Nuclear Q Values in a Dense Stellar Plasma

Details Nuclear Q Values in a Dense Stellar Plasma Nuclear Q Values in a Dense Stellar Plasma

Jun 1969

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1969phrv..182.1369s&link_type=abstract

Physical Review, vol. 182, Issue 5, pp. 1369-1373

Physics

1

Scientific paper

Corrections to nuclear Q values in a dense stellar plasma are calculated by means of a modified ionic cluster expansion in which the electrons are treated as a dielectric medium. Corrections beyond the weak-screening (Debye) approximation are given in tabular form for purposes of interpolation. A comparison between the Debye correction and the double-cluster correction is made for the chemical potential of a one-component plasma; the latter correction is ~20% of the former for a plasma parameter as large as unity.

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