Recent results at LUNA, using a solid target

Details Recent results at LUNA, using a solid target Recent results at LUNA, using a solid target

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aipc..831..466i&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS - FINUSTAR. AIP Conference Proceedings, Volume 831, pp. 466-468 (20

Astronomy and Astrophysics

Astrophysics

Radiative Capture, Spectroscopic Factors And Asymptotic Normalization Coefficients, 6<=A<=19, Solar Neutrinos

Scientific paper

The determination of the astrophysical S-factor of the 14N(p,γ)15O reaction is of great interest because this reaction represents the bottleneck of the CNO cycle, which in turn has a large influence on the determination of the age of globular clusters and also plays a role in the estimation of the Solar neutrino fluxes. We have performed a new underground measurement (LUNA, Gran Sasso Laboratory, Italy) using a high resolution set-up, extending the investigated energy range down to Ecm=130 keV. This allowed a more reliable extrapolation to astrophysical energies, using an R-matrix fit to the decay to different final states in 15O.

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