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2020

Parameter estimation of stellar-mass black hole binaries with LISA

Toubiana, Alexandre, Marsat, Sylvain, Babak, Stanislav et al.

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Stellar-mass black hole binaries (SBHBs), like those currently being detected with the ground-based gravitational-wave (GW) observatories LIGO and Virgo, are also an anticipated GW source for LISA.

LISA will observe them during the early inspiral stage of evolution; some of them will chirp through the LISA band and reappear some time later in the band of $3^{rd}$ generation ground-based detectors.
SBHBs could serve as laboratories for testing the theory of General Relativity and inferring the astrophysical properties of the underlying population.
In this study, we assess LISA's ability to infer the parameters of those systems, a crucial first step in understanding and interpreting the observation of those binaries and their use in fundamental physics and astrophysics.

Parameter estimation of stellar-mass black hole binaries with LISA · Around

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