Direct measurement of the 11C(α, p)14N stellar reaction at CRIB

Details Direct measurement of the 11C(α, p)14N stellar reaction at CRIB Direct measurement of the 11C(α, p)14N stellar reaction at CRIB

Aug 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1269..104h&link_type=abstract

THE 10TH INTERNATIONAL SYMPOSIUM ON ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: OMEG-2010. AIP Conference Proceedings, Volume 1

Physics

Nuclear Physics

1

Radioactive Ion Beams, Supernovae, Cyclotrons, Telescopes, Sources Of Radioactive Nuclei, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, Cyclotrons, Astronomical And Space-Research Instrumentation

Scientific paper

The first direct measurement of the 11C(α, p)14N reaction cross section of astrophysical interest has been performed for the center-of-mass energies from 1 to 4.5 MeV with the CRIB (Center for Nuclear Study Radioactive Ion Beam separator). We successfully distinguished the transition to the ground state of 14N and that to the second excited state with a comparable yield. The resonant shapes in the preliminary excitation function for the ground state transition have been confirmed to be consistent with the ones from the time-reversal reaction data of previous experiments.

Affiliated with

Also associated with

No associations

Rating

Direct measurement of the 11C(α, p)14N stellar reaction at CRIB 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 Direct measurement of the 11C(α, p)14N stellar reaction at CRIB, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct measurement of the 11C(α, p)14N stellar reaction at CRIB will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1862484