Mo-92(alpha,alpha)Mo-92 scattering, the Mo-92-alpha optical potential, and the Ru-96(gamma,alpha)Mo-92 reaction rate at astrophysically relevant energies
Fulop, Zs., Gyurky, Gy., Mate, Z., Somorjai, E., Zolnai, L., Galaviz, D., Babilon, M., Mohr, P., Zilges, A., Rauscher, T., Oberhummer, H. and Staudt, G.
(2001)
Mo-92(alpha,alpha)Mo-92 scattering, the Mo-92-alpha optical potential, and the Ru-96(gamma,alpha)Mo-92 reaction rate at astrophysically relevant energies.
Physical Review C (nuclear physics), 64 (6): 065805.
ISSN 2469-9985
The elastic scattering cross section of (MO)-M-92(alpha,alpha)Mo-92 has been measured at energies of E-c.m. approximate to 13, 16, and 19 MeV in a wide angular range. The real and imaginary parts of the optical potential for the system Mo-92-alpha have been derived at energies around and below the Coulomb barrier, The result fits into the systematic behavior of alpha -nucleus folding potentials. The astrophysically relevant Ru-96(gamma,alpha)Mo-92 reaction rates at, T-9 = 2.0 and T-9 = 3.0 could be determined to an accuracy of about 16% and are compared to previously published theoretical rates.
Item Type | Article |
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Keywords | gamma-process, isotopes, range, supernovae, nuclear astrophysics, cross-section, incident energies, p-process |
Date Deposited | 15 May 2025 12:36 |
Last Modified | 30 May 2025 23:54 |
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