Zhang Z Y, Chang J, Huang Y F, et al. Reinforcement learning-based stray light suppression study for space-based gravitational wave detection telescope system[J]. Opto-Electron Eng, 2024, 51(2): 230210. doi: 10.12086/oee.2024.230210
Citation: Zhang Z Y, Chang J, Huang Y F, et al. Reinforcement learning-based stray light suppression study for space-based gravitational wave detection telescope system[J]. Opto-Electron Eng, 2024, 51(2): 230210. doi: 10.12086/oee.2024.230210

Reinforcement learning-based stray light suppression study for space-based gravitational wave detection telescope system

    Fund Project: Project supported by National Key R&D Program of China (2021YFC2202100)
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  • In gravitational wave telescopes, the energy of the collected space target light signals is dwarfed by the energy of stray light, necessitating robust stray light suppression for reliable telescope operation. Due to the inherent unpredictability of scattered light and the intricate nature of opto-mechanical systems, the formulation of stray light suppression strategies often involves complex mathematical modeling, substantial expertise, and iterative simulations. This paper introduces a Reinforcement Learning-based approach to devise the stray light suppression scheme within a Monte Carlo ray tracing environment, specifically for space gravitational wave telescope systems. Our empirical findings confirm the efficacy of this methodology in generating effective stray light suppression strategies, yielding favorable suppression performance. This study contributes a novel, efficient, and adaptable solution to the stray light challenges faced in space gravitational wave detection as well as other high-precision optical systems, thereby holding extensive applicative promise.
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  • In the field of space gravitational wave detection, the functionality of telescopes is critically hampered by the presence of stray light. This stray light, significantly overpowering the energy of collected space-target optical signals, poses a substantial challenge, necessitating robust stray light suppression for the telescope's reliable operation. Traditionally, this suppression has been achieved through complex mathematical modeling, extensive expertise, and iterative simulations, given the inherent unpredictability of scattered light and the intricate nature of optical-mechanical systems.

    This study introduces a novel approach to stray light suppression by integrating reinforcement learning, a key area in machine learning. Reinforcement learning optimizes problem-solving strategies through an intelligent agent that learns to maximize cumulative rewards from its environment to achieve specific objectives. By applying this methodology, we address the limitations of traditional stray light suppression scheme formulation.

    Our approach employs reinforcement learning to develop a strategy for stray light suppression within a Monte Carlo ray tracing-based environment, tailored for Space Gravitational Wave Detection Telescope systems. This method is particularly adept at identifying and mitigating stray light paths caused by surface scattering, a prevalent issue in optical systems.

    A comparative analysis was conducted using the specialized stray light analysis software to evaluate the effectiveness of traditional methods against those developed through reinforcement learning. The results reveal that reinforcement learning-based schemes surpass traditional methods in identifying and mitigating stray light paths, especially those caused by surface scattering. Compared with the traditional stray light analysis and suppression, it reduces the designer's manual iteration process based on experience and ray tracing results due to the high standard of stray light suppression brought by the space gravitational wave detection telescope system. The scattering caused by surface properties is considered, and the stray light suppression effect is improved.

    The empirical findings from this study confirm the superiority of reinforcement learning in formulating effective stray light suppression measures for space gravitational wave detection telescope systems. The approach not only achieves superior suppression outcomes but also introduces an efficient, flexible, and innovative solution to the challenges of stray light in space gravitational wave detection and other high-precision optical systems.

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