A morphology-independent search for gravitational wave echoes in data from the first and second observing runs of Advanced LIGO and Advanced Virgo

• DOI: 10.1103/physrevd.101.064012
• Publication Date: 2020-03-09T13:57:28Z
• Authors: Ka Wa Tsang; Archisman Ghosh; Anuradha Samajdar; Katerina Chatziio...; Simone Mastrogiov...; Michalis Agathos; Chris Van Den Broeck
• Keywords: data analysis method; noise; neutron star: binary; alternative theories of gravity; FOS: Physical sciences; General Relativity and Quantum Cosmology (gr-qc); gravitational radiation: direct detection; 530; 01 natural sciences; General Relativity and Quantum Cosmology; 0103 physical sciences; LIGO; numerical calculations; gravitational radiation; statistical analysis: Bayesian; gravitational radiation detector; VIRGO; black hole: binary; General relativity; gravitational radiation: emission; neutron star: binary: coalescence; [PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]

Gravitational wave echoes have been proposed as a smoking-gun signature of exotic compact objects with near-horizon structure. Recently there have been observational claims that echoes are indeed present in stretches of data from Advanced LIGO and Advanced Virgo immediately following gravitational wave signals from presumed binary black hole mergers, as well as a binary neutron star merger. In this paper we deploy a morphology-independent search algorithm for echoes introduced in Tsang et al., Phys. Rev. D 98, 024023 (2018), which (a) is able to accurately reconstruct a possible echoes signal with minimal assumptions about their morphology, and (b) computes Bayesian evidences for the hypotheses that the data contain a signal, an instrumental glitch, or just stationary, Gaussian noise. Here we apply this analysis method to all the significant events in the first Gravitational Wave Transient Catalog (GWTC-1), which comprises the signals from binary black hole and binary neutron star coalescences found during the first and second observing runs of Advanced LIGO and Advanced Virgo. In all cases, the ratios of evidences for signal versus noise and signal versus glitch do not rise above their respective "background distributions" obtained from detector noise, the smallest $p$-value being 3% (for event GW170823). Hence we find no statistically significant evidence for echoes in GWTC-1.<br/>6 pages, 5 figures, 2 tables<br/>