7 research outputs found
High energy solar neutrinos and p-wave contributions to ^3He(p,\nue^+)^4He
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 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.Comment: 4 pages, 1 ps figure, very minor changes, Phys. Rev. C in pres
Realistic Calculation of the hep Astrophysical Factor
The astrophysical factor for the proton weak capture on 3He is calculated
with correlated-hyperspherical-harmonics bound and continuum wave functions
corresponding to a realistic Hamiltonian consisting of the Argonne v18
two-nucleon and Urbana-IX three-nucleon interactions. The nuclear weak charge
and current operators have vector and axial-vector components, that include
one- and many-body terms. All possible multipole transitions connecting any of
the p-3He S- and P-wave channels to the 4He bound state are considered. The
S-factor at a p-3He center-of-mass energy of 10 keV, close to the Gamow-peak
energy, is predicted to be 10.1 10^{-20} keV b, a factor of five larger than
the standard-solar-model value. The P-wave transitions are found to be
important, contributing about 40 % of the calculated S-factor.Comment: 8 pages RevTex file, submitted to Phys. Rev. Let
Modern theories of low-energy astrophysical reactions
We summarize recent ab initio studies of low-energy electroweak reactions of
astrophysical interest, relevant for both big bang nucleosynthesis and solar
neutrino production. The calculational methods include direct integration for
np radiative and pp weak capture, correlated hyperspherical harmonics for
reactions of A=3,4 nuclei, and variational Monte Carlo for A=6,7 nuclei.
Realistic nucleon-nucleon and three-nucleon interactions and consistent current
operators are used as input.Comment: 29 pages, 4 figure
Exchange currents in low-energy nucleon capture by 3He
Electrical Engineering, Mathematics and Computer Scienc