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Screening enhancement of thermonuclear reactions in high density stars [electronic resource].

Published:
Washington, D.C : United States. Dept. of Energy. Office of the Assistant Secretary for Defense Programs, 1998.
Oak Ridge, Tenn. : Distributed by the Office of Scientific and Technical Information, U.S. Dept. of Energy.
Physical Description:
81 Kilobytes pages : digital, PDF file
Additional Creators:
Lawrence Livermore National Laboratory, United States. Department of Energy. Office of the Assistant Secretary for Defense Programs, and United States. Department of Energy. Office of Scientific and Technical Information
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Summary:
The screening function for zero separation for two is reacting nuclei in a strongly coupled OCP plasma is obtained using new very accurate Monte Carlo OCP fluid simulation data by two methods. The first method obtains, H(0), the screening function at x =0, from the difference of free energies before and after the reaction. The second method is a direct fitting of the Widom expansion in powers of x²{sup }to the MC data for the pair distribution function, g(x). The two methods agree to 2%
Report Numbers:
E 1.99:ucrl-jc-132095
E 1.99: dp0102012
dp0102012
ucrl-jc-132095
Subject(s):
Other Subject(s):
Note:
Published through SciTech Connect.
09/28/1998.
"ucrl-jc-132095"
" dp0102012"
"DP0102012"
International Workshop on the Physics of Nonideal Plasma, PNP 9, Rostock (DE), 09/06/1998--09/11/1998.
DeWitt, H.; Slattery, W.
Funding Information:
W-7405-ENG-48
View MARC record | catkey: 13824618