对于脉冲星定时阵列数据集的快速参数估计,使用变量推理和规范化流量
Michele Vallisneri1,2,3, Marco Crisostomi3,4, Aaron D Johnson3
1ETH Zurich, Institute for Particle Physics and Astrophysics, Wolfgang-Paul-Strasse 27, 8093 Zurich, Switzerland.
Physical review letters
|September 10, 2025
概括
我们介绍了一种新的,更快的方法来分析脉冲星定时阵列的引力波数据. 该技术使用贝叶斯变量推理和神经网络,与传统的马尔科夫链蒙特卡洛方法相比,显著加快参数估计.
科学领域:
- 天体物理学 天体物理学
- 宇宙学的宇宙学是什么?
- 数据分析 数据分析
背景情况:
- 脉冲星定时阵列 (PTA) 数据集引力波分析中的参数估计通常使用马尔科夫链蒙特卡洛 (MCMC) 方法.
- MCMC 方法探索后置概率密度,但可能是计算密集且耗时的.
研究的目的:
- 在PTA数据分析中引入一种新的,计算效率高的MCMC替代方案,用于参数估计.
- 利用神经网络和贝叶斯变量推理来实现更快,更可扩展的数据分析.
主要方法:
- 开发了一种随机梯度下降贝叶斯变量推理程序.
- 使用神经网络来近似后面的概率密度.
- 将近似和确切的后部之间的Kullback-Leibler分歧最小化.
- 在单个数据集上训练网络,不同于基于模拟的推断.
主要成果:
- 新技术显著加速了PTA数据集的分析,特别是在GPU等并行计算平台上.
- 对NANOGrav 15年数据集的分析在几十分钟内完成,这与MCMC相比是几个小时或几天的实质性改进.
- 该方法需要计算数据概率及其梯度.
结论:
- 这种快速变异推断技术为引力波数据分析提供了可行的替代方案.
- 加速使新的天体物理和宇宙学探索能够使用计算上昂贵的统计模型.
- 该方法适用于其他引力波数据分析环境,具有可差分和可并行概率.
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