University of Hertfordshire

By the same authors

Uncertainties in the Production of p Nuclides in SN Ia Determined by Monte Carlo Variations

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Documents

  • 1807.11475

    Accepted author manuscript, 211 KB, PDF document

  • Thomas Rauscher
  • Nobuya Nishimura
  • Raphael Hirschi
  • Alex St J. Murphy
  • Gabriele Cescutti
  • Claudia Travaglio
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Original languageEnglish
Title of host publicationNuclei in the Cosmos XV
EditorsLucio Gialanella, Gianluca Imbriani, Alba Formicola, Matthias Junker
PublisherSpringer Science and Business Media, LLC
Pages429-432
Number of pages4
ISBN (Print)9783030138752
DOIs
Publication statusPublished - 20 Aug 2019
Event15th International Symposium on Nuclei in the Cosmos, NIC 2018 - L'Aquila, Italy
Duration: 24 Jun 201829 Jun 2018

Publication series

NameSpringer Proceedings in Physics
Volume219
ISSN (Print)0930-8989
ISSN (Electronic)1867-4941

Conference

Conference15th International Symposium on Nuclei in the Cosmos, NIC 2018
CountryItaly
CityL'Aquila
Period24/06/1829/06/18

Abstract

Several thousand tracers from a 2D model of a thermonuclear supernova were used in a Monte Carlo post-processing approach to determine p-nuclide abundance uncertainties originating from nuclear physics uncertainties in the reaction rates.

Notes

© Springer Nature Switzerland AG 2019

ID: 17387846