Neutrino capture by r-process waiting-point nuclei
| dc.creator | Surman, Rebecca | |
| dc.creator | Engel, Jonathan | |
| dc.date | 1998-05-04 | |
| dc.date.accessioned | 2026-07-07T11:11:41Z | |
| dc.date.available | 2026-07-07T11:11:41Z | |
| dc.description | We use the Quasiparticle Random Phase Approximation to include the effects of low-lying Gamow-Teller and first forbidden strength in neutrino capture by very neutron-rich nuclei with N = 50, 82, or 126. For electron neutrinos in what is currently considered the most likely r-process site the capture cross sections are two or more times previous estimates. We briefly discuss the reliability of our calculations and their implications for nucleosynthesis. | |
| dc.description | 9 pages, 4 figures | |
| dc.identifier | https://arxiv.org/abs/nucl-th/9805007 | |
| dc.identifier | http://arxiv.org/abs/nucl-th/9805007 | |
| dc.identifier | Phys.Rev.C58:2526-2530,1998 | |
| dc.identifier | doi:10.1103/PhysRevC.58.2526 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/191177 | |
| dc.subject | Nuclear Theory | |
| dc.subject | Astrophysics | |
| dc.title | Neutrino capture by r-process waiting-point nuclei | |
| dc.type | text |