NSR Query Results
Output year order : Descending NSR database version of May 3, 2024. Search: Author = S.K.Biswal Found 13 matches. 2021BI05 Can.J.Phys. 99, 312 (2021) S.K.Biswal, S.K.Singh, M.Bhuyan, R.N.Panda, S.K.Patra A bridge between finite and infinite nuclear matter NUCLEAR STRUCTURE 40P, 40S, 40Ca, 112,116,120,124Sn, 208Pb; calculated binding energies from nuclear matter equation of state (EOS). Comparison with available data.
doi: 10.1139/cjp-2020-0104
2020BI13 Nucl.Phys. A1004, 122042 (2020) S.K.Biswal, M.K.Abu El Sheikh, N.Biswal, N.Yusof, H.A.Kassim, S.K.Patra, M.Bhuyan Nuclear matter properties of finite nuclei using relativistic mean field formalism NUCLEAR STRUCTURE N=20, 40, 82, 126; analyzed available data; calculated variation of the symmetry energy with density in the symmetric nuclear matter, symmetry energy for N = 20, 40, 82, 126, and 172 (predicted) isotonic chains as a function of neutron skin-thickness as calculated using the RMF model.
doi: 10.1016/j.nuclphysa.2020.122042
2020LO04 Eur.Phys.J. A 56, 32 (2020) O.Lourenco, M.Dutra, C.H.Lenzi, S.K.Biswal, M.Bhuyan, D.P.Menezes Consistent Skyrme parametrizations constrained by GW170817
doi: 10.1140/epja/s10050-020-00040-z
2020ZH08 Phys.Rev. C 101, 034303 (2020) Y.Zhang, M.Liu, C.-J.Xia, Z.Li, S.K.Biswal Constraints on the symmetry energy and its associated parameters from nuclei to neutron stars NUCLEAR REACTIONS 112,124Sn(124Sn, X), (112Sn, X), E=35, 50 MeV/nucleon; analyzed symmetry energy and related set of 22 nuclear matter parameters by comparing the isospin diffusion data to transport model calculations in five-dimensional parameter space. 208Pb; calculated neutron skin of 208Pb using the deduced nuclear matter parameter set and the restricted density variational (RDV) method. Calculated properties of a neutron star, such as the tidal deformability and maximum mass, and compared with the current constraints.
doi: 10.1103/PhysRevC.101.034303
2017KU01 Phys.Rev. C 95, 015801 (2017) B.Kumar, S.K.Biswal, S.K.Patra Tidal deformability of neutron and hyperon stars within relativistic mean field equations of state
doi: 10.1103/PhysRevC.95.015801
2016IK02 Int.J.Mod.Phys. E25, 1650103 (2016) M.Ikram, Asloob A.A.Rather, B.Kumar, S.K.Biswal, S.K.Patra Quest for magicity in hypernuclei NUCLEAR STRUCTURE 16,17O, 40,41,48,49Ca, 56,57Ni, 90,91Zr, 124,125,132,133Sn, 208,209Pb, 292,293,304,305,378,379120; calculated binding energies, charge and matter radii, separation energy for hypernuclei; deduced magic numbers.
doi: 10.1142/S0218301316501032
2016KU04 Int.J.Mod.Phys. E25, 1650020 (2016) B.Kumar, S.K.Biswal, S.K.Singh, C.Lahiri, S.K.Patra Modes of decay in neutron-rich nuclei NUCLEAR STRUCTURE 208Pb, 232,234,236,238,240,254,256,258Th, 230,232,234,236,248,250,252,254,256U; calculated matter density distributions. RADIOACTIVITY 216,232,254Th, 218,238,256U(α); calculated penetrability parameter using WKB approximation, T1/2. Comparison with available data.
doi: 10.1142/S0218301316500208
2016LA05 Int.J.Mod.Phys. E25, 1650015 (2016) C.Lahiri, S.K.Biswal, S.K.Patra Effects of NN potentials on p Nuclides in the A ∼ 100-120 region NUCLEAR STRUCTURE A = 100-120; calculated S-factors, astrophysical reaction rates using microscopical optical model potential with the Hauser-Feshbach reaction code TALYS. Comparison with experimental data.
doi: 10.1142/S0218301316500154
2015IK01 Int.J.Mod.Phys. E24, 1550019 (2015) M.Ikram, S.K.Singh, S.K.Biswal, S.K.Patra Effects of isovector scalar δ-meson on Λ-hypernuclei NUCLEAR STRUCTURE 6H, 7,8He, 7Li, 9Be, 10B, 16N, 16O, 28Si, 32S, 40Ca, 51V, 89Y, 139La, 208Pb; calculated hypernuclei binding energies, rms radii, orbitals, spin-orbit potentials. Comparison with available data.
doi: 10.1142/S0218301315500196
2015KU28 Phys.Rev. C 92, 054314 (2015) B.Kumar, S.K.Biswal, S.K.Singh, S.K.Patra Examining the stability of thermally fissile Th and U isotopes NUCLEAR STRUCTURE 216,218,220,222,224,226,228,230,232,234,236,238U, 216,218,220,222,224,226,228,230,232,234,236,238,240Th; calculated binding energies, charge radii, quadrupole deformation parameter β2, potential energy surfaces. Relativistic mean-field theory (RMF) with axially deformed basis. Pairing correlations. Comparison with finite-range droplet model (FRDM) calculations, and with available experimental values. 232Th, 236U; calculated single-particle energy levels as function of quadrupole deformation parameter. RADIOACTIVITY 222,224,226,228,230,232,234,236,238,240,242U, 216,218,220,222,224,226,228,230,232,234,236,238Th(α); calculated Q(α) and half-lives. 244,246,248,250,252,254,256,258,260,262,264,266,268,270Th, 240,242,244,246,248,250,252,254,256,258,260,262,264,266,268U(β-); calculated half-lives. 228,230,232,234Th, 232,234,236,238,240Th(SF); calculated fission barriers. Relativistic mean-field (RMF) theory. Comparison with other theoretical calculations, and with available experimental values.
doi: 10.1103/PhysRevC.92.054314
2014BI06 Int.J.Mod.Phys. E23, 1450017 (2014) S.K.Biswal, M.Bhuyan, S.K.Singh, S.K.Patra Search of double shell closure in the superheavy nuclei using a simple effective interaction NUCLEAR STRUCTURE 258Md, 258,261Rf, 259,260Db, 260,261Sg, 264,265Hs, 269Ds, 285,286,287,288,289Fl, 208Pb, 298Fl, 304120, 310126; calculated binding energies, ground state densities, two-neutron separation energies, pairing gap, single particle energy levels. Simple effective interaction, comparison with available data.
doi: 10.1142/S0218301314500177
2014SA19 Phys.Rev. C 89, 034614 (2014) B.B.Sahu, S.K.Singh, M.Bhuyan, S.K.Biswal, S.K.Patra Importance of nonlinearity in the NN potential NUCLEAR STRUCTURE 20Ne, 38Ar, 66Zn, 90Zr, 105Sb, 112Cs, 114Cd, 144Sm, 147Tm, 198Hg, 238U; calculated ground state binding energies, charge radii, and quadrupole deformation parameter using SH, L1 and NL3 interactions, and compared with experimental data. 16O, 208Pb, 270Ds; calculated binding energy from different fields of RMF Hamiltonian density with NL3 force, and compared with experimental data. RADIOACTIVITY 105Sb, 109I, 112,113Cs, 117La, 131Eu, 140,141Ho, 145,146,147Tm(p); calculated half-lives of proton emitters. Relativistic mean field theory (RMFT) with nonlinear self-coupling of the scalar meson field using NR3Y+EX, M3Y+EX and LR3Y+EX nucleon-nucleon interactions. Comparison with experimental data.
doi: 10.1103/PhysRevC.89.034614
2014SI10 Phys.Rev. C 89, 044001 (2014) S.K.Singh, S.K.Biswal, M.Bhuyan, S.K.Patra Effects of δ mesons in relativistic mean field theory
doi: 10.1103/PhysRevC.89.044001
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