Pycnonuclear triple-α fusion rates

S. Schramm, K. Langanke, S. E. Koonin

Research output: Contribution to journalArticle

Abstract

Pycnonuclear triple-α reaction rates are calculated for mass densities from 108 to 5 × 109 g cm -3. The plasma is assumed to be a fluid phase of a particles interacting through both nuclear and Coulomb potentials. It is described by Jastrow-type two-body correlations. The many-body wave function is determined variationally within a space of trial two-body wave functions that reproduce the expected long- and short-range behaviors of the correlations. The resulting three-body fusion rates are compared to previous calculations.

Original languageEnglish (US)
Pages (from-to)579-583
Number of pages5
JournalAstrophysical Journal
Volume397
Issue number2
StatePublished - Jan 1 1992

Keywords

  • Dense matter
  • Nuclear reactions, nucleosynthesis, abundances

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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    Schramm, S., Langanke, K., & Koonin, S. E. (1992). Pycnonuclear triple-α fusion rates. Astrophysical Journal, 397(2), 579-583.