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.
References in corpus (8)
- The r-process of stellar nucleosynthesis: Astrophysics and nuclear physics achievements and mysteries
- Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model
- Alpha-induced cross sections of 106Cd for the astrophysical p-process
- Odd p isotope 113In: Measurement of alpha-induced reactions
- Large-scale prediction of the parity distribution in the nuclear level density and application to astrophysical reaction rates
- Alpha-induced reaction cross section measurements on 151Eu for the astrophysical gamma-process
- Photon-induced Nucleosynthesis: Current Problems and Experimental Approaches
- Astrophysical relevance of transition energies
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- Experimental study of the astrophysical gamma-process reaction 124Xe(alpha,gamma)128Ba
- The 106Cd(alpha,alpha)106Cd elastic scattering in a wide energy range for gamma-process studies
- Unexpected properties of the S(,p)Cl reaction cross section at low energies
- Cross sections at sub-Coulomb energies: full optical model vs.\ barrier transmission for Ca +