STELLAR ELECTRON CAPTURE ON NEUTRON-RICH NUCLEI
The role of Electron Captures in pre-supernova:(A,Z)+e→(A,Z-1)+veEC on nuclei largely determines the mass of collapsing core(MCh~Y2e);EC reduces the pressure of degenerate electron gas and accelerates the collapse;EC produces neutrinos which leave the stellar core freely,carrying away energy and reducing the entropy.Because of the low entropy,most of the nucleons remain bound in large nuclei.
Alan A.Dzhioev A.I.Vdovin Ch.Stoyanov
Bogoliubov Laboratory of Theoretical Physics Joint Institute for Nuclear Research,Dubna,Russia Institute for Nuclear Research and Nuclear Energy,Sofia,Bulgaria
国内会议
深圳
英文
1-15
2017-11-26(万方平台首次上网日期,不代表论文的发表时间)