Lohs, A. ; Martinez-Pinedo, G. ; Fischer, T.

2016
Verlag Deutsches Elektronen-Synchrotron Hamburg
ISBN: 978-3-945931-08-0

2016Lohs, Andreas "Neutrino-Nucleon Interactions in Core Collapse Supernovae" in Proceedings, Magellan Workshop: Connecting Neutrino Physics and Astronomy / Dahmke, Stefan K.G., Meyer, Mikko, Vanhoefer, Laura (eds.), Deutsches Elektronen-Synchrotron, DESY : 2016 ; Magellan Workshop, 2016-03-17 - 2016-03-18, Hamburg
Magellan Workshop, HamburgHamburg, Germany, 17 Mar 2016 - 18 Mar 20162016-03-172016-03-18 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 11-18 (2016) [10.3204/DESY-PROC-2016-05/28]2016  

Abstract: Neutrino interactions in proto-neutron star matter are a major determinant for many key properties of core-collapse supernovae (CCSNe), such as the explosion mechanism or the nucleosynthesis of heavy elements. Recent works identify a need for increasingly precise interaction rates. This work presents an alternative way to compute the relativistic Hartree response for neutrino-nucleon interactions, improving upon previously derived expressions in several aspects. The result will then be compared to the so called elastic approximation which is widely used in supernova simulations, to asses the validity and limitations of the latter.

1. FISH - FaInt Supernovae and Hypernovae: Mechanism and Nucleosynthesis (321263) (321263)

http://join2-wiki.gsi.de/foswiki/pub/Main/Artwork/join2_logo100x88.png Book/Proceedings/Report Dahmke, S. K. G. (Editor) ; Meyer, M. (Editor)Extern* ; Vanhoefer, L. (Editor)Extern*
Proceedings, Magellan Workshop : Connecting Neutrino Physics and Astronomy : Hamburg, Germany, March 17-18, 2016
2016Magellan Workshop, HamburgHamburg, Germany, 17 Mar 2016 - 18 Mar 20162016-03-172016-03-18 Hamburg : Verlag Deutsches Elektronen-Synchrotron, DESY-PROC 1-228 (2016) [10.3204/DESY-PROC-2016-05]2016     Files  Fulltext BibTeX | EndNote: XML, Text | RIS