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ß-delayed neutron emission measurements around the third r-process abundance peak

Author
Caballero-Folch, R.; Domingo-Pardo, C.; Cortes, G.; Calviño, F.; Riego, A.
Type of activity
Presentation of work at congresses
Name of edition
XII International Symposium on Nuclei in the Cosmos (NIC XII)
Date of publication
2012
Presentation's date
2012-08-06
Book of congress proceedings
Proceedings of Science
First page
1
Last page
6
Project funding
FPA 2011-28770-C03-03 Datos nucleares para física nuclear e ingeniería nuclear
Repository
http://hdl.handle.net/2117/26863 Open in new window
Abstract
The elements heavier than iron are produced in the Universe mainly by means of the slow (s) and rapid (r) neutron capture processes (for a recent review see e.g. [1]). The latter nucleosynthesis mechanism occurs between the valley of stability and the neutron drip line, passing along the neutron shell closures where exceptionally long half-lives and small neutron capture cross sections yield the three characteristic abundance maxima at A ~ 80, 130 and 195.
Citation
Caballero-Folch, R. [et al.]. ß-delayed neutron emission measurements around the third r-process abundance peak. A: International Symposium on Nuclei in the Cosmos. "Proceedings of Science". Cairns: 2012, p. 1-6.
Group of research
ANT - Advanced Nuclear Technologies Research Group

Participants