Physics – Nuclear Physics – Nuclear Theory
Scientific paper
1999-05-18
Phys.Rev. C60 (1999) 022801
Physics
Nuclear Physics
Nuclear Theory
4 pages, 1 ps figure, very minor changes, Phys. Rev. C in press
Scientific paper
10.1103/PhysRevC.60.022801
High energy solar neutrinos can come from the hep reaction ^3He(p,\nue^+)^4He with a large end point energy of 18.8 MeV. Understanding the hep reaction may be important for interpreting solar neutrino spectra. We calculate the contribution of the axial charge transition $^3P_0\to ^1S_0$ to the hep thermonuclear S factor using a one-body reaction model involving a nucleon moving in optical potentials. Our result is comparable to or larger than previous calculations of the s-wave Gamow Teller contribution. This indicates that the hep reaction may have p-wave strength leading to an enhancement of the S factor.
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