Self-consistent theory of stellar electron capture rates (CROSBI ID 593723)
Prilog sa skupa u časopisu | izvorni znanstveni rad | međunarodna recenzija
Podaci o odgovornosti
Paar, Nils ; Vretenar, Dario ; Niu, Y. F. ; Meng, J
engleski
Self-consistent theory of stellar electron capture rates
Recently a novel theory framework has been established for description of electron capture rates at temperatures and densities in stellar environment, based on the relativistic energy density functional. The model includes finite temperature relativistic mean field to determine single-particle basis and the corresponding thermal occupation factors of target nucleus, while relevant charge-exchange excitations are described by the self-consistent finite temperature relativistic random phase approximation (FTRRPA). The calculated electron capture rates for 54, 56Fe are shown in comparison with other advanced theory approaches.
electron capture; supernova
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Podaci o prilogu
012013-x.
2012.
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objavljeno
Podaci o matičnoj publikaciji
Naftali Auerbach, Michael Hass and Michael Paul
Bristol: Institute of Physics Publishing
1742-6588
Podaci o skupu
Nepoznat skup
predavanje
29.02.1904-29.02.2096