A Thomas-Fermi model of warm nuclei

Details A Thomas-Fermi model of warm nuclei A Thomas-Fermi model of warm nuclei

Jan 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...235l..91b&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 235, Jan. 15, 1980, p. L91-L93. Research supported by the Ministere

Statistics

9

Gravitational Collapse, Neutron Stars, Nuclear Models, Supernovae, Thomas-Fermi Model, Density Distribution, Energetic Particles, Equations Of State, Quantum Statistics, Temperature Effects

Scientific paper

The average nuclear level density of spherical nuclei is computed with a
finite temperature Thomas-Fermi model. More than 80 percent of the low
energy nuclear excitations can be accounted for in terms of this
statistical model. The relevance for stellar collapse is discussed.

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