no code implementations • 17 Feb 2021 • Marek Cieślar, Tomasz Bulik, Małgorzata Curyło, Magdalena Sieniawska, Neha Singh, Michał Bejger
With conservative values for the neutron stars evolution: supernova rate once per 100 years, initial ellipticity $\epsilon_{0}$ = 1e-5 with no decay of the ellipticity $\eta$ = $t_\rm{hub}$ = 1e4 Myr, the expected number of detected neutron stars is below one: 0. 15 (based on a simulation of 10 M stars) for the Advanced LIGO detector.
General Relativity and Quantum Cosmology High Energy Astrophysical Phenomena
