Neutron Star Properties in the Thomas-Fermi Model
作者： Ch. Schaab , M. K. Weigel , F. Weber , K. Strobel
DOI: 10.1142/S0218301397000329
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摘要: The modern nucleon-nucleon interaction of Myers and Swiatecki, adjusted to the properties finite nuclei, parameters mass formula, behavior optical potential is used calculate β-equilibrated neutron star matter, study impact this equation state on (rapidly rotating) stars their cooling behavior. results are in excellent agreement with outcome calculations performed for a broad collection sophisticated nonrelativistic as well relativistic models state.
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