Study of the agreement between binary neutron star ejecta models derived from numerical relativity simulations
Study of the agreement between binary neutron star ejecta models derived from numerical relativity simulations
Neutron star mergers have recently become a tool to study extreme gravity, nucleosynthesis, and the chemical composition of the Universe. To date, there has been one joint gravitational and electromagnetic observation of a binary neutron star merger, GW170817, as well as a solely gravitational observation, GW190425. In order to accurately …