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The final phase of inspiral of neutron stars: realistic equations of state
Dorota Gondek-Rosinska, Michal Bejger, Tomek Bulik +5
Coalescing compact star binaries are expected to be among the strongest sources of gravitational radiation to be seen by laser interferometers. We present calculations of the final…
Impact of the nuclear equation of state on the last orbits of binary neutron stars
M. Bejger, D. Gondek-Rosinska, E. Gourgoulhon +3
We present calculations of quasiequilibrium sequences of irrotational binary neutron stars based on realistic equations of state (EOS) for the whole neutron star interior. Three re…
Surface gravity of neutron stars and strange stars
M. Bejger, P. Haensel
The upper bound on the value of the surface gravity, g_s, for neutron stars with equations of state respecting v_sound <= c, is derived. This bound is inversely proportional to the…