no code implementations • 7 Dec 2020 • Elias R. Most, L. Jens Papenfort, Samuel Tootle, Luciano Rezzolla
By simulating the merger of black hole--neutron star systems of exactly the same masses and spins, we show that these fast ejecta are entirely absent, if the primary is instead a black hole.
High Energy Astrophysical Phenomena General Relativity and Quantum Cosmology
