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arXiv 2304.04767astro-ph.IMastro-ph.COgr-qc
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国际脉冲星计时阵列探测纳赫兹引力波的检查清单

The International Pulsar Timing Array checklist for the detection of nanohertz gravitational waves

Bruce Allen, Sanjeev Dhurandhar, Yashwant Gupta, Maura McLaughlin, Priyamvada Natarajan, Ryan M. Shannon, Eric Thrane, Alberto Vecchio

AI总结:

本文提出国际脉冲星计时阵列(IPTA)用于验证纳赫兹引力波探测声明的正式检查清单,涵盖赫林斯-唐斯曲线验证、跨PTA数据交叉检验及探测委员会审查流程,为未来可信探测提供路线图。

摘要:

脉冲星计时阵列(PTAs)提供了一种在纳赫兹频段探测引力波的方法。在这一频段中,最可能的信号是随机的,其功率谱在较低频率处急剧上升。事实上,在脉冲星计时数据中观测到的共同红噪声过程表明,纳赫兹频率引力波的首次可信探测可能在未来几年内实现。探测过程因信号和噪声的性质而变得复杂:最初的观测声明将是在可探测性阈值处得出的统计推断。为了证明引力波正在脉冲星计时数据集中产生部分噪声,观测必须展示出赫林斯-唐斯曲线——即与引力波相关的角相关函数——同时还要证明不存在其他合理的解释。为了确保探测声明可信,国际脉冲星计时阵列(IPTA)设有正式流程,在结果发表前进行审查。这包括在不同PTA之间内部共享数据和数据处理流水线,从而能够进行独立的交叉检验和结果验证。为了监督和验证任何探测声明,IPTA还成立了一个由八名成员组成的探测委员会(DC),其中包括四名独立的外部成员。IPTA成员只有在正式审查流程结束后才会发表其结果。本文档是探测委员会的初步检查清单,描述了一个可信探测应当满足的一些条件。目前,没有任何PTA提出探测声明;因此,本文档可作为未来的路线图。

英文摘要:

Pulsar timing arrays (PTAs) provide a way to detect gravitational waves at nanohertz frequencies. In this band, the most likely signals are stochastic, with a power spectrum that rises steeply at lower frequencies. Indeed, the observation of a common red noise process in pulsar-timing data suggests that the first credible detection of nanohertz-frequency gravitational waves could take place within the next few years. The detection process is complicated by the nature of the signals and the noise: the first observational claims will be statistical inferences drawn at the threshold of detectability. To demonstrate that gravitational waves are creating some of the noise in the pulsar-timing data sets, observations must exhibit the Hellings and Downs curve -- the angular correlation function associated with gravitational waves -- as well as demonstrating that there are no other reasonable explanations. To ensure that detection claims are credible, the International Pulsar Timing Array (IPTA) has a formal process to vet results prior to publication. This includes internal sharing of data and processing pipelines between different PTAs, enabling independent cross-checks and validation of results. To oversee and validate any detection claim, the IPTA has also created an eight-member Detection Committee (DC) which includes four independent external members. IPTA members will only publish their results after a formal review process has concluded. This document is the initial DC checklist, describing some of the conditions that should be fulfilled by a credible detection. At the present time none of the PTAs have a detection claim; therefore this document serves as a road map for the future.

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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