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AbstractAbstract
[en] The deleptonization and cooling times of a newly born neutron star depend on the equation of state (EOS) and neutrino opacities in dense matter. Through model calculations we show that effects of Pauli blocking and many-body correlations due to strong interactions reduce both the neutral and charged current neutrino cross sections by large factors compared to the case in which these effects are ignored. (orig.)
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Buballa, M.; Noerenberg, W.; Wambach, J.; Wirzba, A. (eds.); Gesellschaft fuer Schwerionenforschung mbH, Darmstadt (Germany); 442 p; 1998; p. 187-200; 26. international workshop on gross properties of nuclei and nuclear excitations: Nuclear astrophysics (Hirschegg '98); Hirschegg (Austria); 11-17 Jan 1998
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