Parity-Dependence in the Nuclear Level Density

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Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies, where a single parity dominates, to high excitations where the two densities are equal.
4 pages, 3 figures; contribution to Nuclei In The Cosmos VIII, to appear in Nucl. Phys. A

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Nuclear Theory

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http://salesiana.dossiersoluciones.com/handle/123456789/82262

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/nucl-th/0407043
 http://arxiv.org/abs/nucl-th/0407043
 Nucl.Phys. A758 (2005) 154-157
 doi:10.1016/j.nuclphysa.2005.05.032

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