dorsal/arxiv
View SchemaFinite volume of baryons and the mass limit for neutron stars
| Authors | Qi-Ren Zhang, Bo-Qiang Ma, Walter Greiner |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9210019 |
| URL | https://arxiv.org/abs/nucl-th/9210019 |
| DOI | 10.1088/0954-3899/18/12/020 |
| Journal | J.Phys. G18 (1992) 2051-2060 |
Abstract
We confirmed the following idea by numerical calculation: The extended structure of baryons may make the nuclear equation of state stiffer at higher density while keeping the compression modulus for normal nuclear matter around its empirical value $K=240MeV$.The model built in this wayy fits all empirical data for normal nuclear matter and gives the mass limit of neutron stars compatible with the observation.
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"abstract": "We confirmed the following idea by numerical calculation: The extended\nstructure of baryons may make the nuclear equation of state stiffer at higher\ndensity while keeping the compression modulus for normal nuclear matter around\nits empirical value $K=240MeV$.The model built in this wayy fits all empirical\ndata for normal nuclear matter and gives the mass limit of neutron stars\ncompatible with the observation.",
"arxiv_id": "nucl-th/9210019",
"authors": [
"Qi-Ren Zhang",
"Bo-Qiang Ma",
"Walter Greiner"
],
"categories": [
"nucl-th",
"astro-ph"
],
"doi": "10.1088/0954-3899/18/12/020",
"journal_ref": "J.Phys. G18 (1992) 2051-2060",
"title": "Finite volume of baryons and the mass limit for neutron stars",
"url": "https://arxiv.org/abs/nucl-th/9210019"
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