The 14N(p,γ)15O reaction studied at high energy

Details The 14N(p,γ)15O reaction studied at high energy The 14N(p,γ)15O reaction studied at high energy

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1213..222m&link_type=abstract

FIFTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS. AIP Conference Proceedings, Volume 1213, pp. 222-224 (2010).

Other

Solar Neutrinos, Gamma-Ray Spectroscopy, Resonance Reactions And Scattering, Nuclear, Solar Neutrinos, X- And Gamma-Ray Spectroscopy, Other Resonances

Scientific paper

The 14N(p,γ)15O reaction is the bottleneck of the carbon-nitrogen-oxygen (CNO) cycle. Recent studies of this reaction have been performed in the low energy range E<500 keV. However, also data at higher energy are necessary to extrapolate the S-factor down to the energy range of astrophysical interest. Up to now, only one set of data from an experiment performed in 1987 extends up to 2.5 MeV. A new study has been carried out at the high-current FZD Tandetron in Dresden, in the energy region from 0.6 to 2.5 MeV. The astrophysics motivations, setup and on-going analysis are presented.

Affiliated with

Also associated with

No associations

Rating

The 14N(p,γ)15O reaction studied at high energy does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with The 14N(p,γ)15O reaction studied at high energy, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The 14N(p,γ)15O reaction studied at high energy will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1423199