In addition to numerous problems in the quest of the astrophysical site for the r-process, nuclear physics uncertainties of the r-process modeling are still high. For the β-decay rates predictions, they stem mostly from non self-consistency of the nuclear models. Also, the sole consideration of the allowed β-decay commonly used in large-scale microscopic schemes needs to be revised. The first systematic study of the GT and first-forbidden β-decays near the closed neutron shells at N=50, S2, 126 was performed in the self-consistent, EDF+CQRPA approach. The importance of the first-forbidden decays for Z≥50, N ≈ 82 nuclei and near N=126 closed shell is shown.SCOPUS: ar.jinfo:eu-repo/semantics/publishe
This Letter reports on a systematic study of β-decay half-lives of neutron-rich nuclei around doubly...
Commune avec ACENInternational audienceHeavy neutron-rich nuclei close to N=126 were produced by fra...
The pattern of isotopic abundances produced in rapid neutron capture, or r-process, nucleosynthesis ...
The β-decay rates of neutron-rich nuclei relevant to the r-process nucleosynthesis are mostly beyond...
Major astrophysical applications involve a huge number of exotic nuclei. Their beta-decay properties...
We investigated the effects of first-forbidden transitions in β decays on the production of the r-pr...
We investigated the effects of first-forbidden transitions in β decays on the production of the r -p...
Background: r-process nucleosynthesis models rely, by necessity, on nuclear structure models for inp...
We investigated the effects of first-forbidden transitions in β decays on the production of the r -p...
β− decay lifetimes are essential ingredients for r-process yield calculations. In N≈126 r-process wa...
An important effort has been developed in recent decades to measure the masses and β-decay rates of ...
This Letter reports on a systematic study of β-decay half-lives of neutron-rich nuclei around doubly...
Major astrophysical applications involve a huge number of exotic nuclei. An important effort has bee...
The [Formula Presented]-decay rates of neutron-rich nuclei relevant to the r-process nucleosynthesis...
Elements heavier than iron are being created in massive, explosive astrophysical scenarios such as c...
This Letter reports on a systematic study of β-decay half-lives of neutron-rich nuclei around doubly...
Commune avec ACENInternational audienceHeavy neutron-rich nuclei close to N=126 were produced by fra...
The pattern of isotopic abundances produced in rapid neutron capture, or r-process, nucleosynthesis ...
The β-decay rates of neutron-rich nuclei relevant to the r-process nucleosynthesis are mostly beyond...
Major astrophysical applications involve a huge number of exotic nuclei. Their beta-decay properties...
We investigated the effects of first-forbidden transitions in β decays on the production of the r-pr...
We investigated the effects of first-forbidden transitions in β decays on the production of the r -p...
Background: r-process nucleosynthesis models rely, by necessity, on nuclear structure models for inp...
We investigated the effects of first-forbidden transitions in β decays on the production of the r -p...
β− decay lifetimes are essential ingredients for r-process yield calculations. In N≈126 r-process wa...
An important effort has been developed in recent decades to measure the masses and β-decay rates of ...
This Letter reports on a systematic study of β-decay half-lives of neutron-rich nuclei around doubly...
Major astrophysical applications involve a huge number of exotic nuclei. An important effort has bee...
The [Formula Presented]-decay rates of neutron-rich nuclei relevant to the r-process nucleosynthesis...
Elements heavier than iron are being created in massive, explosive astrophysical scenarios such as c...
This Letter reports on a systematic study of β-decay half-lives of neutron-rich nuclei around doubly...
Commune avec ACENInternational audienceHeavy neutron-rich nuclei close to N=126 were produced by fra...
The pattern of isotopic abundances produced in rapid neutron capture, or r-process, nucleosynthesis ...