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Title: Solar Neutrino Fluxes Using The Exponential S-Factor

Journal Article · · AIP Conference Proceedings
DOI:https://doi.org/10.1063/1.2234442· OSTI ID:20877459
; ;  [1]
  1. Department of Physics, University of Malaya, 50603 Kuala Lumpur (Malaysia)

Recently we propose an exponential form for the astrophysical S-factor. This form produces about 20% more solar 3He production through the 3He-3He reaction. In this note, we investigate the effects on the 7Be and 8B neutrino productions since the neutrino fluxes depend on the 3He abundance.

OSTI ID:
20877459
Journal Information:
AIP Conference Proceedings, Vol. 847, Issue 1; Conference: International symposium on origin of matter and evolution of galaxies 2005: New horizon of nuclear astrophysics and cosmology, Tokyo (Japan), 8-11 Nov 2005; Other Information: DOI: 10.1063/1.2234442; (c) 2006 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
Country of Publication:
United States
Language:
English

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