| dc.contributor.author | Rauscher, T. | |
| dc.contributor.editor | Qian, Y-Z. | |
| dc.contributor.editor | Rehm, E. | |
| dc.contributor.editor | Schatz, H. | |
| dc.contributor.editor | Theilemann, Friedrich-Karl | |
| dc.date.accessioned | 2014-12-04T10:14:36Z | |
| dc.date.available | 2014-12-04T10:14:36Z | |
| dc.date.issued | 2004 | |
| dc.identifier.citation | Rauscher , T 2004 , Neutron captures and the r-process . in Y-Z Qian , E Rehm , H Schatz & F-K Theilemann (eds) , The r-Process : The Astrophysical Origin of the Heavy Elements and Related Rare Isotope Accelerator Physics . Procs from the Institute for Nuclear Theory , vol. 13 , World Scientific Publishing , pp. 63-72 , 1st Argonne/MSU/JINA/INT RIA Workshop on the r-Process , Seattle , 1/01/04 . | |
| dc.identifier.citation | conference | |
| dc.identifier.isbn | 981-256-032-7 | |
| dc.identifier.uri | http://hdl.handle.net/2299/14880 | |
| dc.description.abstract | The r-process involves neutron-rich nuclei far off stability for which no experimental cross sections are known. Therefore, one has to rely on theory. The difficulties in the predictions are briefly addressed. To investigate the impact of altered rates, a comparison of r-process production in hot bubble models with largely varied rates is shown. Due to the (n,gamma)-(gamma,n) equilibrium established at the onset of the r-process, only late-time neutron captures are important which mainly modify the abundances around the third r-process peak. | en |
| dc.format.extent | 10 | |
| dc.language.iso | eng | |
| dc.publisher | World Scientific Publishing | |
| dc.relation.ispartof | The r-Process | |
| dc.relation.ispartofseries | Procs from the Institute for Nuclear Theory | |
| dc.subject | RATES | |
| dc.subject | PROCESS ABUNDANCES | |
| dc.title | Neutron captures and the r-process | en |
| dc.contributor.institution | Centre for Astrophysics Research | |
| rioxxterms.type | Other | |
| herts.preservation.rarelyaccessed | true | |
