Investigation of alpha-induced reactions on 127I for the astrophysical gamma process
arXiv:1209.1238 · doi:10.1103/PhysRevC.86.035801
Abstract
(Shorten version of the PRC abstract) Alpha-induced reactions on 127I have been studied using the activation technique in order to provide cross section data for the modeling of the astrophysical gamma process. The relative intensity of the 536.1 keV gamma transition was measured precisely, its uncertainty was reduced from 13% to 4%. By measuring the yield of the characteristic X-rays, the cross sections of the 127I(alpha,gamma)131Cs reaction have been determined for the first time close to the astrophysically relevant energy region, at energies 9.50 < Ec.m. < 15.15Cs and its reverse reaction are factors 4-10 faster than previous calculations, due to improvements in the reaction model.
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- Measurements of Gd(p,)Tb and Gd(p,n)Tb reaction cross sections for the astrophysical process
- Test of statistical model cross section calculations for -induced reactions on Ag at energies of astrophysical interest
- Cross section of -induced reactions on iridium isotopes obtained from thick target yield measurement for the astrophysical process
- Experimental study of the astrophysical gamma-process reaction 124Xe(alpha,gamma)128Ba
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- The 106Cd(alpha,alpha)106Cd elastic scattering in a wide energy range for gamma-process studies
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- An ERC Starting Grant project on p-process nucleosynthesis concluded