Conference item icon

Conference item

Nuclear structure theory for the astrophysical rp-process and r-process

Abstract:
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 for displacement energies to obtain the masses of proton-rich nuclei needed for the rp-process. The second uses a model for configuration mixing near Sn-132 to provide Q values and beta-decay lifetimes for the r-process.
Publication status:
Published

Actions


Access Document


Authors


More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Mathematical Institute
Role:
Author
Expand authors...
Journal:
NUCLEAR PHYSICS A
Volume:
719
Pages:
177C-184C
Publication date:
2003-05-19
Event title:
17th International Nuclear Physics Divisional Conference of the European-Physical-Society
DOI:
ISSN:
0375-9474
Source identifiers:
13547
Keywords:
Pubs id:
pubs:13547
UUID:
uuid:3c5140cd-15ad-40a5-ad14-a097faa49fca
Local pid:
pubs:13547
Deposit date:
2012-12-19

Terms of use


Views and Downloads






If you are the owner of this record, you can report an update to it here: Report update to this record

TO TOP