First result of the cross sectional measurement of 3He-3He solar reaction in OCEAN

Details First result of the cross sectional measurement of 3He-3He solar reaction in OCEAN First result of the cross sectional measurement of 3He-3He solar reaction in OCEAN

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..561..127i&link_type=abstract

TOURS SYMPOSIUM ON NUCLEAR PHYSICS IV: TOURS 2000. AIP Conference Proceedings, Volume 561, pp. 127-136 (2001).

Physics

Nuclear Physics

2

Hydrostatic Stellar Nucleosynthesis, Transfer Reactions, A<=5, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

The first result in OCEAN measurement of the fusion reactions 3He(3He,2p)α at the energy of 40 to 50 keV by means of a low-energy, high current accelerator are reported. The accelerator in this facility can produce an intense beam of 3He1+ and 3He2+ ions of more than 1mA. A detection efficiency for proposed detector assembly of ΔE-E counter telescope is simulated with GEANT program and it expects a detection efficiency about 10% for the two proton coincidence for 3He+3He-->2p+α reaction. The accuracy of Monte Carlo program was checked by D(3He,p)α reaction by replacing the target gas to deuterium. .

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