A Unified Equation for the Reaction Rate in Dense Matter Stars

Details A Unified Equation for the Reaction Rate in Dense Matter Stars A Unified Equation for the Reaction Rate in Dense Matter Stars

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..947..341g&link_type=abstract

VII LATIN AMERICAN SYMPOSIUM ON NUCLEAR PHYSICS AND APPLICATIONS. AIP Conference Proceedings, Volume 947, pp. 341-347 (2007).

Physics

Nuclear Physics

Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, Potential Models, Fusion And Fusion-Fission Reactions

Scientific paper

We analyze thermonuclear and pycnonuclear reaction rates in multi-component dense stellar plasma. First we describe calculations of the astrophysical S-factor at low energies using the Sa~o Paulo potential on the basis of the barrier penetration model. Then we present a simple phenomenological expression for a reaction rate. The expression contains several fit parameters which we adjust to reproduce the best microscopic calculations available in the literature.

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