| dc.contributor.author | Sonnabend, K. | |
| dc.contributor.author | Mohr, P. | |
| dc.contributor.author | Vogt, K. | |
| dc.contributor.author | Zilges, A. | |
| dc.contributor.author | Mengoni, A. | |
| dc.contributor.author | Rauscher, T. | |
| dc.contributor.author | Beer, H. | |
| dc.contributor.author | Kappeler, F. | |
| dc.contributor.author | Gallino, R. | |
| dc.date.accessioned | 2013-08-21T12:45:03Z | |
| dc.date.available | 2013-08-21T12:45:03Z | |
| dc.date.issued | 2003-01-20 | |
| dc.identifier.citation | Sonnabend , K , Mohr , P , Vogt , K , Zilges , A , Mengoni , A , Rauscher , T , Beer , H , Kappeler , F & Gallino , R 2003 , ' The s-process branching at W-185 ' , The Astrophysical Journal , vol. 583 , no. 1 , pp. 506-513 . | |
| dc.identifier.issn | 0004-637X | |
| dc.identifier.uri | http://hdl.handle.net/2299/11434 | |
| dc.description.abstract | The neutron capture cross section of the unstable nucleus W-185 has been derived from experimental photoactivation data of the inverse reaction W-186(gamma, n) W-185. The new result of sigma = 687 +/- 110 mbarn confirms the theoretically predicted neutron capture cross section of W-185 of sigma approximate to 700 mbarn at kT = 30 keV. A neutron density in the classical s-process of n(n) = (3.8(-0.9)(+1.1)) x 10(8) cm(-3) is derived from the new data for the W-185 branching. In a stellar s-process model, one finds a significant overproduction of the residual s-only nucleus Os-186. | en |
| dc.format.extent | 8 | |
| dc.language.iso | eng | |
| dc.relation.ispartof | The Astrophysical Journal | |
| dc.subject | GAMMA-PROCESS | |
| dc.subject | STATISTICAL-MODEL CALCULATIONS | |
| dc.subject | R-PROCESS | |
| dc.subject | PHOTONEUTRON CROSS-SECTIONS | |
| dc.subject | methods : laboratory | |
| dc.subject | NUCLEAR-LEVEL DENSITY | |
| dc.subject | ASTROPHYSICAL REACTION-RATES | |
| dc.subject | nuclear reactions, nucleosynthesis, abundances | |
| dc.subject | NUCLEOSYNTHESIS | |
| dc.subject | HALF-LIVES | |
| dc.subject | NEUTRON-CAPTURE | |
| dc.subject | ASYMPTOTIC GIANT BRANCH | |
| dc.title | The s-process branching at W-185 | en |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.contributor.institution | School of Physics, Engineering & Computer Science | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
