Extrapolation of α+ carbon reaction cross sections to astrophysical energies

Details Extrapolation of α+ carbon reaction cross sections to astrophysical energies Extrapolation of α+ carbon reaction cross sections to astrophysical energies

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997nupha.621..177h&link_type=abstract

Nuclear Physics A, v. 621, p. 177-180.

Physics

Nuclear Physics

17

Scientific paper

R-matrix extrapolations that take into account the effects of subthreshold levels are reported for the α+12,13C reaction cross sections. The relatively low extrapolated value SE1(300 keV) = 20 keV-b for α+12C capture seems compatible with measurements of the β-delayed α-decay spectrum of 16N, while the extrapolated 13C(α, n)16O S-factor is found to be nearly two orders of magnitude larger than the Caughlan-Fowler value.

Affiliated with

Also associated with

No associations

Rating

Extrapolation of α+ carbon reaction cross sections to 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 Extrapolation of α+ carbon reaction cross sections to astrophysical energies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extrapolation of α+ carbon reaction cross sections to astrophysical energies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1606798