Nuclear Aspects of the Solar Neutrino Problem |
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| Authors: | H Oberhummer AN Ivanov NI Troitskaya M Faber |
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| Institution: | 1. InterTrust Technologies Corp., 460 Oakmead Parkway, Sunnyvale, CA, 94086, USA
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| Abstract: | The present status of the nuclear reaction rates determining the solar neutrino flux is discussed. This includes the reaction
rates for the two branching ratios of the three pp-chains involving the reactions 3He(3He,2p)4He and 3He(4He,γ)7Be for the
first branching, and 7Be(e−, νe)7Li and 7Be(p, γ)8B for the second branching. Mainly we will concentrate on the basic nuclear
reaction p + p → D + e+ + νe of the pp-chains. This reaction rate can only be determined using the theoretical methods. The
present status of the application of the relativistic field theory model of the deuteron for this reaction will be discussed.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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