Gravitational-wave astronomy requires population-informed parameter estimation
引力波天文学需要群体信息引导的参数估计
Gravitational-wave events are interpreted in terms of Bayesian posteriors for their source properties inferred under unphysical reference priors. Though these parameter estimates are important intermediate data products for downstream analyses, we demonstrate that they are generically biased and therefore should not be used for astrophysical interpretation directly, as is common. Hierarchical parameter estimation is the solution, as joint analysis of the entire catalog of observations reduces statistical uncertainties and actually informs the correct prior, with population-informed event parameters now appropriate for astrophysical interpretation. As an example, we show how the most extreme measurements from a catalog can be derived and used to identify exceptional events from previous and ongoing observing runs, pointing out they are more informative about the population than any individual event. Using LIGO-Virgo-KAGRA data, we thus demonstrate that population inference is not optional to interpret gravitational-wave observations.
展开 ▾系统性通过P–P图证伪标准单事件PE的覆盖特性;利用顺序统计量定义例外事件并展示群体信息对极端源参数(最大质量、最高自旋)的显著修正;将群体先验应用于新事件GW241011/GW241110,表明非物理先验夸大了极端性。
单事件参数估计在引力波天文学中广泛应用,但已有工作指出其基于非物理先验会引入偏差Vitale+ 2017,并强调了层级群体推断对于识别异常事件的必要性Fishbach+ 2020a。本文系统性地通过P–P图揭示了标准PE的覆盖缺陷,论证了群体信息事件后验的不可或缺性。借助GWTC-4数据的群体再分析,展示了极端源参数的修正Tenorio+ Gerosa 2026,并利用顺序统计量定义了‘例外事件’Essick+ 2022。未来,群体引导的参数估计将在地面Moore+ Gerosa 2021、空间Toubiana+ Gair 2026以及脉冲星计时van Haasteren 2024等观测中成为标准,而非物理先验PE仅应作为中间数据产物。
预印本 2026-04-17 · 刊出 2026-07-16 · 收录 2026-07-27