Hyperneutron Stars from an Ab Initio Calculation

Hyperneutron Stars from an Ab Initio Calculation

The equation of state (EOS) of neutron matter plays a decisive role in understanding the neutron star properties and the gravitational waves from neutron star mergers. At sufficient densities, the appearance of hyperons generally softens the EOS, leading to a reduction in the maximum mass of neutron...

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Bibliographic Details
Main Authors:	Hui Tong, Serdar Elhatisari, Ulf-G. Meißner
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Series:	The Astrophysical Journal
Subjects:	Nuclear physics
Online Access:	https://doi.org/10.3847/1538-4357/adba47
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