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