Stellar reaction rate of26Mg( p, γ)27Al

Details Stellar reaction rate of26Mg( p, γ)27Al Stellar reaction rate of26Mg( p, γ)27Al

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980zphya.296..273b&link_type=abstract

Zeitschrift für Physik A Atoms and Nuclei, Volume 296, Issue 3, pp.273-280

Astronomy and Astrophysics

Astrophysics

7

Scientific paper

The reaction26Mg( p, γ)27Al has been investigated at E p (lab)=80 355 keV. The existence of the resonances at E p =292 and 338 keV has been verified and new resonances were found at E p =227 and 275 keV. Information on branching and mixing ratios, ωγ values, total widths, and J π assignments for the observed resonances is given. Upper limits on the ωγ strengths for expected resonances in the energy range covered are presented. The astrophysical aspects of the data are discussed in the light of the26Mg(26Al) isotopic anomaly.

Affiliated with

Also associated with

No associations

Rating

Stellar reaction rate of26Mg( p, γ)27Al 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 Stellar reaction rate of26Mg( p, γ)27Al, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Stellar reaction rate of26Mg( p, γ)27Al will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-909737