Statistic threshold of distinguishing the environmental effects and modified theory of gravity with multiple massive black-hole binaries
Xulong Yuan

TL;DR
This paper develops a statistical method to distinguish environmental effects from modified gravity theories in gravitational wave signals from black-hole binaries, improving threshold determination for better effect discrimination.
Contribution
It introduces a refined approach to set thresholds for the statistic distinguishing multiple effects, considering overlaps and different astronomical models, enhancing effect identification accuracy.
Findings
Successfully determined thresholds to distinguish three effects at -4 PN order.
The method remains effective despite overlaps in effect distributions.
Threshold selection is crucial for accurate effect discrimination.
Abstract
In future space-borne \ac{GW} observations, matter arround the sources might influence the evolution and \ac{GW} signals from \ac{BBH} inspirals, which can be mistaken as deviations from \ac{GR}. Former research \cite{yuan2024} proposed a statistic that characterizes the dispersion of measured parameters to distinguish environmental effect(\ac{DF} from \ac{DM} spike) and theory of modified gravity effect(varying ). In this work we use the statistic to distinguish other couples of effects with \ac{GW} corrections at PN order: \ac{DF} from \ac{DM} spike and the extra dimension theory, additionally try to determine the distinguishing threshold in more reasonable way to avoid arbitrariness, especially when the two effects to compare have more overlap in the distribution. Sources of different astronomical models are also considered, and two effects are still distinguishable…
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