Hyperonic neutron star matter in light of GW170817
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DOI: 10.1002/asna.201913579
Abstract: Since 2013 the mass of pulsar PSR J0348+0432 ($M = 2.01\,M_{\odot}$) has provided a tight constraint on neutron star equation of state. However, a number of different analyses of the recently detected BNS merger (GW170817)… read more here.
Keywords: matter light; mass; neutron star; star matter ... See more keywords