2023
DOI: 10.48550/arxiv.2303.10847
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The effect of noise artefacts on gravitational-wave searches for neutron star post-merger remnants

Abstract: Gravitational waves from binary neutron star post-merger remnants have the potential to uncover the physics of the hot nuclear equation of state. These gravitational-wave signals are high frequency (∼ kHz) and short lived (O (10 ms)), which introduces potential problems for data-analysis algorithms due to the presence of non-stationary and non-Gaussian noise artefacts in gravitational-wave observatories. We quantify the degree to which these noise features in LIGO data may affect our confidence in identifying … Show more

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