Modeling the gravitational wave signature of neutron star black hole coalescences: PhenomNSBH

26 Jun 2020 Thompson Jonathan E. Fauchon-Jones Edward Khan Sebastian Nitoglia Elisa Pannarale Francesco Dietrich Tim Hannam Mark

Accurate gravitational-wave (GW) signal models exist for black hole binary (BBH) and neutron-star binary (BNS) systems, which are consistent with all of the published GW observations to date. Detections of a third class of compact-binary systems, neutron-star black hole (NSBH) binaries, have not yet been confirmed, but are eagerly awaited in the near future... (read more)

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  • GENERAL RELATIVITY AND QUANTUM COSMOLOGY
  • HIGH ENERGY ASTROPHYSICAL PHENOMENA
  • SOLAR AND STELLAR ASTROPHYSICS