Abstract. We present a new set of electron (e−) capture and β-decay rates that improves previous calculations by Takahara et al. and Oda et al. by: (a) incorporation of recent charge-exchange and β-decay data, (b) contributions of forbidden transitions, and (c) in-clusion of e − screening corrections. The experimental nuclear input is supplemented by theoretical data based on large-scale shell model calculations in the full sd-shell space using the USDB interaction. The impact of these new rates on the late-stage stellar evo-lution of 8.8M ⊙ star is demonstrated.
A detailed model is constructed for the calculation of electron capture rates of some fp-shell nucle...
Supernova simulations to date have assumed that during core collapse electron captures occur dominan...
International audienceThe impact of electron-capture (EC) cross sections on neutron-rich nuclei on t...
Intermediate mass stars develop a degenerate core constituted of O, Ne and Mg during their evolutio...
Recent shell-model calculations of weak-interaction rates for nuclei in the mass range A = 45 - 65 h...
The stellar electron capture on nuclei is an essential, semi-leptonic process that is especially sig...
Background: In the late stages of stellar core collapse just prior to core bounce, electron captures...
12 pages, 7 figures, submitted to Phys. Rev. CInternational audienceDuring the late stages of gravit...
We present shell-model calculations of electron capture strength distributions in A=28 nuclei and co...
In the course of a general study of electron capture and β-decay rates on fp shell nuclei which are ...
International audienceThe importance of microphysical inputs from laboratory nuclear experiments and...
New supernova progenitor models incorporating modern electron capture and beta de-cay rates have rec...
A detailed model is constructed for the calculation of electron capture rates of some fp-shell nucle...
Supernova simulations to date have assumed that during core collapse electron captures occur dominan...
International audienceThe impact of electron-capture (EC) cross sections on neutron-rich nuclei on t...
Intermediate mass stars develop a degenerate core constituted of O, Ne and Mg during their evolutio...
Recent shell-model calculations of weak-interaction rates for nuclei in the mass range A = 45 - 65 h...
The stellar electron capture on nuclei is an essential, semi-leptonic process that is especially sig...
Background: In the late stages of stellar core collapse just prior to core bounce, electron captures...
12 pages, 7 figures, submitted to Phys. Rev. CInternational audienceDuring the late stages of gravit...
We present shell-model calculations of electron capture strength distributions in A=28 nuclei and co...
In the course of a general study of electron capture and β-decay rates on fp shell nuclei which are ...
International audienceThe importance of microphysical inputs from laboratory nuclear experiments and...
New supernova progenitor models incorporating modern electron capture and beta de-cay rates have rec...
A detailed model is constructed for the calculation of electron capture rates of some fp-shell nucle...
Supernova simulations to date have assumed that during core collapse electron captures occur dominan...
International audienceThe impact of electron-capture (EC) cross sections on neutron-rich nuclei on t...