Statistical Hauser-Feshbach theory with width fluctuation correction including direct reaction channels for neutron induced reaction at low energies
arXiv:1604.08635 · doi:10.1103/PhysRevC.94.014612
Abstract
A model to calculate particle-induced reaction cross sections with statistical Hauser-Feshbach theory including direct reactions is given. The energy average of scattering matrix from the coupled-channels optical model is diagonalized by the transformation proposed by Engelbrecht and Weidenmüller. The ensemble average of -matrix elements in the diagonalized channel space is approximated by a model of Moldauer [Phys.Rev.C {\bf 12}, 744 (1975)] using newly parametrized channel degree-of-freedom to better describe the Gaussian Orthogonal Ensemble (GOE) reference calculations. Moldauer approximation is confirmed by a Monte Carlo study using randomly generated -matrix, as well as the GOE three-fold integration formula. The method proposed is applied to the U(n,n') cross section calculation in the fast energy range, showing an enhancement in the inelastic scattering cross sections.
Cited by in corpus (31)
- The Origin of r-Process Elements in the Milky Way
- Modeling Kilonova Light Curves: Dependence on Nuclear Inputs
- -delayed fission in -process nucleosynthesis
- Full Transport General Relativistic Radiation Magnetohydrodynamics for Nucleosynthesis in Collapsars
- Actinide Production in Neutron-Rich Ejecta of a Neutron Star Merger
- Neutron-gamma competition for -delayed neutron emission
- Nuclear masses learned from a probabilistic neural network
- Physically Interpretable Machine Learning for nuclear masses
- 129I and 247Cm in Meteorites Constrain the Last Astrophysical Source of Solar r-process Elements
- Estimation of M1 scissors mode strength for deformed nuclei in the medium to heavy mass region by statistical Hauser-Feshbach model calculations
- Actinide-rich and Actinide-poor -Process Enhanced Metal-Poor Stars do not Require Separate -Process Progenitors
- Nucleosynthesis and observation of the heaviest elements
- Gamma-rays from kilonova: a potential probe of r-process nucleosynthesis
- Propagation of Statistical Uncertainties of Skyrme Mass Models to Simulations of -Process Nucleosynthesis
- Co-production of light and heavy -process elements via fission deposition
- Reverse engineering nuclear properties from rare earth abundances in the process
- Actinide opacities for modeling the spectra and light curves of kilonovae
- Following nuclei through nucleosynthesis: a novel tracing technique
- The Influence of Beta Decay Rates on r-Process Observables
- The link between rare earth peak formation and the astrophysical site of the process
- Markov Chain Monte Carlo Predictions of Neutron-rich Lanthanide Properties as a Probe of -process Dynamics
- Nucleosynthesis in Outflows from Black Hole-Neutron Star Merger Disks With Full GRRMHD
- Distribution of Off-Diagonal Cross Sections in Quantum Chaotic Scattering: Exact Results and Data Comparison
- Unified description of the coupled-channels and statistical Hauser-Feshbach nuclear reaction theories for low energy neutron incident reactions
- Modeling photon--induced reactions on U actinide targets
- Sandblasting the -Process: Spallation of Ejecta from Neutron Star Mergers
- Angle-dependent in-situ fast flavor transformations in post-neutron star merger disks
- Cross sections of -induced reactions slightly below doubly-magic Ca from the statistical model
- Magnetic Field Strength Effects on Nucleosynthesis from Neutron Star Merger Outflows
- Deviations from the Porter-Thomas Distribution due to Nonstatistical Decay below the Nd Neutron Separation Threshold
- Nuclear data activities for medium mass and heavy nuclei at Los Alamos