An Approach to Neutrino Radiative Transfer in Supernova Simulations
| dc.creator | Cardall, Christian Y. | |
| dc.date | 2004-04-20 | |
| dc.date.accessioned | 2026-07-07T02:12:57Z | |
| dc.date.available | 2026-07-07T02:12:57Z | |
| dc.description | Neutrinos dominate the energetics of core-collapse supernovae, and are believed to play an important role in driving the explosion. The development of a spatially multidimensional neutrino radiative transfer code is a key part of the Terascale Supernova Initiative, a multi-year effort aimed at understanding the supernova explosion mechanism through supercomputer simulations. I will describe the conservative formulations of general relativistic radiative transfer we have developed for this application, and the algorithm we are implementing in our parallel code. | |
| dc.description | 11 pages. Contribution to the proceedings of Numerical Methods for Multidimensional Radiative Transfer Problems (RadConf2003), Heidelberg, Germany, 24-26 September 2003, edited by R. Rannacher and R. Wehrse | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0404401 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0404401 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/7640 | |
| dc.subject | Astrophysics | |
| dc.title | An Approach to Neutrino Radiative Transfer in Supernova Simulations | |
| dc.type | text |