NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = A.Quddus Found 9 matches. 2021SI01 Nucl.Phys. A1006, 122080 (2021) T.A.Siddiqui, A.Quddus, S.Ahmad, S.K.Patra Microscopic description of structural, surface, and decay properties of Z=124, 126 superheavy nuclei NUCLEAR STRUCTURE 284,285,286,287,288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329,330,331,332,333,334,335,336,337,338,339,340,341,342,343,344124, 288,289,290,291,292,293,294,295,296,297,298,299,300,301,302,303,304,305,306,307,308,309,310,311,312,313,314,315,316,317,318,319,320,321,322,323,324,325,326,327,328,329,330,331,332,333,334,335,336,337,338,339,340,341,342,343,344126; calculated binding energies, deformation parameters, charge and matter radii within the frame-work of covariant density functional theory (CDFT).
doi: 10.1016/j.nuclphysa.2020.122080
2020KA28 Nucl.Phys. A1000, 121871 (2020) M.Kaur, A.Quddus, A.Kumar, M.Bhuyan, S.K.Patra Effect of temperature on the volume and surface contributions in the symmetry energy of rare earth nuclei
doi: 10.1016/j.nuclphysa.2020.121871
2020KA50 J.Phys.(London) G47, 105102 (2020) M.Kaur, A.Quddus, A.Kumar, M.Bhuyan, S.K.Patra On the symmetry energy and deformed magic number at N = 100 in rare earth nuclei NUCLEAR STRUCTURE 160Nd, 162Sm, 164Gd, 166Dy; calculated ground state neutron single particle spectra, variation of nuclear symmetry energy within the coherent density fluctuation model with relativistic mean densities with NL3 and IOPB-I parameter sets.
doi: 10.1088/1361-6471/ab92e4
2020QU04 J.Phys.(London) G47, 045105 (2020) Effective surface properties of light, heavy, and superheavy nuclei NUCLEAR STRUCTURE 16,28O, 40,48Ca, 68Ni, 90Zr, 100,132Sn, 208Pb; calculated binding energy per particle, charge radius. Comparison with available data.
doi: 10.1088/1361-6471/ab4f3e
2020SI21 J.Phys.(London) G47, 115103 (2020) T.A.Siddiqui, A.Quddus, S.Ahmad, S.K.Patra A search for neutron magicity in the isotopic series of Z = 122, 128 superheavy nuclei NUCLEAR STRUCTURE N=158-218; analyzed available data; calculated neutron pairing energy, two-neutron-separation energy, single-particle energy levels, total shell-correction energy using density-dependent meson-exchange (DD-ME) and point-coupling (DD-PC) models within the framework of covariant density functional theory (CDFT); deduced N=168, 174, 178 as deformed neutron-magic numbers.
doi: 10.1088/1361-6471/ab8914
2019QU02 Phys.Rev. C 99, 044314 (2019) A.Quddus, M.Bhuyan, S.Ahmad, B.V.Carlson, S.K.Patra Temperature-dependent symmetry energy of neutron-rich thermally fissile nuclei NUCLEAR STRUCTURE 234,236,250U, 240Pu; calculated nuclear densities, effective symmetry energy coefficients and curvatures, binding energies, charge radius, and β deformation parameter at finite temperature, neutron pressure and symmetry energy coefficients as function of neutron skin thickness using temperature-dependent relativistic mean field model (TRMF) with FSUGarnet, IOPB-I, and NL3 parameters. Comparison with available experimental data.
doi: 10.1103/PhysRevC.99.044314
2019QU03 Nucl.Phys. A987, 222 (2019) A.Quddus, K.C.Naik, R.N.Panda, S.K.Patra Temperature dependent study of neutron-rich thermally fissile 244-262Th and 246-264U nuclei within E-TRMF model NUCLEAR STRUCTURE 227,228,229,230,231,232,244,245,246,247,248,249,250,251,252,253,254,255,256,257,258,259,260,261,262Th, 246,247,248,249,250,251,252,253,254,255,256,257,258,259,260,261,262,263,264U; calculated gs binding energy, mass excess, charge radius, neutron skin thickness using NL3, FSLGarnet and IOPB-I force parameters, excitation energy E* vs nuclear temperature, nuclear shell correction, 2n separation energy vs temperature, entropy (squared) vs excitation E*, neutron energy spectrum of selected levels, quadrupole and hexadecapole deformations and rms neutron and rms proton radii, level density parameter vs temperature, asymmetry energy coefficient vs temperature and vs mass number.
doi: 10.1016/j.nuclphysa.2019.04.004
2018NA19 Braz.J.Phys. 48, 342 (2018) K.C.Naik, R.N.Panda, A.Quddus, S.K.Patra Astrophysical S-factor of some (p, γ) Reactions
doi: 10.1007/s13538-018-0569-5
2018QU03 J.Phys.(London) G45, 075102 (2018) Study of hot thermally fissile nuclei using relativistic mean field theory NUCLEAR STRUCTURE 208Pb, 234,236U, 240Pu; calculated the ground state binding energy per nucleon, charge radii, excitation and two-neutron separation energies, quadrupole and hexadecapole deformations parameters, asymmetry energy coefficient. FSUGarnet and IOPB-I parameter sets.
doi: 10.1088/1361-6471/aac3a5
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