dorsal/arxiv
View SchemaPauli exclusion operator and binding energy of nuclear matter
| Authors | E. Schiller, H. Müther, P. Czerski |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/9812011 |
| URL | https://arxiv.org/abs/nucl-th/9812011 |
| DOI | 10.1103/PhysRevC.59.2934 10.1103/PhysRevC.60.059901 |
| Journal | Phys.Rev.C59:2934-2936,1999; Erratum-ibid.C60:059901,1999 |
Abstract
Brueckner-Hartree-Fock calculations are performed for nuclear matter with an exact treatment of the Pauli exclusion operator in the Bethe-Goldstone equation. The differences in the calculated binding energy, compared to the angle-average approximation, which is commonly used, are non-negligible. These difference exhibits a specific density dependence, which shifts the calculated saturation point towards smaller densities. This effect is observed for various versions of modern models for the NN interaction.
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"abstract": "Brueckner-Hartree-Fock calculations are performed for nuclear matter with an\nexact treatment of the Pauli exclusion operator in the Bethe-Goldstone\nequation. The differences in the calculated binding energy, compared to the\nangle-average approximation, which is commonly used, are non-negligible. These\ndifference exhibits a specific density dependence, which shifts the calculated\nsaturation point towards smaller densities. This effect is observed for various\nversions of modern models for the NN interaction.",
"arxiv_id": "nucl-th/9812011",
"authors": [
"E. Schiller",
"H. M\u00fcther",
"P. Czerski"
],
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"nucl-th"
],
"doi": "10.1103/PhysRevC.59.2934 10.1103/PhysRevC.60.059901",
"journal_ref": "Phys.Rev.C59:2934-2936,1999; Erratum-ibid.C60:059901,1999",
"title": "Pauli exclusion operator and binding energy of nuclear matter",
"url": "https://arxiv.org/abs/nucl-th/9812011"
},
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