First measurement of the 18O(p,α)15N cross section at astrophysical energies

Details First measurement of the 18O(p,α)15N cross section at astrophysical energies First measurement of the 18O(p,α)15N cross section at astrophysical energies

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010jphcs.202a2019l&link_type=abstract

Journal of Physics: Conference Series, Volume 202, Issue 1, pp. 012019 (2010).

Physics

Scientific paper

The 18O(p,α)15N reaction rate has been deduced by means of the Trojan horse method. For the first time the contribution of the 20 keV resonance has been directly evaluated, giving a value about 35% larger than the one in the literature. Moreover, the present approach has allowed to improve the accuracy by a factor 8.5, as it is based on the measured strength instead of spectroscopic measurements. The contribution of the 90 keV resonance has been also determined, which turned out to be of negligible importance to astrophysics.

Affiliated with

Also associated with

No associations

Rating

First measurement of the 18O(p,α)15N cross section at astrophysical energies 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 First measurement of the 18O(p,α)15N cross section at astrophysical energies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and First measurement of the 18O(p,α)15N cross section at astrophysical energies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1600670