The Si28(p,t)Si26*(p) reaction and implications for the astrophysical Al25(p,γ)Si26 reaction rate

Details The Si28(p,t)Si26*(p) reaction and implications for the astrophysical Al25(p,γ)Si26 reaction rate The Si28(p,t)Si26*(p) reaction and implications for the astrophysical Al25(p,γ)Si26 reaction rate

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010phrvc..82d5803c&link_type=abstract

Physical Review C, vol. 82, Issue 4, id. 045803

Physics

Nuclear Physics

3

Transfer Reactions, Nuclear Physics Aspects Of Novae, Supernovae, And Other Explosive Environments, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 20<=A<=38

Scientific paper

Several resonances in Al25(p,γ)Si26 have been studied via the Si28(p,t)Si26 reaction. Triton energies and angular distributions were measured using a segmented annular detector array. An additional silicon detector array was used to simultaneously detect the coincident protons emitted from the decay of states in Si26 above the proton threshold in order to determine branching ratios. A resonance at 5927±4 keV has been experimentally confirmed as the first ℓ=0 state above the proton threshold, with a proton branching ratio consistent with one.

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