A fast inversion method of parameters for contact binaries based on differential evolution

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Astronomy and Computing Pub Date : 2024-02-07 DOI:10.1016/j.ascom.2024.100799
X. Zeng , J. Song , S. Zheng , G. Xu , S. Zeng , Y. Wang , A. Esamdin , Y. Huang , S. Xia , J. Huang
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Abstract

With the development of modern astronomical observation techniques and contact binary research, a large number of light curves of contact binaries have been published, and it has become a challenge to quickly derive the basic physical parameters of contact binaries from their light curves. This article presents a neural network (NN) based on the differential evolution intelligent optimization algorithm to infer the fundamental physical parameters of contact binaries from their light curve. Based on a large dataset of light curves and parameter data generated by Phoebe, a NN mapping model is established, while Differential Evolution (DE) and Markov Chain Monte Carlo (MCMC) algorithms are used to find reasonable parameter combinations, respectively. The experiments show that the parameter inversion speed of the DE algorithm is approximately 50% faster than that of the MCMC algorithm, while guaranteeing a parameter accuracy at least consistent with the those of MCMC algorithm.

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基于微分演化的接触双星参数快速反演法
随着现代天文观测技术和接触双星研究的发展,大量接触双星的光变曲线被发表出来,如何从它们的光变曲线中快速推导出接触双星的基本物理参数成为一个难题。本文提出了一种基于微分进化智能优化算法的神经网络(NN),从接触双星的光曲线推导出接触双星的基本物理参数。基于Phoebe产生的大量光曲线和参数数据集,建立了一个NN映射模型,并分别采用差分进化(DE)和马尔可夫链蒙特卡洛(MCMC)算法来寻找合理的参数组合。实验表明,DE 算法的参数反演速度比 MCMC 算法快约 50%,同时保证了参数精度至少与 MCMC 算法一致。
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来源期刊
Astronomy and Computing
Astronomy and Computing ASTRONOMY & ASTROPHYSICSCOMPUTER SCIENCE,-COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS
CiteScore
4.10
自引率
8.00%
发文量
67
期刊介绍: Astronomy and Computing is a peer-reviewed journal that focuses on the broad area between astronomy, computer science and information technology. The journal aims to publish the work of scientists and (software) engineers in all aspects of astronomical computing, including the collection, analysis, reduction, visualisation, preservation and dissemination of data, and the development of astronomical software and simulations. The journal covers applications for academic computer science techniques to astronomy, as well as novel applications of information technologies within astronomy.
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