We provide a theoretical overview of r-process nucleosynthesis. We then identify the nuclear properties that have the greatest astrophysical impact according to recent sensitivity studies as: nuclear masses, β decays and neutron capture rates. Finally, we briefly discuss how the NuCRL model can enhance the performance of the relevant simulations
We present the status of nucleosynthesis beyond Sr, using up-to-date nuclear inputs for both the slo...
The identification of the astrophysical site and the specific conditions in which r-process nucleosy...
© 2019 IOP Publishing Ltd. This is an exciting time for the study of r-process nucleosynthesis. Rece...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
About half of the nuclei heavier than iron observed in nature are produced by the socalled rapid neu...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
Although important effort has been devoted in the last decades to measure decay half-lives and react...
The origin of the heaviest elements in our Universe is an unresolved mystery. We know that half of t...
The overarching aim of my PhD research is to deepen our understanding of r-process nu- cleosynthesis...
The pattern of isotopic abundances produced in rapid neutron capture, or r-process, nucleosynthesis ...
The astrophysical r-process produces about half of the elements heavier than iron in the Universe an...
We examined a potential r-process site by modeling nucleosynthesis in a late-stage supernova explosi...
About half of the nuclei heavier than iron observed in nature are produced by the so-called rapid ne...
Rapid neutron capture in stellar explosions is responsible for the heaviest elements in nature, up t...
Theoretically predicted yields of elements created by the rapid neutron capture (r-) process carry p...
We present the status of nucleosynthesis beyond Sr, using up-to-date nuclear inputs for both the slo...
The identification of the astrophysical site and the specific conditions in which r-process nucleosy...
© 2019 IOP Publishing Ltd. This is an exciting time for the study of r-process nucleosynthesis. Rece...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
About half of the nuclei heavier than iron observed in nature are produced by the socalled rapid neu...
In rapid neutron capture, or r-process, nucleosynthesis, heavy elements are built up via a sequence ...
Although important effort has been devoted in the last decades to measure decay half-lives and react...
The origin of the heaviest elements in our Universe is an unresolved mystery. We know that half of t...
The overarching aim of my PhD research is to deepen our understanding of r-process nu- cleosynthesis...
The pattern of isotopic abundances produced in rapid neutron capture, or r-process, nucleosynthesis ...
The astrophysical r-process produces about half of the elements heavier than iron in the Universe an...
We examined a potential r-process site by modeling nucleosynthesis in a late-stage supernova explosi...
About half of the nuclei heavier than iron observed in nature are produced by the so-called rapid ne...
Rapid neutron capture in stellar explosions is responsible for the heaviest elements in nature, up t...
Theoretically predicted yields of elements created by the rapid neutron capture (r-) process carry p...
We present the status of nucleosynthesis beyond Sr, using up-to-date nuclear inputs for both the slo...
The identification of the astrophysical site and the specific conditions in which r-process nucleosy...
© 2019 IOP Publishing Ltd. This is an exciting time for the study of r-process nucleosynthesis. Rece...
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