dorsal/arxiv
View SchemaHigh density behaviour of nuclear symmetry energy
| Authors | D. N. Basu, Tapan Mukhopadhyay |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0603073 |
| URL | https://arxiv.org/abs/nucl-th/0603073 |
| Journal | Acta Phys.Polon. B38 (2007) 169-180 |
Abstract
Role of the isospin asymmetry in nuclei and neutron stars, with an emphasis on the density dependence of the nuclear symmetry energy, is discussed. The symmetry energy is obtained using the isoscalar as well as isovector components of the density dependent M3Y effective interaction. The constants of density dependence of the effective interaction are obtained by reproducing the saturation energy per nucleon and the saturation density of spin and isospin symmetric cold infinite nuclear matter. Implications for the density dependence of the symmetry energy in case of a neutron star are discussed, and also possible constraints on the density dependence obtained from finite nuclei are compared.
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"abstract": "Role of the isospin asymmetry in nuclei and neutron stars, with an emphasis\non the density dependence of the nuclear symmetry energy, is discussed. The\nsymmetry energy is obtained using the isoscalar as well as isovector components\nof the density dependent M3Y effective interaction. The constants of density\ndependence of the effective interaction are obtained by reproducing the\nsaturation energy per nucleon and the saturation density of spin and isospin\nsymmetric cold infinite nuclear matter. Implications for the density dependence\nof the symmetry energy in case of a neutron star are discussed, and also\npossible constraints on the density dependence obtained from finite nuclei are\ncompared.",
"arxiv_id": "nucl-th/0603073",
"authors": [
"D. N. Basu",
"Tapan Mukhopadhyay"
],
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"nucl-th",
"astro-ph"
],
"journal_ref": "Acta Phys.Polon. B38 (2007) 169-180",
"title": "High density behaviour of nuclear symmetry energy",
"url": "https://arxiv.org/abs/nucl-th/0603073"
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