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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

机译:mo-92(α,α)mo-92散射,mo-92-α光学势和Ru-96(γ,α)mo-92在天体物理相关能量下的反应速率

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摘要

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.
机译:(MO)-M-92ααMo-92的弹性散射截面是在E-c.m的能量下测量的。在宽角度范围内大约为13 MeV,13 MeV和19 MeV。 Mo-92-α系统的光势的实部和虚部是在库仑势垒附近和下方的能量处得出的,其结果适合于α核折叠势的系统行为。可以确定在T-9 = 2.0和T-9 = 3.0时与天体相关的Ru-96(γ,α)Mo-92反应速率,其准确度约为16,并与先前发表的理论速率进行了比较。

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