Steven Karataglidis

Extrapolation of the astrophysicalSfactor for7Be(p,γ)8Bto solar energies

We investigate the energy dependence of the astrophysical

Low-energy M1 strength in the Li-7(p,gamma_0)Be-8 reaction

S

Low-energy M1 strength in the

factor for the reaction

^7Li (p, \gamma_0) ^8Be

^7

reaction

Be

Shell model structures of low-lying excited states in {sup 6,7}Li

(p,\gamma)^8

Microscopic model analyses of select scattering of 135 MeV protons from {sup 12}C

B, the primary source of high-energy solar neutrinos in the solar

Predictions of the scattering of 200 and 300 MeV polarized protons from polarized3He

pp

Large basis shell model analysis of {sup 14}N({gamma},{pi}{sup +}){sup 14}C{sub g.s.} reaction

chain. Using simple models we explore the model dependence in the extrapolation of the experimental data to the region of astrophysical interest near 20 keV. We find that below approximately 400 keV the energy dependence is very well understood and constrained by the data for the elastic scattering of low energy neutrons from

Seff and the 7Be(p,?)8B reaction

^7