dc.contributor.author | Vogt, K. | |
dc.contributor.author | Mohr, P. | |
dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Sonnabend, K. | |
dc.contributor.author | Zilges, A. | |
dc.date.accessioned | 2013-07-02T12:47:10Z | |
dc.date.available | 2013-07-02T12:47:10Z | |
dc.date.issued | 2003-05-05 | |
dc.identifier.citation | Vogt , K , Mohr , P , Rauscher , T , Sonnabend , K & Zilges , A 2003 , ' Determination of (gamma,n) reaction rates for the astrophysical gamma process ' , Nuclear Physics A , vol. 718 , pp. 575C-577C . https://doi.org/10.1016/S0375-9474(03)00857-1 | |
dc.identifier.issn | 0375-9474 | |
dc.identifier.uri | http://hdl.handle.net/2299/11020 | |
dc.description.abstract | (gamma,n) cross sections and reaction rates in the astrophysical gamma-process have been measured for the nucleus Pb-204 using the method of photoactivation. Some peculiarities of the (gamma,n) cross.section of this nucleus are discussed. | en |
dc.format.extent | 3 | |
dc.language.iso | eng | |
dc.relation.ispartof | Nuclear Physics A | |
dc.subject | THRESHOLD | |
dc.subject | P-PROCESS | |
dc.title | Determination of (gamma,n) reaction rates for the astrophysical gamma process | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1016/S0375-9474(03)00857-1 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |