The 40Ca(alpha,gamma)44Ti reaction in the energy regime of supernova nucleosynthesis
arXiv:nucl-ex/0509006 · doi:10.1103/PhysRevLett.96.041102
Abstract
The 44Ti(t1/2 = 59 y) nuclide, an important signature of supernova nucleosynthesis, has recently been observed as live radioactivity by gamma-ray astronomy from the Cas A remnant. We investigate in the laboratory the major 44Ti production reaction, 40Ca(alpha,gamma)44Ti (E_cm = 0.6-1.2 MeV/u), by direct off- line counting of 44Ti nuclei. The yield, significantly higher than inferred from previous experiments, is analyzed in terms of a statistical model using microscopic nuclear inputs. The associated stellar rate has important astrophysical consequences, increasing the calculated supernova 44Ti yield by a factor ~2 over previous estimates and bringing it closer to Cas A observations.
To be published in Phys. Rev. lett., 4 pages, 1 table, 2 figures
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- Cross sections of -induced reactions for targets with masses at low energies
- The resonance triplet at E_alpha = 4.5 MeV in the 40Ca(alpha,gamma)44Ti reaction
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- Measurement of the stellar NiNi cross section with AMS
- Alpha-decay from Ti: A study of the microscopic clusterization
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