| dc.contributor.author | Mocelj, D. | |
| dc.contributor.author | Rauscher, T. | |
| dc.contributor.author | Thielemann, Friedrich-Karl | |
| dc.contributor.author | Martinez-Pinedo, G. | |
| dc.contributor.author | Langanke, K. | |
| dc.contributor.author | Pacearescu, L. | |
| dc.contributor.author | Fassler, A. | |
| dc.date.accessioned | 2013-07-02T10:32:05Z | |
| dc.date.available | 2013-07-02T10:32:05Z | |
| dc.date.issued | 2005-10 | |
| dc.identifier.citation | Mocelj , D , Rauscher , T , Thielemann , F-K , Martinez-Pinedo , G , Langanke , K , Pacearescu , L & Fassler , A 2005 , ' Towards a parity-dependent level density for astrophysics ' , Journal of Physics G: Nuclear and Particle Physics , vol. 31 , no. 10 , pp. S1927-S1930 . https://doi.org/10.1088/0954-3899/31/10/103 | |
| dc.identifier.issn | 0954-3899 | |
| dc.identifier.uri | http://hdl.handle.net/2299/11002 | |
| dc.description.abstract | Astrophysical reaction rates are sensitive to the parity distribution at low excitation energies. We combine a formula for the energy-dependent parity distribution with a microscopic-macroscopic nuclear level density. This approach describes well the transition from low excitation energies where a single parity dominates to high excitations where the two densities are equal. | en |
| dc.format.extent | 4 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | Journal of Physics G: Nuclear and Particle Physics | |
| dc.title | Towards a parity-dependent level density for 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 | 10.1088/0954-3899/31/10/103 | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
