dc.contributor.author | Mohr, P. | |
dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Sonnabend, K. | |
dc.contributor.author | Vogt, K. | |
dc.contributor.author | Zilges, A. | |
dc.date.accessioned | 2013-07-02T13:02:01Z | |
dc.date.available | 2013-07-02T13:02:01Z | |
dc.date.issued | 2003-05-05 | |
dc.identifier.citation | Mohr , P , Rauscher , T , Sonnabend , K , Vogt , K & Zilges , A 2003 , ' Photoreactions in nuclear astrophysics ' , Nuclear Physics A , vol. 718 , pp. 243C-246C . https://doi.org/10.1016/S0375-9474(03)00721-8 | |
dc.identifier.issn | 0375-9474 | |
dc.identifier.uri | http://hdl.handle.net/2299/11023 | |
dc.description.abstract | Cross sections and reaction rates of (gamma,n) reactions have been measured close above threshold with the photoactivation technique. The experimental data for W-186,Pt-190,Pt-192,Pt-198, Hg-196,Hg-198,Hg-204, Au-197, and Pb-204 show good agreement with theoretical predictions. | en |
dc.format.extent | 4 | |
dc.language.iso | eng | |
dc.relation.ispartof | Nuclear Physics A | |
dc.subject | PHOTON BATH | |
dc.subject | GAMMA | |
dc.subject | P-PROCESS | |
dc.title | Photoreactions in nuclear astrophysics | 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)00721-8 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |