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Solar fusion cross sections

E. G. AdelbergerNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Sam M. AustinNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195John N. BahcallNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195A. B. BalantekinNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195G. BogaertNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Lowell S. BrownNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195L. BuchmannNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195F. Edward CecilNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Arthur E. ChampagneNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195L. De BraeckeleerNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Charles A. DubaNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195S. R. ElliottNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195S. J. FreedmanNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195M. GaiNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195G. GoldringNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195C. R. GouldNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Andrei GruzinovNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195W. C. HaxtonNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195K. M. HeegerNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Ernest M. HenleyNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Calvin W. JohnsonNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Marc KamionkowskiNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Ralph W. KavanaghNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195S. E. KooninNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195K. KuboderaNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195K. LangankeNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195T. MotobayashiNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195V. R. PandharipandeNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Peter D. ParkerNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195R. G. H. RobertsonNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195C. RolfsNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195R. F. SawyerNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Nir J. ShavivNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195T. D. ShoppaNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195K. A. SnoverNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Erik SwansonNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195Robert E. TribbleNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195S. Turck‐ChièzeNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195J. F. WilkersonNuclear Physics Laboratory, University of Washington, Seattle, Washington 98195
1998en
ABI

Abstract

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.

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Cited by 110 references
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