Identification of Key Astrophysical Resonances Relevant for the Al26g(p,γ)Si27 Reaction in Wolf-Rayet Stars, AGB stars, and Classical Novae

Physics – Nuclear Physics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

10

Gamma Transitions And Level Energies, Binding Energies And Masses, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, 20<=A<=38

Scientific paper

A γ-ray spectroscopy study of Al26g+p resonant states in Si27 is presented. Excitation energies were measured with improved precision and first spin-parity assignments made for excited states in Si27 above the proton threshold. The results indicate the presence of low-lying resonances with lp=0 and lp=2 captures that could strongly influence the Al26g(p,γ)Si27 reaction rate at low stellar temperatures, found in low-mass asymptotic giant branch (AGB), intermediate-mass AGB, super AGB, and Wolf-Rayet stars.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Identification of Key Astrophysical Resonances Relevant for the Al26g(p,γ)Si27 Reaction in Wolf-Rayet Stars, AGB stars, and Classical Novae 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 Identification of Key Astrophysical Resonances Relevant for the Al26g(p,γ)Si27 Reaction in Wolf-Rayet Stars, AGB stars, and Classical Novae, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Identification of Key Astrophysical Resonances Relevant for the Al26g(p,γ)Si27 Reaction in Wolf-Rayet Stars, AGB stars, and Classical Novae will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1865269

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.