📝 SummarXiv

Abstract

GW230814 was detected by the LIGO Livingston observatory with a signal-to-noise ratio of 42.4 making it the loudest gravitational-wave signal in the GWTC-4.0 catalog. The source is consistent with a binary black hole coalescence similar to those in the previously observed population, with component masses $m_1 = 33.7^{+2.9}_{-2.2}$ $\mathrm{M}_\odot$, $m_2 = 28.2^{+2.2}_{-3.1} M_\odot$, and small effective inspiral spin $\chi_{\mathrm{eff}}= -0.01^{+0.06}_{-0.07}$. The high signal-to-noise ratio enabled us to confidently detect an $\ell = |m| = 4$ mode in the inspiral signal for the first time, and enables a range of tests of consistency between theoretical predictions and the observed waveform. Most of these tests show good agreement with expectations from general relativity. However, a few indicate deviations, particularly in the ringdown part of the signal. We find that deviations comparable to those observed can be obtained from similar simulated signals based on general relativity and detector noise effects. Therefore, the apparent deviations do not provide evidence for a violation of general relativity. The observation of GW230814 demonstrates that while the unprecedented sensitivity of the detectors enable highly significant detections with a single observatory, drawing robust inferences about fundamental physics remains limited without data from a multiple observatory network.