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 language | English (US) |
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Pages (from-to) | 579-583 |
Number of pages | 5 |
Journal | Astrophysical Journal |
Volume | 397 |
Issue number | 2 |
DOIs | |
State | Published - 1992 |
Keywords
- Dense matter
- Nuclear reactions, nucleosynthesis, abundances
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science