dorsal/arxiv
View SchemaDelayed Collapse of Protoneutron Stars with Kaon Condensate
| Authors | Masatomi Yasuhira, Toshitaka Tatsumi |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9908064 |
| URL | https://arxiv.org/abs/nucl-th/9908064 |
| DOI | 10.1016/S0375-9474(99)00737-X |
| Journal | Nucl.Phys. A663 (2000) 881-884 |
Abstract
Equation of state with kaon condensate is derived for isentropic and neutrino-trapped matter. Both are important ingredients to study the delayed collapse of protoneutron stars. Solving the TOV equation, we discuss the static properties of protoneutron stars and implications for their delayed collapse.
{
"annotation_id": "34a0db8a-7fe0-4482-aac1-4d7ec83340e6",
"date_created": "2026-03-02T18:00:25.834000Z",
"date_modified": "2026-03-02T18:00:25.834000Z",
"file_hash": "e11fac0286fea84541bb377efb5ab7cc71b30793bd7ecf2b81603caf108ff6e5",
"private": false,
"record": {
"abstract": "Equation of state with kaon condensate is derived for isentropic and\nneutrino-trapped matter. Both are important ingredients to study the delayed\ncollapse of protoneutron stars. Solving the TOV equation, we discuss the static\nproperties of protoneutron stars and implications for their delayed collapse.",
"arxiv_id": "nucl-th/9908064",
"authors": [
"Masatomi Yasuhira",
"Toshitaka Tatsumi"
],
"categories": [
"nucl-th",
"astro-ph"
],
"doi": "10.1016/S0375-9474(99)00737-X",
"journal_ref": "Nucl.Phys. A663 (2000) 881-884",
"title": "Delayed Collapse of Protoneutron Stars with Kaon Condensate",
"url": "https://arxiv.org/abs/nucl-th/9908064"
},
"schema_id": "dorsal/arxiv",
"source": {
"execution_id": "9cc50da4-b148-4d36-b729-57ec6ca2e56d",
"id": "arXiv Dataset IDs",
"type": "Model",
"variant": "snapshot-2026-03-01",
"version": "0.1.0"
},
"user_id": 1000002
}