skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Condensed matter effects on nuclear fusion rates in laboratory and astrophysical environments

Journal Article · · International Journal of Theoretical Physics; (United States)
DOI:https://doi.org/10.1007/BF00671799· OSTI ID:5763650
;  [1];  [2]
  1. Purdue Univ. West Lafayette, IN (United States)
  2. Electric Power Research Institute, Palo Alto, CA (United States)

Previously overlooked condensed matter effects (CME) can significantly influence nuclear fusion rates in both laboratory and astrophysical environments. In dense plasmas, the ensemble of fusing particles has a significant exchange of kinetic and potential energies. Thus, there are diminished effective flux velocities resulting in a significant selective reduction of fusion rates. The authors CME predictions are testable in laboratory experiments and have broad-ranging implications on the fusion rates for stellar media in general. By calculating reaction rates for p(p,e[sup +]v[sub e]) D and [sup 7]Be(p,[gamma])[sup 8]B in the sun, they show that CME help to solve the solar neutrino problem.

OSTI ID:
5763650
Journal Information:
International Journal of Theoretical Physics; (United States), Vol. 32:7; ISSN 0020-7748
Country of Publication:
United States
Language:
English

Similar Records

Condensed matter effects for high density fusion and the solar neutrino problem
Journal Article · Fri Oct 01 00:00:00 EDT 1993 · Bulletin of the American Physical Society · OSTI ID:5763650

Nuclear fusion in dense matter: Reaction rate and carbon burning
Journal Article · Mon Aug 01 00:00:00 EDT 2005 · Physical Review. C, Nuclear Physics · OSTI ID:5763650

Astrophysical impact of the updated {sup 9}Be(p,α){sup 6}Li and {sup 10}B(p,α){sup 7}Be reaction rates as deduced by THM
Journal Article · Thu Oct 01 00:00:00 EDT 2015 · Astrophysical Journal · OSTI ID:5763650