dorsal/arxiv
View SchemaProtoneutron stars with kaon condensate
| Authors | Toshitaka Tatsumi, Masatomi Yasuhira |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9904038 |
| URL | https://arxiv.org/abs/nucl-th/9904038 |
| DOI | 10.1016/S0375-9474(00)00103-2 |
| Journal | Nucl.Phys. A670 (2000) 218-221 |
Abstract
A new formulation is presented to treat fluctuations around the kaon condensate. Equation of state (EOS) is given for isothermal and isentropic cases in the heavy-baryon-limit (HBL). The coexistent phase appears in the latter case. The mass-radius relation is given for protoneutron stars and the possibility of the delayed collapse is discussed.
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"abstract": "A new formulation is presented to treat fluctuations around the kaon\ncondensate. Equation of state (EOS) is given for isothermal and isentropic\ncases in the heavy-baryon-limit (HBL). The coexistent phase appears in the\nlatter case. The mass-radius relation is given for protoneutron stars and the\npossibility of the delayed collapse is discussed.",
"arxiv_id": "nucl-th/9904038",
"authors": [
"Toshitaka Tatsumi",
"Masatomi Yasuhira"
],
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"doi": "10.1016/S0375-9474(00)00103-2",
"journal_ref": "Nucl.Phys. A670 (2000) 218-221",
"title": "Protoneutron stars with kaon condensate",
"url": "https://arxiv.org/abs/nucl-th/9904038"
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