Solar fusion cross sections
Journal Article (Journal Article)
We review and analyze the available information on the nuclear-fusion cross sections that are most important for solar energy generation and solar neutrino production. We provide best values for the low-energy cross-section factors and, wherever possible, estimates of the uncertainties. We also describe the most important experiments and calculations that are required in order to improve our knowledge of solar fusion rates. © 1998 The American Physical Society.
Full Text
Duke Authors
Cited Authors
- Adelberger, EG; Austin, SM; Bahcall, JN; Balantekin, AB; Bogaert, G; Brown, LS; Buchmann, L; Cecil, FE; Champagne, AE; De Braeckeleer, L; Duba, CA; Elliott, SR; Freedman, SJ; Gai, M; Goldring, G; Gould, CR; Gruzinov, A; Haxton, WC; Heeger, KM; Henley, E; Johnson, CW; Kamionkowski, M; Kavanagh, RW; Koonin, SE; Kubodera, K; Langanke, K; Motobayashi, T; Pandharipande, V; Parker, P; Robertson, RGH; Rolfs, C; Sawyer, RF; Shaviv, N; Shoppa, TD; Snover, KA; Swanson, E; Tribble, RE; Turck-Chièze, S; Wilkerson, JF
Published Date
- January 1, 1998
Published In
Volume / Issue
- 70 / 4 PART II
Start / End Page
- 1265 - 1291
International Standard Serial Number (ISSN)
- 0034-6861
Digital Object Identifier (DOI)
- 10.1103/revmodphys.70.1265
Citation Source
- Scopus