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The 44Ti(alpha,p) reaction and its implication on the 44Ti yield in supernovae
1Argonne National Laboratory, 9700 South Cass Avenue, Argonne, Illinois 60439, USA.
Abstract:
Cross sections for the 44Ti(alpha,p)47V reaction which significantly affects the yield of 44Ti in supernovae were measured in the energy range 5.7 MeV=E(c.m.)=9 MeV, using a beam of radioactive 44Ti. The cross sections and the deduced astrophysical reaction rates are larger than the results from theoretical calculations by about a factor of 2. The implications of this increase in the reaction rate for the search of supernovae using space-based gamma detectors are discussed.
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