Study of the ^56Ni(d,p)^57Ni Reaction and the Astrophysical ^56Ni(p,γ)^57Cu Reaction Rate.

Details Study of the ^56Ni(d,p)^57Ni Reaction and the Astrophysical ^56Ni(p,γ)^57Cu Reaction Rate. Study of the ^56Ni(d,p)^57Ni Reaction and the Astrophysical ^56Ni(p,γ)^57Cu Reaction Rate.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aps..dnp..bc02r&link_type=abstract

American Physical Society, Division of Nuclear Physics Meeting, October 5-8, 1997, abstract #BC.02

Physics

Nuclear Physics

Scientific paper

Beams of doubly-magic ^56Ni(T_1/2=6.1d) ions have been produced for the first time at ATLAS with the two-accelerator method. Using a high-efficiency Si detector array and the Fragment Mass Analyzer for particle identification, angular distributions for the inverse (d,p) reaction d(^56Ni,p)^57Ni have been measured. Spectroscopic factors for low-lying single-particle(?) states in ^57Ni have been obtained. With these spectropic factors, the yield for the ^56Ni(p,γ) reaction to the mirror nucleus ^57Cu has been calculated. The astrophysical rate for this reaction is found to be more than 10 times higher than previously assumed. Information on the d(^56Co,p)^57Co was obtained from the same measurement. This work was supported by the US Department of Energy, Nuclear Physics Division, under contract W-31-109-ENG-38 and by the NSF.

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