Pregled bibliografske jedinice broj: 518583
Stellar electron-capture rates calculated with the finite- temperature relativistic random-phase approximation
Stellar electron-capture rates calculated with the finite- temperature relativistic random-phase approximation // Physical Review C, 83 (2011), 4; 045807-1 doi:10.1103/PhysRevC.83.045807 (međunarodna recenzija, članak, znanstveni)
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Naslov
Stellar electron-capture rates calculated with the finite- temperature relativistic random-phase approximation
Autori
Niu, Yifei ; Paar, Nils ; Vretenar, Dario ; Meng, Jie
Izvornik
Physical Review C (0556-2813) 83
(2011), 4;
045807-1
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
weak-interaction rates; intermediate-mass nuclei; Mean-field theory; Hartree-bogoliubov theory; shell-model calculations; range a=45-65; rate tables; FP-shell; environments; supernovae
Sažetak
We introduce a self-consistent microscopic theoretical framework for modeling the process of electron capture on nuclei in stellar environment, based on relativistic energy density functionals. The finite-temperature relativistic mean-field model is used to calculate the single-nucleon basis and the occupation factors in a target nucleus, and Jπ=0±, 1±, and 2± charge- exchange transitions are described by the self-consistent finite- temperature relativistic random-phase approximation. Cross sections and rates are calculated for electron capture on 54, 56Fe and 76, 78Ge in stellar environment, and results compared with predictions of similar and complementary model calculations.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
UKF 17/08
119-1191005-1010 - Nuklearna struktura i nuklearna astrofizika (Vretenar, Dario, MZOS ) ( CroRIS)
Ustanove:
Prirodoslovno-matematički fakultet, Zagreb
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus