3 code implementations • 16 May 2018 • Daniel Wysocki, Jacob Lange, Richard O'Shaughnessy
Using concrete synthetic data based on projections for LIGO and Virgo's O3 run, we discuss how well GW measurements could constrain the mass and spin distribution of coalescing neutron stars and black holes in the near future, within the context of several phenomenological models described in this work.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena Solar and Stellar Astrophysics
