S factor of the 3H(3H,2n)4He and 3He(3He,2p)4He reactions using a three-cluster exit channel

Details S factor of the 3H(3H,2n)4He and 3He(3He,2p)4He reactions using a three-cluster exit channel S factor of the 3H(3H,2n)4He and 3He(3He,2p)4He reactions using a three-cluster exit channel

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001phrvc..63f4604v&link_type=abstract

Physical Review C, vol. 63, Issue 6, id. 064604

Astronomy and Astrophysics

Astrophysics

3

Nuclear Reaction Models And Methods, Cluster Models, Scattering Theory, Solar Neutrinos

Scientific paper

The reactions 3H(3H,2n)4He and 3He(3He,2p)4He are investigated within a fully microscopic cluster model featuring a three-cluster exit channel. A hyperspherical harmonics basis is used to describe the three-cluster continuum. The resulting astrophysical S factor of both reactions is in good agreement with experimental data. Analysis of the low-energy scattering parameters reveals no evidence for a hidden resonance state that would increase the cross section of the reactions, and would help to resolve the solar neutrino problem.

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