Preprint
Oct 2026
Numerical simulations of low-mass black hole-neutron star mergers with moderate eccentricities
A confident detection of orbital eccentricity in gravitational-wave signals from black hole-neutron star systems would be a strong indicator of their dynamical formation origin. While eccentric waveform models have recently been developed, their validity for analyzing black hole--neutron star signals has yet to be test...
Ivan Markin, G. Morr'as, Tim Dietrich
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