dc.contributor.author | Rauscher, T. | |
dc.contributor.author | Thielemann, Friedrich-Karl | |
dc.contributor.author | Kratz, K.L. | |
dc.date.accessioned | 2013-07-02T14:02:01Z | |
dc.date.available | 2013-07-02T14:02:01Z | |
dc.date.issued | 1997-08-04 | |
dc.identifier.citation | Rauscher , T , Thielemann , F-K & Kratz , K L 1997 , ' Applicability of the Hauser-Feshbach approach for the determination of astrophysical reaction rates ' , Nuclear Physics A , vol. 621 , no. 1-2 , pp. C331-C334 . | |
dc.identifier.issn | 0375-9474 | |
dc.identifier.other | PURE: 1635978 | |
dc.identifier.other | PURE UUID: 78157cc0-1ead-4bec-ab17-04753d9dcf86 | |
dc.identifier.other | WOS: A1997XU96500067 | |
dc.identifier.other | Scopus: 0031552709 | |
dc.identifier.uri | http://hdl.handle.net/2299/11036 | |
dc.description.abstract | Nuclear Astrophysics requires the knowledge of reaction rates over a wide range of nuclei and temperatures. In recent calculations the nuclear level density – as an important ingredient to the statistical model (Hauser-Feshbach) – has shown the highest uncertainties. In a back-shifted fermi-Gas formalism utilizing an energy-dependent level density parameter and employing microscopic corrections from a recent FRDM mass formula, we obtain a highly improved fit to experimental level densities. The resulting level density is used for determining criteria for the applicability of the statistical model | en |
dc.format.extent | 4 | |
dc.language.iso | eng | |
dc.relation.ispartof | Nuclear Physics A | |
dc.subject | LEVEL | |
dc.title | Applicability of the Hauser-Feshbach approach for the determination of astrophysical reaction rates | en |
dc.contributor.institution | Centre for Astrophysics Research | |
dc.description.status | Peer reviewed | |
rioxxterms.version | SMUR | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |