp function sampling criteria and consequences,” Appl. Opt. 48(32), 6132–6142 (2009). [CrossRef]  

15. G. Makey, Ö Yavuz, D. K. Kesim, A. Turnalı, P. Elahi, S. Ilday, O. Tokel, and FÖ Ilday, “Breaking crosstalk limits to dynamic holography using orthogonality of high-dimensional random vectors,” Nat. Photonics 13(4), 251–256 (2019). [CrossRef]  

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Data availability

Data underlying the results presented in this paper are not publicly available at this time but may be obtained from the authors upon reasonable request.

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Figures (5)

Fig. 1.
Fig. 1. Principle of depth multiplexing OAM holography with random phase. (a) The role of random phase; (b) The normalized inner product of two random vectors; (c) The normalized inner product of two complementary chequerboard images as a function of the number of elements.
Fig. 2.
Fig. 2. The design of a depth multiplexing OAM hologram with random phases. (a) The generation of OAM depth selective hologram. (b) Generation of the OAM depth multiplexing hologram.
Fig. 3.
Fig. 3. Comparisons of DM-OAMH with and without random phases. (a) Schematic diagram of the sampled target image. (b) The total crosstalk of 10 background layers with random phases. (c) The total crosstalk of 10 background layers without random phases. (d) A profile in (b). (e) A profile in (c).
Fig. 4.
Fig. 4. Reconstruction result of OAM hologram with 2 layers. (a) Optical setup. (b) Reconstruction results. (b1-b2) Reconstruction result at z=0.200 m and 0.213 m, when decoded by the OAM mode with l=-10. (c1-c2) Reconstruction result at z=0.200 m and 0.213 m, when decoded by the OAM mode with l=10. (d1-d2) Reconstruction result at z=0.200 m and 0.213 m, when simultaneously decoded by the OAM mode with l=10 and OAM mode with l=-10.
Fig. 5.
Fig. 5. Reconstruction results of OAM holograms with 5 layers. (a) The reconstruction results of 5 image layers “A”, “B”, “C”, “D” and “E”. (b) The reconstruction results of 5 images “1”, “2”, “3”, “4” and “5”.

Tables (1)

Tables Icon

Table 1. Comparisons of DM-OAMH with and without random phases

Equations (11)

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H ( ξ , η ) = E ( x , y ) exp [ i ( ξ x + η y ) ] d x d y
H m u l ( ξ , η )  =  n = 1 N H n ( ξ , η ) e i l n φ Q ( 1 f n ) ,
H r e c = H m Q ( 1 f m ) + n = 1 n m N H n e i ( l n l m ) φ exp Q ( 1 f n ) ,
E r e c ( x , y ) = exp ( i k f m ) i λ f m H r e c ( ξ , η ) exp ( i k 2 f m [ ( x ξ ) 2 + ( y η ) 2 ] ) d ξ d η ,
E r e c ( x , y ) = exp ( i k f m ) i f m λ exp [ i k 2 f m ( x 2 + y 2 ) ] E m ( x , y ) + n = 1 n m N exp ( i k f n ) i f n λ exp [ i k 2 f n ( x 2 + y 2 ) ] F n ( x , y )
F n ( x , y ) = E n ( x , y ) F { exp [ i ( l n l m ) φ ] } Q ( 1 f m f n ) .
E r e c ( x , y ) E m ( x , y ) + n = 1 n m N F n ( x , y )
I r e c = E r e c ( x , y ) E r e c ( x , y ) = | E m ( x , y ) | 2 + n = 1 n m N | F n ( x , y ) | 2 + E m ( x , y ) n = 1 n m N F n ( x , y ) + E m ( x , y ) n = 1 n m N F n ( x , y )
F n ( x , y ) = E n ( x , y ) exp [ i Φ n ( x , y ) ] F { exp [ i ( l n l m ) φ ] } Q ( 1 f m f n )
I r e c = E r e c ( x , y ) E r e c ( x , y ) = | E m ( x , y ) | 2 + n = 1 n m N | F n ( x , y ) | 2 + E m ( x , y ) exp [ i Φ m ( x , y ) ] n = 1 n m N F n ( x , y ) + E m ( x , y ) exp [ i Φ m ( x , y ) ] n = 1 n m N F n ( x , y )
C C O E F F = m n ( X m n X ¯ ) ( Y m n Y ¯ ) [ m n ( X m n X ¯ ) 2 ] [ m n ( Y m n Y ¯ ) 2 ] ,
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