Underground nuclear astrophysics and solar neutrinos

Details Underground nuclear astrophysics and solar neutrinos Underground nuclear astrophysics and solar neutrinos

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..853..358b&link_type=abstract

FUSION06: Reaction Mechanisms and Nuclear Structure at the Coulomb Barrier. AIP Conference Proceedings, Volume 853, pp. 358-365

Other

Solar Neutrinos, 3H-, 3He-, And 4He-Induced Reactions, Radiative Capture, Fusion Reactions, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments

Scientific paper

LUNA, Laboratory for Underground Nuclear Astrophysics at Gran Sasso, is studying thermonuclear reactions down to the energy of the nucleosynthesis inside stars. Significant results, relevant for neutrino physics, have been the measurements of the 3He(3He,2p)4He cross section within the Gamow peak of the Sun and of 14N(p,γ)15O down to very low energy. The results will be discussed together with the status of the running experiment on 3He(α, γ)7Be.

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