dc.contributor.author | Descouvemont, P. | |
dc.contributor.author | Rauscher, T. | |
dc.date.accessioned | 2013-06-20T11:00:50Z | |
dc.date.available | 2013-06-20T11:00:50Z | |
dc.date.issued | 2006-10-17 | |
dc.identifier.citation | Descouvemont , P & Rauscher , T 2006 , ' Cross section predictions for hydrostatic and explosive burning ' , Nuclear Physics A , vol. 777 , pp. 137-156 . https://doi.org/10.1016/j.nuclphysa.2004.10.024 | |
dc.identifier.issn | 0375-9474 | |
dc.identifier.uri | http://hdl.handle.net/2299/10894 | |
dc.description.abstract | We review different models used for reactions involved in nuclear astrophysics. The reaction rate is defined for resonant as well as for non-resonant processes. For low-density nuclei, we describe the DWBA method, the potential model, the R-matrix method, and microscopic cluster models. The statistical model is developed for high-level densities. Details of calculations in the low- and high-density regimes are illustrated with new results concerning transfer reactions and level densities. (c) 2004 Elsevier B.V. All rights reserved. | en |
dc.format.extent | 20 | |
dc.format.extent | 284843 | |
dc.language.iso | eng | |
dc.relation.ispartof | Nuclear Physics A | |
dc.subject | GAMMA-PROCESS | |
dc.subject | THERMONUCLEAR REACTION-RATES | |
dc.subject | STATISTICAL-MODEL CALCULATIONS | |
dc.subject | RADIATIVE-CAPTURE REACTIONS | |
dc.subject | DIRECT NEUTRON-CAPTURE | |
dc.subject | ELASTIC-SCATTERING | |
dc.subject | NUCLEAR-LEVEL DENSITY | |
dc.subject | NON-SPHERICAL NUCLEI | |
dc.subject | ASTROPHYSICAL REACTION-RATES | |
dc.subject | SHELL NUCLEI | |
dc.title | Cross section predictions for hydrostatic and explosive burning | en |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1016/j.nuclphysa.2004.10.024 | |
rioxxterms.type | Other | |
herts.preservation.rarelyaccessed | true | |