出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The signal of neutron star (NS) mergers has the imprint of the EOS of dense nuclear matter,
which is still not well known. A set of gravitational waves (GW) signals have been calculated
from 3D hydrodynamical simulations of NS-NS mergers using the Smoothed Particle
Hydrodynamics technique (SPH) with different EOS. By analyzing the morphology and time
evolution of the signal we want to be able to discriminate among the variety of proposed EOS
after a successful GW detection has been done.
