alpha-induced reactions on 115In: cross section measurements and statistical model analysis
arXiv:1805.07533 · doi:10.1103/PhysRevC.97.055803
Abstract
[Background] Alpha-nucleus optical potentials are basic ingredients of statistical model calculations used in nucleosynthesis simulations. While the nucleon+nucleus optical potential is fairly well known, for the alpha+nucleus optical potential several different parameter sets exist and large deviations, reaching sometimes even an order of magnitude, are found between the cross section predictions calculated using different parameter sets. [Purpose] A measurement of the radiative alpha-capture and the alpha-induced reaction cross sections on the nucleus 115In at low energies allows a stringent test of statistical model predictions. Since experimental data is scarce in this mass region, this measurement can be an important input to test the global applicability of alpha+nucleus optical model potentials and further ingredients of the statistical model. [Methods] The reaction cross sections were measured by means of the activation method. The produced activities were determined by off-line detection of the gamma-rays and characteristic x-rays emitted during the electron capture decay of the produced Sb isotopes. The 115In(alpha,gamma)119Sb and 115In(alpha,n)118Sbm reaction cross sections were measured between Ec.m. = 8.83 MeV - 15.58 MeV, and the 115In(alpha,n)118Sbg reaction was studied between Ec.m. = 11.10 MeV - 15.58 MeV. The theoretical analysis was performed within the statistical model.
References in corpus (46)
- Nucleosynthesis in Massive Stars With Improved Nuclear and Stellar Physics
- Astrophysical Reaction Rates From Statistical Model Calculations
- The s Process: Nuclear Physics, Stellar Models, Observations
- Neutrino-induced nucleosynthesis of A>64 nuclei: The nu p-process
- Neutrino Signal of Electron-Capture Supernovae from Core Collapse to Cooling
- Where, oh where has the r-process gone?
- Microscopic HFB+QRPA predictions of dipole strength for astrophysics applications
- Tables of Nuclear Cross Sections and Reaction Rates: an Addendum to the Paper "Astrophysical Reaction Rates from Statistical Model Calculations"
- Constraining the astrophysical origin of the p-nuclei through nuclear physics and meteoritic data
- Nucleosynthesis in Early Supernova Winds II: The Role of Neutrinos
- Production of Light Element Primary Process nuclei in neutrino-driven winds
- Charged-current weak interaction processes in hot and dense matter and its impact on the spectra of neutrinos emitted from proto-neutron star cooling
- The intermediate neutron-capture process and carbon-enhanced metal-poor stars
- Type Ia Supernovae as Sites of p-process: Two-Dimensional Models Coupled to Nucleosynthesis
- Sensitivity of p-Process Nucleosynthesis to Nuclear Reaction Rates in a 25 Solar Mass Supernova Model
- Further explorations of the alpha-particle optical model potential at low energies for the mass range A=45-209
- The Path to Improved Reaction Rates for Astrophysics
- Branchings in the gamma-process path revisited
- Sensitivity of astrophysical reaction rates to nuclear uncertainties
- Alpha-induced cross sections of 106Cd for the astrophysical p-process
- The ^{144}Sm-αoptical potential at astrophysically relevant energies derived from ^{144}Sm(α,α)^{144}Sm elastic scattering
- Odd p isotope 113In: Measurement of alpha-induced reactions
- Determination of 141Pr(alpha,n)144Pm cross sections at energies of relevance for the astrophysical p-process using the gamma-gamma coincidence method
- Elastic alpha scattering experiments and the alpha-nucleus optical potential at low energies
- Role of core-collapse supernovae in explaining Solar System abundances of p nuclides
- Impact of reactions on weak r-process in neutrino-driven winds
- Mo()Mo scattering,the Mo-- optical potential, and the Ru()Mo reaction rate at astrophysically relevant energies
- Uncertainties in the production of p nuclides in thermonuclear supernovae determined by Monte Carlo variations
- Cross section measurements of -induced reactions on Mo and Sn for -process studies
- Elastic alpha-scattering of 112Sn and 124Sn at astrophysically relevant energies
- Investigation of alpha-induced reactions on 130Ba and 132Ba and their importance for the synthesis of heavy p nuclei
- Investigation of alpha-induced reactions on the p nucleus 168Yb
- Nucleosynthesis of elements between Sr and Ag in neutron- and proton-rich neutrino-driven winds
- Total and partial cross sections of the Sn()Te reaction measured via in-beam -ray spectroscopy
- High precision In()In elastic scattering at energies around the Coulomb barrier for the astrophysical process
- High precision Y(,)Y scattering at low energies
- Role of (,n) reactions under -process conditions in neutrino-driven winds revisited
- Measurement of the 187Re(α,n)190Ir reaction cross section at sub-Coulomb energies using the Cologne Clover Counting Setup
- Total reaction cross sections from elastic alpha-nucleus scattering angular distributions around the Coulomb barrier
- Cd()Cd elastic scattering and systematic investigation of elastic scattering cross sections along the = 48 isotopic and = 62 isotonic chains
- Statistical model analysis of -induced reaction cross sections of Zn at low energies
- -scattering and -induced reaction cross sections of Zn at low energies
- Direct study of the alpha-nucleus optical potential at astrophysical energies using the 64Zn(p,alpha)61Cu reaction
- Measurement of (alpha,n) reaction cross sections of erbium isotopes for testing astrophysical rate predictions
- 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
Cited by in corpus (5)
- The activation method for cross section measurements in nuclear astrophysics
- Low Energy measurement of the reaction cross section and its impact on weak r-process nucleosynthesis
- Cross section of -induced reactions on Au at sub-Coulomb energies
- Role of consistent parameter sets in an assessment of the alpha-particle optical potential below the Coulomb barrier
- Cross sections at sub-Coulomb energies: full optical model vs.\ barrier transmission for Ca +