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Effects of the microphysical equation of state in the mergers of magnetized neutron stars with neutrino cooling

Effects of the microphysical equation of state in the mergers of magnetized neutron stars with neutrino cooling

We study the merger of binary neutron stars using different realistic, microphysical nuclear equations of state, as well as incorporating magnetic field and neutrino cooling effects. In particular, we concentrate on the influence of the equation of state on the gravitational wave signature and also on its role, in combination …