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| HAL : in2p3-00022776, version 1 |
| DOI : 10.1103/PhysRevA.36.1824 |
| Fiche détaillée |  Récupérer au format |
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| Physical Review A: Atomic, Molecular and Optical Physics 36 (1987) 1824-1833 |
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| Wigner-Kirkwood expansion of the phase-space density for semi-infinite nuclear matter |
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| M. Durand1P. Schuck1X. Vinas |
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| (1987) |
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| The phase-space distribution of semi-infinite nuclear matter is expanded in an ħ series analogous to the low-temperature expansion of the Fermi function. Besides the usual Wigner-Kirkwood expansion, oscillatory terms are derived. In the case of a Woods-Saxon potential, a smallness parameter is defined, which determines the convergence of the series and explains the very rapid convergence of the Wigner-Kirkwood expansion for average (nuclear) binding energies. |
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| 1 : | LPSC - Laboratoire de Physique Subatomique et de Cosmologie |
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| Thème(s) | : | Physique/Physique Nucléaire Théorique Physique/Physique Quantique |
| in2p3-00022776, version 1 | |
| http://hal.in2p3.fr/in2p3-00022776 | |
| oai:hal.in2p3.fr:in2p3-00022776 | |
| Contributeur : Emmanuelle Vernay | |
| Soumis le : Jeudi 18 Mai 2000, 15:42:31 | |
| Dernière modification le : Mardi 23 Mai 2006, 13:42:23 | |
