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