Nuclear fission of superheavy elements can affect the r-process nucleosynthesis via a fission cycling process. In that process, the identification of the nuclide of a fission fragment and its abundance is essential for a precise evaluation of their contribution as seed nuclei of the r-process. We have investigated the nuclear fission of SHEs from the proton-rich side to the neutron-rich side using our three-and four-dimensional Langevin models [1, 4]. This model can reproduce the experimental data on nuclear fission of actinides and SHEs, while it can only provide various quantities to each fission fragment, we also developed a semi-empirical charge distribution model based on abundant experimental data of actinides [3]. A new semi-empirica...
The systematic data on the fission fragment mass distribution for nuclei ranging from Z = 88 to 120 ...
Fission plays a crucial role for the r-process nucleosynthesis in neutron star mergers. Due to the h...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
Nuclear fission is expected to play an essential role in the r-process nucleosynthesis via the fissi...
Nuclear fission is expected to play an essential role in the r-process nucleosynthesis via the fissi...
We have developed a full set of fission rates that include spontaneous fission, neutron-induced fiss...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
International audienceFission barriers for a large number of nuclei have been extracted from Gogny D...
International audienceNeutron star (NS) merger ejecta offer viable sites for the production of heavy...
Fission barriers for a large number of nuclei have been extracted from Gogny D1M potential energy su...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
We review recent work examining the influence of fission in rapid neutron capture (r-process) nucleo...
Nucleosynthesis by the rapid neutron-capture process (r-process) produces elements heavier than iron...
Fission plays a crucial role for the r-process nucleosynthesis in neutron star mergers. Due to the h...
Nucleosynthesis by the rapid neutron-capture process (r-process) produces elements heavier than iron...
The systematic data on the fission fragment mass distribution for nuclei ranging from Z = 88 to 120 ...
Fission plays a crucial role for the r-process nucleosynthesis in neutron star mergers. Due to the h...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
Nuclear fission is expected to play an essential role in the r-process nucleosynthesis via the fissi...
Nuclear fission is expected to play an essential role in the r-process nucleosynthesis via the fissi...
We have developed a full set of fission rates that include spontaneous fission, neutron-induced fiss...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
International audienceFission barriers for a large number of nuclei have been extracted from Gogny D...
International audienceNeutron star (NS) merger ejecta offer viable sites for the production of heavy...
Fission barriers for a large number of nuclei have been extracted from Gogny D1M potential energy su...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...
We review recent work examining the influence of fission in rapid neutron capture (r-process) nucleo...
Nucleosynthesis by the rapid neutron-capture process (r-process) produces elements heavier than iron...
Fission plays a crucial role for the r-process nucleosynthesis in neutron star mergers. Due to the h...
Nucleosynthesis by the rapid neutron-capture process (r-process) produces elements heavier than iron...
The systematic data on the fission fragment mass distribution for nuclei ranging from Z = 88 to 120 ...
Fission plays a crucial role for the r-process nucleosynthesis in neutron star mergers. Due to the h...
Comparing observational abundance features with nucleosynthesis predictions of stellar evolution or ...