Element synthesis calculations for stellar explosions: Robust uncertainties, sensitivities, and radioactive ion beam measurements

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    3 Scopus citations

    Abstract

    We utilize multiple-zone, post-processing element synthesis calculations to determine the impact of recent ORNL radioactive ion beam measurements on predictions of novae and X-ray burst simulations. We also assess the correlations between all relevant reaction rates and all synthesized isotopes, and translate nuclear reaction rate uncertainties into abundance prediction uncertainties, via a unique Monte Carlo technique.

    Original languageEnglish
    Pages (from-to)565-568
    Number of pages4
    JournalNuclear Physics A
    Volume746
    Issue number1-4 SPEC.ISS.
    DOIs
    StatePublished - Dec 27 2004

    Funding

    ORNL is managed by UT-Battelle, LLC, for the U.S. Dept. of Energy under contract DE-AC05-00OR22725.

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