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Study of the 3H(3H,2n)4He and 3H(3He,2p)4He reactions in the frameworks of three-cluster microscopic model
V. S. Vasilevsky1, A. B. Nesterov1, F. Arickx2, J. Broeckhove2
1Bogolyubov Institute for Theoretical Physics of the National Academy of Sciences of Ukraine, Kyiv, Ukraine
2University of Antwerp, Antwerp, Belgium
Abstract: 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 would increase the cross-section of the reactions, and would help to resolve the solar neutrino problem.
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