STELLAR ELECTRON-CAPTURE RATES: A COVARIANT DENSITY FUNCTIONAL CALCULATION

被引：0

作者：

Niu, Y. F. ^{[1
]}

Paar, N. ^{[2
]}

Vretenar, D. ^{[2
]}

Meng, J. ^{[1
,3
,4
]}

机构：

[1] Peking Univ, Sch Phys, State Key Lab Nucl Phys & Technol, Beijing 100871, Peoples R China

[2] Univ Zagreb, Fac Sci, Dept Phys, Zagreb 41000, Croatia

[3] Beihang Univ, Sch Phys & Nucl Energy Engn, Beijing 100191, Peoples R China

[4] Univ Stellenbosch, Dept Phys, Stellenbosch, South Africa

来源：

NUCLEAR STRUCTURE IN CHINA 2012 | 2013年

关键词：

electron capture; covariant density functional theory; random phase approximation; finite temperature; SHELL NUCLEI; DISTRIBUTIONS;

D O I：

暂无

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Gamow-Teller transitions and stellar electron-capture rates in hot nuclei are computed using the self-consistent finite-temperature relativistic random-phase approximation (FTRRPA). The predicted electron-capture rates in stellar environment for Fe-54,Fe-56 are consistent with those obtained in the shell-model approach. The FTRRPA provides an efficient and accurate theoretical framework for large-scale calculations of stellar electron-capture rates.

引用

页码：181 / 184

页数：4

共 13 条

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