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arXiv 2510.00533gr-qcastro-ph.IMphysics.comp-phstat.CO
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基于惩罚样条的LISA噪声贝叶斯功率谱密度估计方法

Bayesian power spectral density estimation for LISA noise based on penalized splines with a parametric boost

The University of Auckland(奥克兰大学);Auckland University of Technology(奥克兰理工大学);Université Côte d’Azur, Observatoire de la Côte d’Azur, Artemis, CNRS(蔚蓝海岸大学,蔚蓝海岸天文台,Artemis,法国国家科学研究中心)

Nazeela Aimen, Patricio Maturana-Russel, Avi Vajpeyi, Nelson Christensen, Renate Meyer

AI总结:

本文提出一种贝叶斯方法,利用惩罚样条和参数模型结合,准确估计长时序噪声功率谱密度,适用于LISA数据分析,减少误差并提高精度。

摘要:

灵活且准确的噪声表征对于精确估计引力波参数至关重要。我们介绍了一种贝叶斯方法,用于估计长时平稳时间序列的功率谱密度(PSD),特别针对LISA数据分析。我们的方法将PSD建模为参数和非参数组件的几何平均,结合参数模型的知识与非参数组件的灵活性,以捕捉偏离理论预期的偏差。非参数组件通过惩罚B-样条的混合表达。自适应的数据驱动的knot放置在初始化时进行一次,无需可逆跳跃马尔可夫链蒙特卡洛,而分层粗糙度惩罚先验防止过拟合。在模拟自回归AR(4)数据上的验证显示估计器一致性,并表明与理论匹配的参数组件相比,集成绝对误差更小,且需要更少的样条knots即可达到相当的精度。应用于一年的模拟LISA X通道(单变量)噪声数据,我们的方法实现了相对集成绝对误差为O(10^{-2}),使其适用于迭代分析流水线和多年任务数据集。

英文摘要:

Flexible and accurate noise characterization is crucial for the precise estimation of gravitational-wave parameters. We introduce a Bayesian method for estimating the power spectral density (PSD) of long, stationary time series, explicitly tailored for LISA data analysis. Our approach models the PSD as the geometric mean of a parametric and a nonparametric component, combining the knowledge from parametric models with the flexibility to capture deviations from theoretical expectations. The nonparametric component is expressed by a mixture of penalized B-splines. Adaptive, data-driven knot placement, performed once at initialization, removes the need for reversible-jump Markov chain Monte Carlo, while hierarchical roughness-penalty priors prevent overfitting. Validation on simulated autoregressive AR(4) data demonstrates estimator consistency and shows that well-matched parametric components reduce the integrated absolute error compared to an uninformative baseline, requiring fewer spline knots to achieve comparable accuracy. Applied to one year of simulated LISA X-channel (univariate) noise, our method achieves relative integrated absolute errors of $\mathcal{O}(10^{-2})$, making it suitable for iterative analysis pipelines and multi-year mission data sets.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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