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• W3160695107 abstract "Abstract In 2017 August, the first detection of a binary neutron star merger, GW170817, made it possible to study neutron stars in compact binary systems using gravitational waves. Despite being the loudest gravitational-wave event detected to date (in terms of signal-to-noise ratio), it was not possible to unequivocally determine that GW170817 was caused by the merger of two neutron stars instead of two black holes from the gravitational-wave data alone. That distinction was primarily due to the accompanying electromagnetic counterpart. This raises the question: under what circumstances can gravitational-wave data alone, in the absence of an electromagnetic signal, be used to distinguish between different types of mergers? Here, we study whether a neutron star–black hole binary merger can be distinguished from a binary black hole merger using gravitational-wave data alone. We build on earlier results using chiral effective field theory to explore whether the data from LIGO and Virgo, LIGO A+, LIGO Voyager, the Einstein Telescope, or Cosmic Explorer could lead to such a distinction. The results suggest that the present LIGO–Virgo detector network will most likely be unable to distinguish between these systems even with the planned near-term upgrades. However, given an event with favorable parameters, third-generation instruments such as Cosmic Explorer will be capable of making this distinction. This result further strengthens the science case for third-generation detectors." @default.
• W3160695107 created "2021-05-24" @default.
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• W3160695107 date "2022-12-01" @default.
• W3160695107 modified "2023-09-24" @default.
• W3160695107 title "Using Gravitational Waves to Distinguish between Neutron Stars and Black Holes in Compact Binary Mergers" @default.
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• W3160695107 doi "https://doi.org/10.3847/1538-4357/ac98fe" @default.
• W3160695107 hasPublicationYear "2022" @default.
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