| dc.contributor.author | Fulop, Zs. | |
| dc.contributor.author | Kiss, A.Z. | |
| dc.contributor.author | Somorjai, E. | |
| dc.contributor.author | Rolfs, C.E. | |
| dc.contributor.author | Trautvetter, H.P. | |
| dc.contributor.author | Rauscher, T. | |
| dc.contributor.author | Oberhummer, H. | |
| dc.date.accessioned | 2013-07-02T14:02:04Z | |
| dc.date.available | 2013-07-02T14:02:04Z | |
| dc.date.issued | 1996-07 | |
| dc.identifier.citation | Fulop , Z , Kiss , A Z , Somorjai , E , Rolfs , C E , Trautvetter , H P , Rauscher , T & Oberhummer , H 1996 , ' Ge-70(alpha,gamma)Se-74 cross section measurements at energies of astrophysical interest ' , Zeitschrift fur Physik A-Hadrons and Nuclei , vol. 355 , no. 2 , pp. 203-207 . | |
| dc.identifier.issn | 0939-7922 | |
| dc.identifier.uri | http://hdl.handle.net/2299/11038 | |
| dc.description.abstract | The cross section of the reaction Ge-70(alpha, gamma)Se-74 has been measured over the bombarding energy range of 5.05 MeV <E(alpha) <7.80 MeV using single and coincidence gamma spectroscopy techniques. The experimental S-factor values are in agreement with theoretical statistical-model calculations. Reaction rates for the Ge-70(alpha, gamma)Se-74 and the inverse (gamma, alpha) reactions have been determined for appropriate temperatures. | en |
| dc.format.extent | 5 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Zeitschrift fur Physik A-Hadrons and Nuclei | |
| dc.subject | DETECTOR | |
| dc.subject | P-PROCESS | |
| dc.title | Ge-70(alpha,gamma)Se-74 cross section measurements at energies of astrophysical interest | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
