dc.contributor.author |
Kokkoris, M |
en |
dc.contributor.author |
Galanopoulos, S |
en |
dc.contributor.author |
Demetriou, P |
en |
dc.contributor.author |
Harissopulos, S |
en |
dc.contributor.author |
Rauscher, T |
en |
dc.contributor.author |
Goriely, S |
en |
dc.date.accessioned |
2014-03-01T01:52:51Z |
|
dc.date.available |
2014-03-01T01:52:51Z |
|
dc.date.issued |
2003 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/26743 |
|
dc.subject |
Activity Techniques |
en |
dc.subject |
Cross Section |
en |
dc.subject |
Reaction Rate |
en |
dc.subject |
Statistical Model |
en |
dc.title |
Proton induced reaction cross section measurements on Se isotopes for the astrophysical p process |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevC.68.055803 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevC.68.055803 |
en |
heal.publicationDate |
2003 |
en |
heal.abstract |
As a continuation of a systematic study of reactions relevant to theastrophysical p process, the cross sections of the 74,76Se(p,gamma)75,77Br and82Se(p,n)82Br reactions have been measured at energies from 1.3 to 3.6 MeVusing an activation technique. The results are compared to the predictions ofHauser-Feshbach statistical model calculations using the NON-SMOKER and MOSTcodes. The sensitivity of the |
en |
heal.journalName |
Physical Review C |
en |
dc.identifier.doi |
10.1103/PhysRevC.68.055803 |
en |