Absolute cross section of the 12C(p,γ)13N reaction
Published: September 2023 Wiescher
Solar neutrino measurements have reached a level of sensitivity such that CNO fluxes can now be experimentally determined. While these first measurements are only sensitive to higher energy neutrinos from the β+decays of 15O produced by the 14N(p,γ)15O reaction, future measurements will detect neutrinos from the β+decay of 13N from the 12C(p,γ)13N reaction. This paper reports on a recent measurement of the 12C(p,γ)13N reaction covering the laboratory energy range between 1.0 and 2.5 MeV. Learn more
Publication: Absolute cross section of the 12C(p,γ)13N reaction