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

Jan 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998phrvl..80..676r&link_type=abstract

Physical Review Letters, Volume 80, Issue 4, January 26, 1998, pp.676-679

Astronomy and Astrophysics

Astrophysics

34

Scientific paper

The single-particle character of states outside the doubly magic (radioactive) nucleus 56Ni has been determined through a measurement of the \(d,p\) neutron transfer reaction using inverse kinematics. From the spectroscopic factors of the low-lying states in 57Ni, the astrophysically interesting yield for the 56Ni\(p,γ\) reaction to the mirror nucleus 57Cu has been calculated, utilizing charge symmetry. The rate for this reaction in the temperature range typical of novae, supernovae, and x-ray bursts is found to be more than 10 times higher than previously assumed.

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