Calculation of the Astrophysical S-Factor S12 with the Lorentz Integral Transform View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2017-01

AUTHORS

Sergio Deflorian, Victor D. Efros, Winfried Leidemann

ABSTRACT

The LIT approach is tested for the calculation of astrophysical S-factors. As an example the S-factor of the reaction 2H(p,γ)3He is considered. It is discussed that a sufficiently high density of LIT states at low energies is necessary for a precise determination of S-factors. In particular it is shown that the hyperspherical basis is not very well suited for such a calculation and that a different basis system is much more advantageous. A comparison of LIT results with calculations, where continuum wave functions are explicitly used, shows that the LIT approach leads to reliable results. It is also shown how an error estimate of the LIT inversion can be obtained. More... »

PAGES

3

References to SciGraph publications

  • 2010-05. The Lorentz Integral Transform and its Inversion in FEW-BODY SYSTEMS
  • 2008-07. Calculation of a narrow resonance with the LIT method in FEW-BODY SYSTEMS
  • 2005-06. New inversion methods for the Lorentz Integral Transform in THE EUROPEAN PHYSICAL JOURNAL A
  • Identifiers

    URI

    http://scigraph.springernature.com/pub.10.1007/s00601-016-1167-0

    DOI

    http://dx.doi.org/10.1007/s00601-016-1167-0

    DIMENSIONS

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