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NSR database version of April 29, 2024.

Search: Author = E.V.Chimanski

Found 7 matches.

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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
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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
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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
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2021CH31      Eur.Phys.J. A 57, 212 (2021)

E.V.Chimanski, B.V.Carlson

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
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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
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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
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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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