dc.contributor.author | He, J. J. | |
dc.contributor.author | Parikh, A. | |
dc.contributor.author | Brown, B. A. | |
dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Hou, S. Q. | |
dc.contributor.author | Zhang, Y. H. | |
dc.contributor.author | Zhou, X. H. | |
dc.contributor.author | Xu, H. S. | |
dc.date.accessioned | 2014-04-17T10:30:21Z | |
dc.date.available | 2014-04-17T10:30:21Z | |
dc.date.issued | 2014-03-05 | |
dc.identifier.citation | He , J J , Parikh , A , Brown , B A , Rauscher , T , Hou , S Q , Zhang , Y H , Zhou , X H & Xu , H S 2014 , ' Thermonuclear Ti-42(p, gamma)V-43 rate in type-I x-ray bursts ' , Physical Review C (nuclear physics) , vol. 89 , no. 3 , 035802 . https://doi.org/10.1103/PhysRevC.89.035802 | |
dc.identifier.issn | 2469-9985 | |
dc.identifier.uri | http://hdl.handle.net/2299/13381 | |
dc.description.abstract | The thermonuclear rate of the Ti-42(p, gamma)V-43 reaction has been reevaluated based on a recent precise proton separation energy measurement of S-p(V-43) = 83 +/- 43 keV. The astrophysical impact of our new rates has been investigated through one-zone postprocessing type-I x-ray burst calculations. It shows that the new experimental value of S-p significantly affects the yields of species for A approximate to 40-45. As well, the precision of the recent experimental S-p value constrains these yields to better than a factor of 3. | en |
dc.format.extent | 8 | |
dc.format.extent | 321514 | |
dc.language.iso | eng | |
dc.relation.ispartof | Physical Review C (nuclear physics) | |
dc.subject | ATOMIC MASS EVALUATION | |
dc.subject | STATISTICAL-MODEL CALCULATIONS | |
dc.subject | ASTROPHYSICAL REACTION-RATES | |
dc.subject | RP-PROCESS | |
dc.subject | NEUTRON-STARS | |
dc.subject | ENERGY-LEVELS | |
dc.subject | NUCLEOSYNTHESIS | |
dc.subject | SHELL | |
dc.subject | TEMPERATURE | |
dc.subject | DENSITY | |
dc.title | Thermonuclear Ti-42(p, gamma)V-43 rate in type-I x-ray bursts | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Science & Technology Research Institute | |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1103/PhysRevC.89.035802 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |