Photodisintegration studies of astrophysically relevant p-nuclei
The majority of the light elements up to iron (Fe) are formed by successive rounds of thermonuclear fusion burning in the stellar interiors. The nuclei heavier than iron (Z>26) are being synthesized mainly by neutron-capture reactions - the astrophysical r-and s-processes. There are 35 neutron de...
| Main Author: | |
|---|---|
| Other Authors: | |
| Format: | Others |
| Language: | English |
| Published: |
Forschungszentrum Dresden
2013
|
| Subjects: | |
| Online Access: | http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-124733 http://nbn-resolving.de/urn:nbn:de:bsz:d120-qucosa-124733 http://www.qucosa.de/fileadmin/data/qucosa/documents/12473/19256.pdf |