NSR Query Results
Output year order : Descending NSR database version of April 29, 2024. Search: Author = E.V.Chimanski Found 7 matches. 2023CH56 Particles 6, 198 (2023) E.V.Chimanski, R.V.Lobato, A.R.Goncalves, C.A.Bertulani Bayesian Exploration of Phenomenological EoS of Neutron/Hybrid Stars with Recent Observations
doi: 10.3390/particles6010011
2023HU24 Nucl.Instrum.Methods Phys.Res. A1057, 168715 (2023) A.M.Hurst, R.B.Firestone, E.V.Chimanski pyEGAF: An open-source Python library for the Evaluated Gamma-ray Activation File COMPILATION 29Si, 56Fe, 73Ge, 75As, 87Rb, 104Ru, 113In, 151Eu, 164Dy, 167Er, 170Yb, 176Lu, 181Ta, 184W, 187Re; compiled γ-ray energies and intensities. Comparison with available data.
doi: 10.1016/j.nima.2023.168715
2022LO16 J.Phys.:Conf.Ser. 2340, 012014 (2022) R.V.Lobato, E.V.Chimanski, C.A.Bertulani Cluster Structures with Machine Learning Support in Neutron Star M-R relations
doi: 10.1088/1742-6596/2340/1/012014
2021CH31 Eur.Phys.J. A 57, 212 (2021) Nucleon-induced inelastic scattering with statistical strength functions and the ECIS direct reaction code NUCLEAR REACTIONS 90Zr(p, p), E=80 MeV; calculated σ, σ(θ, E) using DWBA reaction calculations using the ECIS code. Comparison with available data.
doi: 10.1140/epja/s10050-021-00497-6
2021CH69 Braz.J.Phys. 51, 323 (2021) E.V.Chimanski, L.A.Souza, B.V.Carlson The Sao Paulo Potential and the 3He Breakup Reaction at 130 MeV on 93Nb and 197Au NUCLEAR REACTIONS 93Nb, 197Au(3He, X), (3He, d), E=130 MeV; calculated σ(θ, E); deduced Sao Paulo potential parameters adjusted for the nuclear diffusivity.
doi: 10.1007/s13538-020-00819-x
2021SO26 Phys.Rev. C 104, 034623 (2021) L.A.Souza, E.V.Chimanski, B.V.Carlson Inclusive breakup cross sections in reactions induced by the nuclides 6He and 6, 7Li in the two-body cluster model NUCLEAR REACTIONS 64Zn, 209Bi(6He, α), E=9-25 MeV; 64Zn(6He, α), E=9.8, 13.5, 14.85, 17.9 MeV; 120Sn(6He, α), E=17.4, 18.05, 19.8, 20.5, 22.2 MeV; 208Pb(6Li, α), (6Li, d), E=19-40 MeV; 90Zr(6Li, α), E=14-31, 19, 21, 25, 30 MeV; 58Ni(6Li, α), E=14, 16, 18, 20 MeV; 118Sn(6Li, α), E=18, 19, 21, 24 MeV; 56Fe(7Li, α), E=68 MeV; 58Ni(7Li, α), E=14.22, 16.25, 18.28, 20.31 MeV; calculated inclusive σ(E) for α and deuteron emission, α angular distributions, and spectra; deduce zero-range overall large contribution from inclusive breakup emission of α particles. Zero-range post-form Ichimura, Austern, and Vincent (IAV)-distorted-wave Born approximation (DWBA) formalism for elastic and nonelastic breakup cross sections, with Wood-Saxon parametrization of Sao Paulo optical potential with a modified diffuseness, and with projectiles treated as two-body clusters, 6He as α+dineutron, 6Li as α+d and 7Li as α+triton. Comparison with experimental data.
doi: 10.1103/PhysRevC.104.034623
2019CH01 Phys.Rev. C 99, 014305 (2019) E.V.Chimanski, B.V.Carlson, R.Capote, A.J.Koning Quasiparticle nature of excited states in random-phase approximation NUCLEAR STRUCTURE 56Ni; calculated level energy deviation, state strength function and width as function of excitation energy, contributions to the RPA transition matrix from collective, two-noncollective, and 3- states, response functions for low-energy 3-, and high energy particle-hole configurations of 3- states, single-particle contribution to the response function, width of the Breit-Wigner distribution for 3- and 4+ states, energy level spacing with local widths of particle-hole pair configurations. 16O, 56Ni, 90Zr, 120Sn; calculated spreading width of Breit Wigner distributions. Random phase approximation (RPA) on the basis of particle-hole configurations of excited states. Relevance to multistep direct (MSD) nuclear reactions.
doi: 10.1103/PhysRevC.99.014305
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