NSR Query Results
Output year order : Descending NSR database version of May 10, 2024. Search: Author = N.Rudra Found 5 matches. 1996DE05 Phys.Rev. C53, 780 (1996) J.N.De, N.Rudra, S.Pal, S.K.Samaddar Refined Thomas-Fermi Description of Hot Nuclei NUCLEAR STRUCTURE 40Ca, 90Zr, 208Pb; calculated equilibrium gas density, pressure, compression moduli, level density parameter, entropy per particle, neutron evaporation lifetime vs temperature. Other nuclei in this mass range included. Hot nuclei, refined Thomas-Fermi description.
doi: 10.1103/PhysRevC.53.780
1994MA04 Phys.Rev. C49, 541 (1994) M.M.Majumdar, S.K.Samaddar, N.Rudra, J.N.De Finite Range Momentum and Density Dependent Effective Interaction and Analysis of Nuclear Incompressibility NUCLEAR STRUCTURE A=40-250; calculated giant monopole resonance energy vs mass. Finite range effective interaction, Thomas Fermi approximation based nuclear compressibility.
doi: 10.1103/PhysRevC.49.541
1991DE29 Nucl.Phys. A534, 294 (1991) J.N.De, D.Bandyopadhyay, S.K.Samaddar, N.Rudra Stability Against Nucleon Dripping in Hot Nuclei NUCLEAR STRUCTURE N=126; calculated isotone limiting temperature. Z=10-80; calculated n, p drip lines vs temperature. Thermodynamic model, metastable equilibrium.
doi: 10.1016/0375-9474(91)90499-V
1986RU06 Pramana 26, 409 (1986) Stochastic Model of Nuclear Levelwidth NUCLEAR STRUCTURE 207Pb; calculated single particle level widths. Stochastic model.
doi: 10.1007/BF02845713
1978RU02 Nucl.Phys. A312, 33 (1978) Structure Calculations of 18O: A Collective Hamiltonian Approach NUCLEAR STRUCTURE 18O; calculated ground-state band, binding energy using collective Hamiltonian where potential energy is sum of liquid-drop, shell collection terms. Kinetic energy computed microscopically.
doi: 10.1016/0375-9474(78)90573-0
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