Nuclear Electron Capture in a Plasma

Details Nuclear Electron Capture in a Plasma Nuclear Electron Capture in a Plasma

1997-04-30

arxiv.org/abs/astro-ph/9704299v1

Astrophys.J.489:968,1997

Astronomy and Astrophysics

Astrophysics

20 pages, RevTeX

Scientific paper

10.1086/304828

We consider the electron density at the position of an ion of charge Ze in a plasma under conditions approximating those in the core of the sun. Numerical calculations have shown that the plasma effects on the density, over and above the ordinary Coulomb factors that are obtained in the absence of electron-electron interactions, are well represented by a reduction factor, exp{- Z e^2 beta kappa_D }, where beta is the inverse temperature and kappa_D is the Debye wave length. Although this factor is the direct analogue of the Salpeter enhancement factor for the fusion rates in stars, the elementary considerations that establish it in the fusion case are not applicable to the determination of the electron density and the resulting electron capture rates. We show analytically, through a sum rule that leads to a well-defined perturbative approach, that in the limit of Boltzmann statistics the Salpeter factor indeed provides the leading correction. We estimate residual effects, both from Fermi statistics and from short range terms.

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