Breakout from the hot CNO cycle via the 18Ne(α,p)21Na reaction

Details Breakout from the hot CNO cycle via the 18Ne(α,p)21Na reaction Breakout from the hot CNO cycle via the 18Ne(α,p)21Na reaction

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999phrvc..59.3402b&link_type=abstract

Physical Review C (Nuclear Physics), Volume 59, Issue 6, June 1999, pp.3402-3409

Physics

Nuclear Physics

25

Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Transfer Reactions, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, 20<=A<=38

Scientific paper

The reaction 18Ne(α,p)21Na, of importance to nuclear astrophysics, has been studied directly using the postaccelerated radioactive 18Ne beam available at Louvain-la-Neuve and a gaseous helium target. This study covered the energy region from 2.04 to 3.01 MeV in the center of mass, and identified various levels in the compound nucleus 22Mg. The stellar reaction rate due to these states has been deduced. The experimental rate shows good agreement with theoretical predictions [J. Görres, M. Wiescher, and F. K. Thielemann, Phys. Rev. C 51, 392 (1995)] above 2.5 GK.

Affiliated with

Also associated with

No associations

Rating

Breakout from the hot CNO cycle via the 18Ne(α,p)21Na reaction 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 Breakout from the hot CNO cycle via the 18Ne(α,p)21Na reaction, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Breakout from the hot CNO cycle via the 18Ne(α,p)21Na reaction will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1801269