Abstract
We introduce a novel, to the best of our knowledge, method to increase the bandwidth in holographic displays. Here, multi-angle illumination using multiple laser diodes (LDs) is adopted to expand the limited diffraction angle of the spatial light modulator (SLM). To solve the problem of signal repetitions caused by sharing the same SLM pattern, we use a random binary mask (BM). We demonstrate via simulations and experiments that our method effectively increases the bandwidth with sufficient image quality. Furthermore, the speckle noise, a critical issue of the holographic display that decreases the contrast and is potentially harmful to eyes, is reduced by the advantage of incoherent summation in the reconstruction plane. We believe that this method is a practical approach that can expand the bandwidth of the holographic display by alleviating the bottleneck of hardware limitations.
© 2022 Optica Publishing Group under the terms of the Optica Open Access Publishing Agreement
Holographic display is considered as the ultimate display as it can express a three-dimensional (3D) object by reproducing the wavefront of light. Since the advent of the hologram, efforts have been steadily made to replace the existing flat panel display [1–11]. However, the holographic displays have an inherent trade-off relationship between the viewing angle and the display size. Unlike the flat panel display using an incoherent light source, a hologram is generally reproduced by a coherent beam and a spatial light modulator (SLM) with pixelated structure. Here, the product of the diffraction angle and the area of the SLM is defined as the space-bandwidth product (SBP) that determines the overall performance of the holographic display system.
Typically, the SBP is equal to the number of pixels of the SLM. However, even with the 4K–8K resolution of the most advanced SLMs, there is a fundamental limitation of having a much smaller viewing angle and size than flat panel displays. Accordingly, with the innovation in the manufacturing industry to increase the number of SLM pixels, a lot of research has been actively done to overcome the bandwidth limitations of the holographic display.
The multiplexing technique in time or space can effectively extend the limited bandwidth of the SLM, so it has been widely used in holographic displays. However, the spatial multiplexing method using multiple SLMs is bulky and expensive [1]. In addition, for the case of the temporal multiplexing method, it requires relatively complex optics and consumes the system’s frame rate as the number of multiplexing [2,3]. Recently, several studies have shown that a scattering medium can be used to expand the viewing angle of the holographic display [4,5]. However, they require highly precise alignment between the scattering medium and the SLM.
In this Letter, we propose a novel method to increase the bandwidth of the holographic display using a multi-illumination strategy without temporal multiplexing. Typically, the effective range of the bandwidth is confined within the Nyquist frequency so as not to violate the sampling theorem. By illuminating multiple laser diodes (LDs) from different angles, the spatial frequency range of the hologram becomes wider with the extended energy distribution. However, the wavefront from each LD transfers identical information of the SLM that differs only in the carrier frequency, resulting in indistinguishable cross talk between the signals. Here, the main idea is to optically break the equivalence of the information by using a random binary mask (BM) at the frequency domain.
Figure 1 shows a schematic diagram of the proposed holographic display. It is based on a conventional holographic display with filtering optics. A multi-illumination is realized by adopting the LD array. Then, the BM in the spatial frequency domain acts as the filter and gives the degrees of freedom to modify the information from each of the LDs individually.
A BM of arbitrary shape is considered in generating the computer graphic hologram (CGH). In this Letter, each direction (${i}, {j}$) of illumination is set to match with that of high diffraction orders as below:
where $\lambda$ is the wavelength, $d$ is the pixel pitch of the SLM, $m_{ij}$ denotes the ${(i, j)}\text {th}$ diffraction order, and $i$, $j$ take positive and negative values $(\ldots,-2, -1, 0, 1, 2,\ldots )$.The periodic pattern of the SLM generates high-order diffraction, which is the repeated pattern of the zero-order signal. Those repetition signals cause spatial aliasing artifacts that are considered noise and removed by filtering. However, in the proposed method, the intensity of the high diffraction order is further strengthened by the multi-illumination strategy to expand the bandwidth. In addition, each signal is filtered by the BM at different positions, which breaks the correlation of the signal. Finally, by making the duplicated information meaningful with the BM, it is possible to seamlessly extend the entire bandwidth of the holographic display over the number of illuminations.
Figure 2(a) illustrates our algorithm to synthesize the CGH. We optimize the phase of the SLM by using the stochastic gradient descent (SGD) approach. First, we consider the high-order diffraction [9], described as follows:
where $U$ is the tiled spectrum, $\operatorname {comb}[\cdot,\cdot ]$ denotes the Dirac comb function, the symbol $\otimes$ is the convolution operator, $\operatorname {FT}[\cdot ]$ denotes a 2D Fourier transform operator, $e^{i\phi }$ is the modulated wavefront at the SLM, and $f_x$, $f_y$ are the spatial frequencies.The tiled spectrum $U$ is then multiplied by the binary mask $M\in \{ 1,0\}^{N_x \times N_y}$ and transfer function $H$ of the angular spectrum method after padding in the frequency domain [12]. With the propagation distance $z$, $H$ is defined as
We account for the carrier frequencies of the LDs and the fill factor of the SLM in the frequency domain by multiplying the sinc amplitude. When the SLM is illuminated by the $(i, j)\text {th}$ LD, the 2D sinc amplitude $T_{ij}$ is given by
where $a$ is the width of the active area of the pixel. Note that each carrier frequency is set to be matched with high-order direction, as shown in Fig. 2(b), but not mandatory if taken into account in the optimization. The hologram can be optimized even if the carrier frequency and wavelength are set differently. Thus, a full-color image could be produced using a time-sequential operation without any hardware change.From Eqs. (2)–(4), the complex amplitude $u_{ij}$ for the $(i, j)\text {th}$ LD at the distance $z$ is represented as
where $\operatorname {iFT}[\cdot ]$ denotes an inverse 2D Fourier transform operator and $\circ$ is elemental-wise multiplication. Finally, we find an optimal phase pattern based on the SGD approach by solving the following problem:We verify the feasibility of the proposed method by measuring the reconstructed image quality using the peak signal-to-noise ratio (PSNR) and structural similarity (SSIM) index. To confirm the essential characteristic of the BM, we compare the proposed method against the single LD and multiple LDs cases without the mask. For the simulation, $3\times 3$ LDs with a wavelength of 635 nm and virtual SLM of $1000\times 1000$ resolution with 8 $\mu$m pixel pitch are used. The SLM fill factor $(a^2/d^2)$ is set to 0.92.
First, we investigated the properties of the BM pattern. For the simulation, the learning rate is set to 1.00, and the number of iterations is 1000. The phase value $\phi$ is initialized randomly in the range of $[-\pi,\pi )$ for optimization. Figure 3(a) shows that the image quality of the system is not significantly affected by the resolution of the BM. Here, very low-resolution BM may cause a noticeable discontinuity in the viewing angle. However, high-resolution BM requires precise alignment and decreases the optimization performance with a sparse spectrum. In addition, the BM with a lower density shows higher PSNR values as it increases the capacity to modify the information of each source; however, it penalizes the energy efficiency. Therefore, concerning the practical aspects, we chose the BM with $50\%$ density and $45 \times 45$ resolution, as marked with a red arrow.
Then, we investigated the reliability using 50 images in the DIV2K test dataset [13]. As shown in Fig. 3(b), our method achieves higher image quality than the cases where the BM is not applied. Even in the case without downsampling, it gives better performance. Although the performance can vary depending on the image used, our method not only yields a PSNR improvement but also is more robust near the SLM, where the information overlap is aggravated. Our approach can cover the wide depth range as the noise from the duplicated information is highly mitigated compared with the case without the BM. The simulation results verify that the proposed method could support high image quality with the multi-illumination strategy.
Figure 3(c) directly shows the validity of the random BM. In the case of not applying the BM, the duplicated images of the zero-order signal are placed in the shifted location according to each carrier frequency of LDs. In contrast, the proposed method effectively suppresses the noise originating from duplicated information. After each wavefront of the LD is blocked differently in the BM, the correlation sharing the single SLM is broken. As a result, the target image can be reproduced individually from the multiple illuminations. In Fig. 3(d), each ${(i, j)}\text {th}$ image represents the reconstructed result at the distance of 50 mm when the LDs are turned on one by one for the same phase pattern. The proposed method simultaneously reconstructs the image with multiple carrier frequencies, which in turn results in a wider viewing angle of the hologram with extended bandwidth.
Figure 4(a) shows the experiment setup. We used Thorlabs Exulus HD2 for the SLM and the CPS635F laser module with a wavelength of 635 nm. The $3\times 3$ LD array was assembled with a plastic housing made with a 3D printer. The BM was fabricated on glass (50 mm $\times$ 50 mm square, 2.3 mm thick) coated with patterned chromium. Three Nikon 105 mm camera lenses were used for the collimation and 4$f$ relay optics in the experiment. The results were captured using a CCD camera without lenses mounted on.
As provided in Fig. 4(b), the captured results show the novel feature of decreasing unwanted speckle noise with extended bandwidth. Overall, our method produces a face more smoothly compared with the standard case using a single LD source without the mask. Figure 4(c) presents the enlarged image cropped from the result. The speckle reduction effect is proportional to the overlap ratio of the regions illuminated by the LDs in the reconstruction plane. Since each central point of the high diffraction orders is placed at the edge of the image for a propagation distance of 50 mm, the speckle contrast reduces to approximately half without sacrificing the frame rate of the system as four independent speckle patterns are superimposed [2,3].
Furthermore, Fig. 5 demonstrates that the proposed method can expand the viewing angle and express 3D holograms. As shown in Fig. 5(a), the aliasing artifacts are effectively alleviated, and the viewing angle exceeds that of the single LD case, $\pm {2.3}^{\circ }$. We optimize the phase pattern with an amplitude loss function for two target planes to obtain the results of Fig. 5(b). The images are well reproduced experimentally at each depth.
In summary, we propose a novel method to solve the limited bandwidth which has been a hurdle to the practical use of the holographic display. In this Letter, we introduce a new optical configuration using multi-illumination and a BM to enlarge the bandwidth of the holographic display. This approach effectively circumvents the trade-off between viewing angle and display size. Our experimental results demonstrate that the multi-illumination strategy achieved sufficient image quality with the extended bandwidth and effectively reduces the speckle noise. The maximum SBP of the method can be limited by the change in the characteristics of the SLM as the incident angle increases [14]. However, it was not a major concern in our experimental system, and more detailed analysis will be done in the future. The proposed method has practical significance as it is less sensitive to errors than the methods using a scattering device which requires a high-precision component and micro-scale alignment optics to improve the bandwidth. Even though it takes more time to synthesize the hologram with the expanded bandwidth, previous work has shown that training propagation models make real-time hologram synthesis possible [7]. Furthermore, our method can be integrated with previous works optimizing light sources to further reduce the speckle noise [8], and replace the random BM with a gray-scale mask to improve light throughput and image quality for future work [5].
We believe our concept of multi-illumination with the mask would be generally applicable to other systems such as near-eye or table-top holographic displays. We hope that our approach can contribute to the further development and realization of practical holographic displays.
Funding
Institute of Information and Communications Technology Planning and Evaluation (IITP) Grant funded by the Korea Government (MSIT) (2017-0-00787).
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.
Supplemental document
See Supplement 1 for supporting content.
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