Constraints on Microscopic and Phenomenological Equations of State of Dense Matter from GW170817

We discuss the constraints on the equation of state (EOS) of neutron star matter obtained by the data analysis of the neutron star-neutron star merger in the event GW170807. To this scope, we consider two recent microscopic EOS models computed starting from two-body and three-body nuclear interactio...

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Bibliographic Details
Main Authors: Domenico Logoteta, Ignazio Bombaci
Format: Article
Language:English
Published: MDPI AG 2019-09-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/5/10/204