利用量子扰动理论,神经网络辅助 Metropolis-Hastings 对四维椭圆黑洞解的临界指数进行贝叶斯估计

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Armin Hatefi, Ehsan Hatefi and Roberto J. Lopez-Sastre
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引用次数: 0

摘要

众所周知,临界引力坍缩会产生连续的自相似解,其特征是肖普图克临界指数γ。我们研究了线性扰动方程域中的解,并考虑了数值测量误差。具体地说,我们研究了 SL(2,ℝ) 变换椭圆类的四维爱因斯坦-轴-稀拉顿系统的量子扰动理论。我们在量子扰动理论的基础上开发了一种新的人工神经网络辅助 Metropolis-Hastings 算法,在贝叶斯框架内找到临界指数的分布。与现有方法不同的是,这种新的概率方法可以识别可用的确定性解,并探索由于数值测量误差而可能产生的物理上可区分的临界指数范围。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Neural networks assisted Metropolis-Hastings for Bayesian estimation of critical exponent on elliptic black hole solution in 4D using quantum perturbation theory
It is well-known that the critical gravitational collapse produces continuous self-similar solutions characterized by the Choptuik critical exponent, γ. We examine the solutions in the domains of the linear perturbation equations, considering the numerical measurement errors. Specifically, we study quantum perturbation theory for the four-dimensional Einstein-axion-dilaton system of the elliptic class of SL(2,ℝ) transformations. We develop a novel artificial neural network-assisted Metropolis-Hastings algorithm based on quantum perturbation theory to find the distribution of the critical exponent in a Bayesian framework. Unlike existing methods, this new probabilistic approach identifies the available deterministic solution and explores the range of physically distinguishable critical exponents that may arise due to numerical measurement errors.
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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