Nuclear structure theory for the astrophysical rp-process and r-process
The astrophysical processes of rapid-proton capture and rapid-neutron capture require the knowledge of many nuclear properties which are not known from experiment. I will describe two examples of how theoretical models are used to provide this input. The first of these uses the Hartree-Fock method f...
| Main Authors: | , , , , , , , , |
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| Format: | Conference item |
| Published: |
2003
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