dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Guber, K. H. | |
dc.date.accessioned | 2013-05-07T13:10:01Z | |
dc.date.available | 2013-05-07T13:10:01Z | |
dc.date.issued | 2002-08 | |
dc.identifier.citation | Rauscher , T & Guber , K H 2002 , ' Direct neutron capture cross sections of Ni-62 in the s-process energy range ' , Physical Review C (nuclear physics) , vol. 66 , no. 2 , 028802 . https://doi.org/10.1103/PhysRevC.66.028802 | |
dc.identifier.issn | 2469-9985 | |
dc.identifier.uri | http://hdl.handle.net/2299/10637 | |
dc.description.abstract | Direct neutron capture on Ni-62 is calculated in the DWBA and the Maxwellian averaged cross sections and astrophysical reaction rates in the energy range relevant for s-process nucleosynthesis are given. It is confirmed that the thermal value of the capture cross section contains a subthreshold resonance contribution. Contrary to previous investigations it is found that the capture at higher energies is dominated by p waves, thus leading to a considerably increased cross section at s-process energies and a modified energy dependence. | en |
dc.format.extent | 4 | |
dc.format.extent | 126300 | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review C (nuclear physics) | |
dc.subject | SCATTERING | |
dc.subject | MASSIVE STARS | |
dc.subject | NUCLEOSYNTHESIS | |
dc.subject | REACTION-RATES | |
dc.title | Direct neutron capture cross sections of Ni-62 in the s-process energy range | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1103/PhysRevC.66.028802 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |