Multi-Segment Consistency Tests of General Relativity

TL;DR

This paper introduces a multi-parameter Multi-Segment Consistency Test (MSCT) for gravitational-wave signals, enhancing the precision of tests of general relativity and black hole area laws by ensuring signal segment consistency and capturing parameter covariances.

Contribution

It presents a generalized MSCT that improves upon existing tests by incorporating extrinsic property consistency and an accelerated time-domain approach, leading to more stringent constraints on area increase.

Findings

Achieved a 4.61 sigma significance in area increase test for GW250114.

Captured covariances among parameters, improving test accuracy.

Provided the most precise test of the black hole area law to date.

Abstract

As the LIGO-VIRGO-KAGRA Network of gravitational-wave detectors improves in sensitivity, accumulating hundreds of gravitational-wave detections per year, it becomes imperative to improve tests of general relativity in concert. The test of Hawking's law of area increase has gained prominence since GW250114, where black holes in General Relativity were tested with unprecedented precision, using the linear ringdown and pre-merger portions of the signal. A closely related test is the Inspiral-Merger-Ringdown Consistency Test, which assesses the consistency of the high- and low-frequency parts of the signals. In this letter, I present a multi-parameter Multi-Segment Consistency Test (MSCT) that generalizes and improves upon existing tests by ensuring that the extrinsic properties of the signal are consistent across its independent segments and by adopting an accelerated time-domain approach. The improved area law test is then presented as a projection of this MSCT test. These crucial improvements, which bring physical consistency to the area law test, lead to more stringent constraints on the increase in estimated area from observed binary black hole mergers, while also capturing covariances among the parameters. Applying the two-segment version of this test to the inspiral and ringdown parts of GW250114, and keeping some of the extrinsic parameters common between the segments, I test the signal to unprecedented accuracy, obtaining $4.61 ^{+0.24} _{-0.11}\sigma$ significant result for the area increase, even as more than 4 pre-merger cycles of the signal are excluded from the analysis. Also, I infer that the final state lies within the 15\% highest posterior density confidence interval.