NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = J.N.De Found 100 matches. 2021AG09 Eur.Phys.J. Special Topics 230, 517 (2021) B.K.Agrawal, T.Malik, J.N.De, S.K.Samaddar Constraining nuclear matter parameters from correlation systematics: a mean-field perspective
doi: 10.1140/epjs/s11734-021-00001-7
2020MA58 Phys.Rev. C 102, 052801(R) (2020) T.Malik, B.K.Agrawal, C.Providencia, J.N.De Unveiling the correlations of tidal deformability with the nuclear symmetry energy parameters
doi: 10.1103/PhysRevC.102.052801
2020MO26 Phys.Rev. C 102, 015802 (2020) C.Mondal, X.Vinas, M.Centelles, J.N.De Structure and composition of the inner crust of neutron stars from Gogny interactions NUCLEAR STRUCTURE A=15-215; calculated binding energies using variational Wigner-Kirkwood with shell and pairing corrections (VWKSP) and HFB methods using D1M, D1S and D1M* Gogny forces, and compared to experimental values for about 160 even-even nuclei. Z=5-100; calculated binding energies per particle at different nucleon densities for inner crust of neutron star subtracted by free nucleon mass using the D1M* Gogny force. 32Mg, 40,50Ca, 90Zr, 100Sn, 142Sm, 176Hg, 208Pb, 216Po, 224U; calculated binding energies using VWKSP and HFB methods using D1M* Gogny force and compared with experimental values. Calculated number of protons (Z=20-92) and the total number of baryons (A=100-2500) corresponding to the β-equilibrium configurations as a function of the inner crust density, and constructed the equation of state (EoS) of the inner crust of neutron stars for D1M, D1S and D1M* interactions.
doi: 10.1103/PhysRevC.102.015802
2019MA35 Phys.Rev. C 99, 052801 (2019) T.Malik, B.K.Agrawal, J.N.De, S.K.Samaddar, C.Providencia, C.Mondal, T.K.Jha Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei
doi: 10.1103/PhysRevC.99.052801
2018MA70 Phys.Rev. C 98, 064316 (2018) T.Malik, C.Mondal, B.K.Agrawal, J.N.De, S.K.Samaddar Nucleon effective mass and its isovector splitting NUCLEAR STRUCTURE 48Ca, 68Ni, 120Sn, 208Pb; calculated dipole enhancement factor, correlation of the isovector parameter, and energy weighted sum rule using energy density functional (EDF) based on the thermodynamic Gibbs-Duhem relation. Nucleon effective mass and its isovector splitting. Comparison with other theoretical predictions.
doi: 10.1103/PhysRevC.98.064316
2018MO26 Int.J.Mod.Phys. E27, 1850078 (2018) C.Mondal, B.K.Agrawal, J.N.De, S.K.Samaddar Correlations among symmetry energy elements in Skyrme models
doi: 10.1142/S0218301318500787
2017BI07 Phys.Rev. C 95, 045201 (2017) S.Biswas, J.N.De, P.S.Joarder, S.Raha, D.Syam Multifragmentation model for the production of astrophysical strangelets
doi: 10.1103/PhysRevC.95.045201
2017MO23 Phys.Rev. C 96, 021302 (2017) C.Mondal, B.K.Agrawal, J.N.De, S.K.Samaddar, M.Centelles, X.Vinas Interdependence of different symmetry energy elements
doi: 10.1103/PhysRevC.96.021302
2016MO10 Phys.Rev. C 93, 044328 (2016) C.Mondal, B.K.Agrawal, J.N.De, S.K.Samaddar Sensitivity of elements of the symmetry energy of nuclear matter to the properties of neutron-rich systems NUCLEAR STRUCTURE 16,24O, 20,30Ne, 24,36Mg, 40,48,54,58Ca, 56,68,78Ni, 90Zr, 100,116,132,138Sn, 144Sm, 208Pb; analyzed best-fit parameters for binding energy and charge radius of a nucleus. Nuclear symmetry energy matter density for ultra-neutron-rich nuclei. Maximum mass of a neutron star. Relativistic mean field model.
doi: 10.1103/PhysRevC.93.044328
2015DE19 Phys.Rev. C 92, 014304 (2015) J.N.De, S.K.Samaddar, B.K.Agrawal Reassessing nuclear matter incompressibility and its density dependence
doi: 10.1103/PhysRevC.92.014304
2015MO16 Phys.Rev. C 92, 024302 (2015) Constraining the symmetry energy content of nuclear matter from nuclear masses: A covariance analysis NUCLEAR STRUCTURE 16,24O, 18,30Ne, 40,48Ca, 56,68Ni, 90Zr, 100,116,132Sn, 144Sm, 208Pb; calculated binding energies and charge radii, binding energy/nucleon, incompressibility coefficient K, Dirac effective mass of nucleon, symmetry energy coefficient, density slope parameter of symmetry energy, and neutron skins using two different models and constrained by experimental masses. Covariance analysis. Relativistic mean-field (RMF) approach using 16 different models.
doi: 10.1103/PhysRevC.92.024302
2014AG02 Eur.Phys.J. A 50, 19 (2014) B. K. Agrawal, J. N. De, S. K. Samaddar, M. Centelles, X.Vinas Symmetry energy of warm nuclear systems NUCLEAR STRUCTURE A=56, 112, 150, 208; calculated symmetry energy coefficients vs temperature using energy functional with Skyrme interaction and subtracted finite-temperature Thomas-Fermi.
doi: 10.1140/epja/i2014-14019-8
2014AG05 Phys.Rev. C 89, 044320 (2014) B.K.Agrawal, D.Bandyopadhyay, J.N.De, S.K.Samaddar Thermal properties of the nuclear surface
doi: 10.1103/PhysRevC.89.044320
2014AL31 Phys.Rev. C 90, 054317 (2014) N.Alam, B.K.Agrawal, J.N.De, S.K.Samaddar, G.Colo Equation of state of nuclear matter from empirical constraints
doi: 10.1103/PhysRevC.90.054317
2013AG06 Phys.Rev. C 87, 051306 (2013) B.K.Agrawal, J.N.De, S.K.Samaddar, G.Colo, A.Sulaksono Constraining the density dependence of the symmetry energy from nuclear masses NUCLEAR STRUCTURE 208Pb, 238U; calculated symmetry slope parameter L, neutron skin thickness for spherical and deformed nuclei, symmetry energy using a microscopic framework with different energy density functionals.
doi: 10.1103/PhysRevC.87.051306
2012AG22 Phys.Rev.Lett. 109, 262501 (2012) B.K.Agrawal, J.N.De, S.K.Samaddar Determining the Density Content of Symmetry Energy and Neutron Skin: An Empirical Approach NUCLEAR STRUCTURE 208Pb; calculated energy density functionals, symmetry energy slope parameter, neutron skin thickness.
doi: 10.1103/PhysRevLett.109.262501
2012DE02 Phys.Rev. C 85, 024310 (2012) Temperature dependence of the symmetry energy of finite nuclei NUCLEAR STRUCTURE A=26, Z=10, 12; A=40, Z=16, 18; A=56, Z=24, 26, 28; A=64, Z=26, 28, 30; A=80, Z=34, 36; A=112, Z=48, 50, 52; A=120, Z=50, 52; A=150, Z=60, 62; A=197, Z=77, 79; A=238, Z=90, 92; calculated symmetry energy coefficient as function of nuclear mass, temperature dependence of symmetry energy for various nucleon pairs. Thomas-Fermi model with SkM* and SBM interactions.
doi: 10.1103/PhysRevC.85.024310
2012DE17 Phys.Rev. C 86, 024606 (2012) J.N.De, S.K.Samaddar, X.Vinas, M.Centelles, I.N.Mishustin, W.Greiner Effects of medium on nuclear properties in multifragmentation
doi: 10.1103/PhysRevC.86.024606
2011SA21 Phys.Rev. C 83, 055802 (2011) Warm α-nucleon matter
doi: 10.1103/PhysRevC.83.055802
2010DE36 Phys.Rev. C 82, 045201 (2010) J.N.De, S.K.Samaddar, B.K.Agrawal Anatomy of the symmetry energy of dilute nuclear matter
doi: 10.1103/PhysRevC.82.045201
2010SA06 Phys.Rev. C 81, 041601 (2010) Examining the efficacy of isotope thermometry in the S-matrix approach NUCLEAR STRUCTURE 124Sn; calculated temperature and volume of a hot fragmenting nuclear system by isotope thermometry in the S-matrix approach.
doi: 10.1103/PhysRevC.81.041601
2009SA18 Phys.Rev. C 79, 051602 (2009) Scattering effects on nuclear thermodynamic observables
doi: 10.1103/PhysRevC.79.051602
2009SA36 Phys.Rev. C 80, 035803 (2009) S.K.Samaddar, J.N.De, X.Vinas, M.Centelles Symmetry coefficients and incompressibility of clusterized supernova matter
doi: 10.1103/PhysRevC.80.035803
2008DE33 Phys.Rev. C 78, 065204 (2008) Nuclear condensation and symmetry energy of dilute nuclear matter: An S-matrix approach
doi: 10.1103/PhysRevC.78.065204
2008MA11 Phys.Rev. C 77, 032201 (2008) S.Mallik, J.N.De, S.K.Samaddar, S.Sarkar S-matrix approach to equation of state of nuclear matter
doi: 10.1103/PhysRevC.77.032201
2008SA37 Phys.Rev. C 78, 034607 (2008) S.K.Samaddar, J.N.De, X.Vinas, M.Centelles Density dependence of the symmetry free energy of hot nuclei NUCLEAR STRUCTURE 40S, 110Sn, 150Sm, 150Cs, 197Au; calculated equilibrium temperature, equilibrium central density, symmetry coefficients for nuclear matter.
doi: 10.1103/PhysRevC.78.034607
2007DE54 Phys.Rev. C 76, 044607 (2007) Nuclear condensation and the equation of state of nuclear matter
doi: 10.1103/PhysRevC.76.044607
2007SA34 Phys.Rev. C 75, 054608 (2007) S.K.Samaddar, J.N.De, X.Vinas, M.Centelles Density reorganization in hot nuclei NUCLEAR STRUCTURE 40S, 40Ca, 150Sm, 150Yb, 150Cs; calculated equilibrium density profile as a function of excitation energy.
doi: 10.1103/PhysRevC.75.054608
2007SA52 Phys.Rev. C 76, 041602 (2007) S.K.Samaddar, J.N.De, X.Vinas, M.Centelles Excitation energy dependence of the symmetry energy of finite nuclei NUCLEAR STRUCTURE 40S, 150Sm, 150Cs; calculated density and temperature dependence of symmetry coefficients, nucleon-nucleon collisions.
doi: 10.1103/PhysRevC.76.041602
2006DE16 Phys.Rev. C 73, 034602 (2006) J.N.De, S.K.Samaddar, S.Shlomo, J.B.Natowitz Continuous phase transition and negative specific heat in finite nuclei NUCLEAR STRUCTURE 40,50Ca, 150Re, 150Nd; calculated thermodynamic quantities, phase transition features. Heated liquid-drop model.
doi: 10.1103/PhysRevC.73.034602
2006DE29 Phys.Lett. B 638, 160 (2006) J.N.De, S.K.Samaddar, X.Vinas, M.Centelles Nuclear expansion with excitation NUCLEAR STRUCTURE 150Sm; calculated thermodynamic quantities, density, phase transition features. Skyrme type effective two-body interaction model.
doi: 10.1016/j.physletb.2006.05.046
2005CE03 Phys.Rev. C 72, 014304 (2005) M.Centelles, X.Vinas, S.K.Patra, J.N.De, T.Sil Sum rule approach to the isoscalar giant monopole resonance in drip line nuclei NUCLEAR STRUCTURE O, Ca, Ni, Zr, Pb; calculated giant monopole resonance energies, sum rules. Density-dependent Hartree-Fock approximation, Skyrme forces.
doi: 10.1103/PhysRevC.72.014304
2005SA02 Phys.Rev. C 71, 011601 (2005) S.K.Samaddar, J.N.De, A.Bonasera Ambiguities in statistical calculations of nuclear fragmentation NUCLEAR STRUCTURE 197Au; calculated fragment charge distributions, isotopic yield ratios for fragmentation of excited system, possible recombination effects. Statistical approach.
doi: 10.1103/PhysRevC.71.011601
2004SA29 Phys.Rev. C 69, 064615 (2004) S.K.Samaddar, J.N.De, S.Shlomo Flow effects on multifragmentation in the canonical model NUCLEAR STRUCTURE 109Ag, 197Au; calculated fragment multiplicities, flow effects in multifragmentation of hot nuclei. Analytically solvable canonical model.
doi: 10.1103/PhysRevC.69.064615
2004SI01 Phys.Rev. C 69, 014602 (2004) T.Sil, S.K.Samaddar, J.N.De, S.Shlomo Liquid-gas phase transition in infinite and finite nuclear systems NUCLEAR STRUCTURE 50Ca, 150,186Re; calculated thermodynamic quantities, phase transition features. Heated liquid drop model.
doi: 10.1103/PhysRevC.69.014602
2002SI25 Phys.Rev. C66, 045803 (2002) T.Sil, J.N.De, S.K.Samaddar, X.Vinas, M.Centelles, B.K.Agrawal, S.K.Patra Isospin-rich nuclei in neutron star matter NUCLEAR STRUCTURE 140,330Pb, 80Ca, 170Sn; calculated nuclear properties in neutron-star environment.
doi: 10.1103/PhysRevC.66.045803
2001AG02 Phys.Rev. C63, 024002 (2001) B.K.Agrawal, T.Sil, S.K.Samaddar, J.N.De Shape Transition in Some Rare-Earth Nuclei in Relativistic Mean Field Theory NUCLEAR STRUCTURE 148,150Sm, 150,152Gd, 152,154Dy; calculated β2 deformation, pairing gaps vs nuclear temperature, shape transitions. Relativistic mean-field approach.
doi: 10.1103/PhysRevC.63.024002
2001AG08 Phys.Rev. C64, 017304 (2001) B.K.Agrawal, T.Sil, S.K.Samaddar, J.N.De Temperature Induced Shell Effects in Deformed Nuclei NUCLEAR STRUCTURE 64,66Zn, 148,150Sm, 152,154Dy; calculated deformation, shell-correction energy vs temperature.
doi: 10.1103/PhysRevC.64.017304
2001AG09 Phys.Rev. C64, 024305 (2001) B.K.Agrawal, T.Sil, S.K.Samaddar, J.N.De, S.Shlomo Coulomb Energy Differences in Mirror Nuclei Revisited NUCLEAR STRUCTURE 15,16,17O, 32S, 39,40,41,48Ca, 56Ni, 90Zr, 208Pb; calculated radii. 15,17O, 15N, 17F, 39,41Ca, 39K, 41Sc, 55,57Ni, 55Co, 57Cu; calculated Coulomb displacement energies. Relativistic mean-field model, comparison with other models and data.
doi: 10.1103/PhysRevC.64.024305
2001DE43 Phys.Rev. C64, 057306 (2001) J.N.De, X.Vinas, S.K.Patra, M.Centelles Nuclei Beyond the Drip Line NUCLEAR STRUCTURE 140,208,340Pb; calculated neutron and proton densities. Ca, Pb calculated radii; deduced limiting asymmetry. Thomas-Fermi model.
doi: 10.1103/PhysRevC.64.057306
2001SI20 Phys.Rev. C63, 054604 (2001) T.Sil, B.K.Agrawal, J.N.De, S.K.Samaddar Liquid-Gas Phase Transition in Nuclei in the Relativistic Thomas-Fermi Theory NUCLEAR STRUCTURE 40Ca, 109Ag, 150Sm; calculated equations of state, caloric curves, other thermodynamic properties. Relativistic Thomas-Fermi theory.
doi: 10.1103/PhysRevC.63.054604
2001SI22 Phys.Rev. C63, 064302 (2001) T.Sil, B.K.Agrawal, J.N.De, S.K.Samaddar Anatomy of Nuclear Shape Transition in the Relativistic Mean Field Theory NUCLEAR STRUCTURE 148,150Sm, 64Zn; calculated single-particle levels, deformation vs temperature. Relativistic mean-field theory.
doi: 10.1103/PhysRevC.63.064302
2000AG07 Phys.Rev. C62, 044307 (2000) B.K.Agrawal, T.Sil, J.N.De, S.K.Samaddar Nuclear Shape Transition at Finite Temperature in a Relativistic Mean Field Approach NUCLEAR STRUCTURE 168,170Er; calculated deformation, pairing strength vs temperature, related features. Relativistic mean-field approach.
doi: 10.1103/PhysRevC.62.044307
1999AG01 Phys.Rev. C59, 832 (1999) B.K.Agrawal, S.K.Samaddar, T.Sil, J.N.De Isotope Thermometry in Nuclear Multifragmentation NUCLEAR STRUCTURE 150Sm; calculated fragmenting system temperature vs excitation energy, time. Comparison of several double-ratio thermometers.
doi: 10.1103/PhysRevC.59.832
1999AG03 Phys.Rev. C59, 3109 (1999) B.K.Agrawal, S.K.Samaddar, A.Ansari, J.N.De Influence of Pairing Correlations on the Excitation Energy, Angular Momentum, and Parity Dependence of Nuclear Level Densities NUCLEAR STRUCTURE 152Sm, 160Yb; calculated level density, related parameters vs excitation energy; deduced pair correlation effects. Static path approximation.
doi: 10.1103/PhysRevC.59.3109
1999DE01 Phys.Rev. C59, R1 (1999) J.N.De, B.K.Agrawal, S.K.Samaddar Equation of State of Finite Nuclei and Liquid-Gas Phase Transition NUCLEAR STRUCTURE 85Kr, 150Sm; calculated equation of state; deduced critical temperatures, finite size effects. Thomas-Fermi framework.
doi: 10.1103/PhysRevC.59.R1
1999SA29 Phys.Lett. 459B, 8 (1999) S.K.Samaddar, S.Das Gupta, J.N.De, B.K.Agrawal, T.Sil The One Body Density in a Finite Size Lattice Gas Model
doi: 10.1016/S0370-2693(99)00665-6
1998AG13 Phys.Rev. C58, 3004 (1998) B.K.Agrawal, S.K.Samaddar, J.N.De, S.Shlomo Large-Model-Space Calculation of the Nuclear Level Density Parameter at Finite Temperature NUCLEAR STRUCTURE 40Ca, 56Fe; calculated level density parameter vs temperature; deduced shell effects, continuum corrections, other contributions. Microscopic model.
doi: 10.1103/PhysRevC.58.3004
1998DE07 Phys.Rev. C57, 1398 (1998) J.N.De, S.Shlomo, S.K.Samaddar Level Density Parameter in a Refined Thomas-Fermi Theory NUCLEAR STRUCTURE 150Sm; calculated level density parameter vs temperature. Thomas-Fermi theory, second-order corrections.
doi: 10.1103/PhysRevC.57.1398
1998DE12 Nucl.Phys. A630, 192c (1998) Liquid-Gas Phase Transition in Finite Nuclei NUCLEAR STRUCTURE 150Sm; calculated caloric curve, specific heat; deduced phase transition. Thomas-Fermi theory.
doi: 10.1016/S0375-9474(97)00756-2
1998PA17 Phys.Rev. C57, 3246 (1998) S.Pal, S.K.Samaddar, J.N.De, B.Djerroud Multiplicity Scaling in Nuclear Fragmentation NUCLEAR STRUCTURE Ca, Ag, Sm, Au; calculated intermediate mass fragment multiplicities from highly excited nuclei; deduced scaling behavior.
doi: 10.1103/PhysRevC.57.3246
1998UM03 Phys.Rev. D57, 3242 (1998) V.S.Uma Maheswari, J.N.De, S.K.Samaddar Hybrid Stars: Spin-polarized nuclear matter and density-dependent quark masses
doi: 10.1103/PhysRevD.57.3242
1997DE09 Phys.Rev. C55, R1641 (1997) J.N.De, S.Das Gupta, S.Shlomo, S.K.Samaddar Caloric Curve for Finite Nuclei in Thomas-Fermi Theory NUCLEAR STRUCTURE 150Sm; calculated proton density profile vs temperature, volume, temperature vs excitation energy per particle, specific heat per particle vs temperature. 85Kr; calculated temperature vs excitation energy per particle, specific heat per particle vs temperature. Finite temperature Thomas-Fermi theory.
doi: 10.1103/PhysRevC.55.R1641
1997SA62 Phys.Rev.Lett. 79, 4962 (1997) S.K.Samaddar, J.N.De, S.Shlomo Effect of Flow on the Caloric Curve for Finite Nuclei NUCLEAR STRUCTURE 150Sm; calculated energy, specific heat per nucleon vs temperature, proton rms radius, density; deduced liquid-gas phase transition. Finite temperature Thomas-Fermi theory.
doi: 10.1103/PhysRevLett.79.4962
1997SH17 Phys.Rev. C55, R2155 (1997) Effect of Flow on the Freeze-Out Density and Temperature of Disassembling Hot Nuclei
doi: 10.1103/PhysRevC.55.R2155
1997UM02 Nucl.Phys. A615, 516 (1997) V.S.Uma Maheswari, D.N.Basu, J.N.De, S.K.Samaddar Spin Polarised Nuclear Matter and Its Application to Neutron Stars
doi: 10.1016/S0375-9474(97)00002-X
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
1996PA24 Nucl.Phys. A608, 49 (1996) The Effect of Flow on Nuclear Multifragmentation in a Quantum Statistical Model NUCLEAR STRUCTURE 108Ag; calculated charge yield, intermediate mass fragment, charged particle multiplicity vs temperature; deduced radial collective flow role. Prompt multi-fragmentation, quantum statistical model.
doi: 10.1016/S0375-9474(96)00271-0
1995PA13 Nucl.Phys. A586, 466 (1995) S.Pal, S.K.Samaddar, A.Das, J.N.De Recombination Effect in Nuclear Multifragmentation NUCLEAR STRUCTURE 150Sm; calculated fragment charge yield, multiplicity probability distribution, other aspects following fragmentation. Sequential binary decay, prompt multi-fragmentation models.
doi: 10.1016/0375-9474(95)00620-G
1995PA20 Nucl.Phys. A589, 489 (1995) Signature of Exotic Nuclear Shapes from IMF-IMF Correlations NUCLEAR STRUCTURE 150Sm; calculated three-fragment configurations charge distributions, angle-integrated correlation functions; deduced exotic nuclear shapes signature related features. BUU type framework calculations.
doi: 10.1016/0375-9474(95)00130-S
1995PA32 Nucl.Phys. A591, 719 (1995) Effect of Neighbouring Fragments on Sequential Binary Decay NUCLEAR REACTIONS Cu(197Au, X), E=600 MeV/nucleon; analyzed fragmentation data. Transition state model.
doi: 10.1016/0375-9474(95)00189-8
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
1994PA39 Phys.Lett. 337B, 14 (1994) S.Pal, S.K.Samaddar, A.Das, J.N.De Microcanonical Simulation of Multifragmentation of Exotic Nuclear Shapes NUCLEAR STRUCTURE 150Sm; calculated charged particle multiplicity distributions, other observables. Multi-fragmentation, toroidal, bubble nuclei, statistical model, microcanonical simulation.
doi: 10.1016/0370-2693(94)91435-4
1993MA41 Phys.Rev. C48, 2093 (1993) M.M.Majumdar, J.N.De, C.Samanta, S.K.Samaddar Role of Nuclear Compressibility on the Fission Path NUCLEAR STRUCTURE 238U, 208Pb; calculated equilibrium density along fission path, deformation energy, volume, Coulomb, surface contributions; deduced nuclear compressibility role. Semi-macroscopic framework.
doi: 10.1103/PhysRevC.48.2093
1992BA12 Nucl.Phys. A539, 370 (1992) D.Bandyopadhyay, S.K.Samaddar, R.Saha, J.N.De Fusion Limited by Temperature NUCLEAR REACTIONS 27Al(40Ar, X), 58Ni(35Cl, X), 40Ca(40Ca, X), E ≈ 5-50 MeV/nucleon; calculated fusion σ(E); deduced temperature dependence.
doi: 10.1016/0375-9474(92)90275-O
1992KR09 Nucl.Phys. A542, 159 (1992) K.Krishan, S.Bhattacharya, J.N.De, S.K.Samaddar Distribution of Angular Momentum in Incomplete Fusion Reaction NUCLEAR REACTIONS 27Al(84Kr, X), E=20, 30 MeV/nucleon; calculated prompt particle average number vs incident L, incompletely fused composites mass, excitation energy, angular momentum distribution. Dynamic trajectory model, particle exchange dissipation, Monte Carlo simulation technique.
doi: 10.1016/0375-9474(92)90404-8
1992SA24 Phys.Rev. C46, 2631 (1992) S.K.Samaddar, J.N.De, D.Sperber Realistic Estimate of Incomplete Fusion Excitation Function in Nucleus-Nucleus Collisions NUCLEAR REACTIONS 200Hg, 40Ca(40Ca, X), E ≤ 60 MeV/nucleon; calculated fusion σ(E). 200Hg(40Ca, X), E ≤ 40 MeV/nucleon; calculated hot residues mass, charge vs E, hot composite maximum angular momentum vs E. Promptly emitted particles model.
doi: 10.1103/PhysRevC.46.2631
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
1990BA17 Nucl.Phys. A511, 1 (1990) D.Bandyopadhyay, C.Samanta, S.K.Samaddar, J.N.De Thermostatic Properties of Finite and Infinite Nuclear Systems NUCLEAR STRUCTURE A=50-200; calculated limiting temperature vs mass number.
doi: 10.1016/0375-9474(90)90024-G
1990DE24 Phys.Rev. C42, R819 (1990) Temperature Dependence of Fusion Barriers NUCLEAR REACTIONS 58Ni(35Cl, X), 40Ca(40Ca, X), E not given; calculated free interaction energy vs separation distance, fusion barrier. 70Ge(27Al, X), 74Ge(74Ge, X), 100Mo(100Mo, X), E not given; calculated fusion barrier.
doi: 10.1103/PhysRevC.42.R819
1989BH03 Phys.Rev.Lett. 62, 2589 (1989) S.Bhattacharya, J.N.De, K.Krishan, S.K.Samaddar Role of Two-Body Collisions in Limiting Momentum Transfer and Energy Deposition in Nucleus-Nucleus Collisions NUCLEAR REACTIONS 40Ca(14N, X), 56Fe(20Ne, X), 90Zr(32S, X), E=10-50 MeV/nucleon; calculated linear momentum transfer, temperature vs E. Promptly emitted particle model.
doi: 10.1103/PhysRevLett.62.2589
1989KR04 Nucl.Phys. A495, 65c (1989) K.Krishan, S.Bhattacharya, J.N.De, S.K.Samaddar Saturation of Energy Deposition and Linear Momentum Transfer in Heavy Ion Collisions NUCLEAR REACTIONS 56Fe(20Ne, X), 90Zr(32S, X), 40Ca(14N, X), E ≤ 10 MeV/nucleon; calculated fractional linear momentum transfer vs E. Prompt emission model.
doi: 10.1016/0375-9474(89)90308-4
1989SA59 Phys.Lett. B 217, 381 (1989) C.Samanta, D.Bandyopadhyay, J.N.De Incompressibility of asymmetric nuclear matter
doi: 10.1016/0370-2693(89)90064-6
1988BH06 Phys.Rev. C37, 2916 (1988) S.Bhattacharya, K.Krishan, S.K.Samaddar, J.N.De Realistic Estimates for Promptly Emitted Particles NUCLEAR REACTIONS 165Ho(20Ne, xn), E=220, 292, 402 MeV; 165Ho(12C, xn), E=300 MeV; calculated promptly emitted multiplicities.
doi: 10.1103/PhysRevC.37.2916
1988KR13 J.Phys.(London) G14, 1423 (1988) K.Krishan, S.K.Samaddar, J.N.De Spin Dispersion and Alignment in Deep Inelastic Collisions NUCLEAR REACTIONS 209Bi(86Kr, X), E=610 MeV; 238U(86Kr, X), E=730 MeV; 154Sm(32S, X), E=214 MeV; calculated fragment angular momentum gain vs incident L, spin variances vs energy loss. Stochastic nucleon exchange model.
doi: 10.1088/0305-4616/14/11/013
1987BA01 Nucl.Phys. A462, 587 (1987) D.Bandyopadhyay, S.R.Samaddar, K.Krishan, J.N.De Energy Dependent Nucleus-Nucleus Potential in Heavy Ion Collisions NUCLEAR REACTIONS 208Pb, 16O(16O, 16O), 208Pb(208Pb, 208Pb), E=0-40 MeV/nucleon; calculated nucleus-nucleus potential parameters. 27Al(16O, X), E(cm) ≈ 50-100 MeV; 17O(13C, X), E(cm) ≈ 8-50 MeV; 26Mg(20Ne, X), E(cm) ≈ 8-50 MeV; 27Al(32S, X), E ≈ 33-500 MeV; 109Ag(40Ar, X), E(cm) ≈ 100-500 MeV; calculated fusion σ(E). Proximity model.
doi: 10.1016/0375-9474(87)90407-6
1987BA57 Phys.Lett. 196B, 424 (1987) D.Bandopadhyay, S.K.Samaddar, K.Krishan, J.N.De Spectator Recoil and Nucleon Emission Spectra in Intermediate-Energy Nuclear Collisions NUCLEAR REACTIONS 124Sn(40Ar, X), E=44 MeV/nucleon; 197Au(12C, X), E=85 MeV/nucleon; calculated σ(E(p), θ(p)), σ(fragment θ, E), X(A)=70-130. Hot-zone model.
doi: 10.1016/0370-2693(87)90794-5
1987SA43 J.Phys.(London) G13, L231 (1987) S.K.Samaddar, K.Krishan, J.N.De Role of Barrier on Spin Orientation in Nucleus-Nucleus Collisions NUCLEAR REACTIONS 209Bi(86Kr, X), E=610 MeV; calculated fragment spin orientation. Stochastic nucleon exchange model.
doi: 10.1088/0305-4616/13/10/002
1986BH08 Z.Phys. A325, 79 (1986) S.Bhattacharyya, J.N.De, S.K.Samaddar, K.Krishan Mass and Charge Distributions with Correlated Exchange NUCLEAR REACTIONS 56Fe(56Fe, X), 166Er, 139La(86Kr, X), E not given; calculated energy loss-mass variance correlation, inclusive variances isospin correlation coefficient dependence. Correlated nucleon exchange model.
1986SA01 Nucl.Phys. A451, 160 (1986) S.K.Samaddar, M.M.Majumdar, B.C.Samanta, J.N.De Vacuum Polarization and the Nuclear Mass Formula NUCLEAR REACTIONS 109Ag(109Ag, X), E(cm) ≈ 227-237 MeV; calculated fusion σ(E); deduced vacuum polarization role.
doi: 10.1016/0375-9474(86)90249-6
1985DE25 Nucl.Phys. A440, 152 (1985) On the Influence of the Shell Structure of Single-Particle Levels in Dissipative Heavy-Ion Collisions NUCLEAR REACTIONS 208Pb(208Pb, X), E=7.6 MeV/nucleon; 209Bi(136Xe, X), E=940, 1130, 1422 MeV; 208Pb(238U, X), E=7.5 MeV/nucleon; 144Sm(144Sm, X), E=6.95 MeV/nucleon; 154Sm(154Sm, X), E=6.3 MeV/nucleon; calculated fragment energy loss vs charge distribution variance; deduced shell structure role on single particle levels. Dissipative heavy ion collision, Randrup formalism.
doi: 10.1016/0375-9474(85)90047-8
1985DE44 Nucl.Phys. A445, 173 (1985) J.N.De, K.Krishan, S.K.Samaddar The Effect of the Shell Gap in Strongly Damped Collisions NUCLEAR REACTIONS 209Bi(56Fe, X), E=465 MeV; 144Sm(144Sm, X), E=6.95 MeV/nucleon; 209Bi(136Xe, X), E=940 MeV; 208Pb(208Pb, X), E=7.6 MeV/nucleon; calculated fragment charge variance energy dependence. 238U, 165Ho(56Fe, X), E=465 MeV; calculated fragment energy loss, charge variance correlation.
doi: 10.1016/0375-9474(85)90367-7
1985SA08 Phys.Rev. C31, 1053 (1985) S.K.Samaddar, J.N.De, K.Krishan Thermal Equilibrium in Strongly Damped Collisions NUCLEAR REACTIONS 238U, 165Ho(56Fe, X), E=465 MeV; calculated fragment charge centroids, variances, energy division. Nucleon exchange model, Monte-Carlo simulation.
doi: 10.1103/PhysRevC.31.1053
1984DE40 Phys.Rev. C30, 1763 (1984) Correlation between Neutrons and Protons in Heavy Ion Collisions NUCLEAR REACTIONS 56Fe, 165Ho, 209Bi, 238U(56Fe, X), 144Sm(144Sm, X), E not given; calculated fragment mass, charge distribution variances ratio vs correlation coefficient. Nucleon exchange model.
doi: 10.1103/PhysRevC.30.1763
1984DE41 J.Phys.(London) G10, L257 (1984) J.N.De, K.Krishan, S.K.Samaddar The Mass and Charge Variances in Sm + Sm Collisions NUCLEAR REACTIONS 154Sm(154Sm, X), E=970 MeV; 144Sm(144Sm, X), E=1000 MeV; calculated charge, mass variances.
doi: 10.1088/0305-4616/10/2/016
1983DE05 Phys.Rev. C27, 1328 (1983) Analysis of Energy Loss Versus Fragment Charge Distributions for the 136Xe + 209Bi System NUCLEAR REACTIONS 209Bi(136Xe, X), E=940, 1130, 1422 MeV; analyzed data; deduced nucleon exchange role. Transport model, isospin effects.
doi: 10.1103/PhysRevC.27.1328
1982DE01 Phys.Rev.Lett. 48, 81 (1982) J.N.De, S.K.Samaddar, K.Krishan Role of Stochastic Transfer of Nucleons for Angular Momentum Misalignment in Nuclear Collisions NUCLEAR REACTIONS 238U(86Kr, X), E=730 MeV; calculated target angular momentum gain, alignment factor vs (L), energy loss. Stochastic nucleon transfer, Pauli effect.
doi: 10.1103/PhysRevLett.48.81
1982DE23 Phys.Lett. 113B, 455 (1982) Stochastic Transfer and Isobaric and Isotopic Distributions in Nuclear Collisions NUCLEAR REACTIONS 165Ho(56Fe, X), E=464 MeV; analyzed fragment charge, mass distribution centroid ratios, mass, charge variance ratios, isotopic charge distributions vs energy loss. Stochastic nucleon transfer.
doi: 10.1016/0370-2693(82)90784-5
1981KA28 Nucl.Phys. A367, 122 (1981) A.O.T.Karvinen, J.N.De, B.Jakobsson Single-Nucleon and Heavy Recoil Spectra in Intermediate Energy Heavy-Ion Reactions NUCLEAR REACTIONS 108Ag(12C, n), E=35, 50, 86 MeV/nucleon; calculated σ(θ) for preequilibrium, equilibrium emission. Local large volume hot zone assumption.
doi: 10.1016/0375-9474(81)90281-5
1981SA11 Phys.Scr. 23, 231 (1981) S.K.Samaddar, A.Sherman, D.Sperber, M.Zielinska-Pfabe, J.N.De The Role of Deformation, Thermal Fluctuations and Single Particle Transfer in Strongly Damped Collisions NUCLEAR REACTIONS 209Bi(136Xe, X), E=1130 MeV; 209Bi(84Kr, X), E=600 MeV; calculated σ(fragment Z), deflection function, final kinetic energy vs incident L, σ(fragment θ); deduced role of deformation, thermal fluctuations, single particle transfer. Dynamical model, strongly damped collisions.
doi: 10.1088/0031-8949/23/3/003
1980BO01 Nucl.Phys. A333, 285 (1980) J.P.Bondorf, J.N.De, G.Fai, A.O.T.Karvinen, B.Jakobsson, J.Randrup Promptly Emitted Particles in Nuclear Collisions NUCLEAR REACTIONS 158Gd(12C, X), E=152 MeV; 146Nd(16O, X), E=126.5 MeV; 158Gd(α, X), E=45 MeV; 136Xe(45Sc, X), E=1360 MeV; calculated σ(E) for 1, 2 prompt nucleons. Proximity model, coupling of internal nucleon motion to relative nuclear motion.
doi: 10.1016/0375-9474(80)90234-1
1979BO15 Phys.Lett. 84B, 162 (1979) J.P.Bondorf, J.N.De, A.O.T.Karvinen, G.Fai, B.Jakobsson Prompt Emission of Nucleons in Heavy-Ion Collisions NUCLEAR REACTIONS 146Nd(16O, n), E=126.5 MeV; 158Gd(12C, n), E=152 MeV; calculated σ(E, θn, En); deduced mechanism of production of quasifree prompt emission. Sharp surface model.
doi: 10.1016/0370-2693(79)90273-9
1979SA36 Nucl.Phys. A332, 210 (1979) S.K.Samaddar, M.I.Sobel, J.N.De, S.I.A.Garpman, D.Sperber, M.Zielinska-Pfabe, S.Moller A Classical Dynamical Model with Shape Deformation for Strongly Damped Collisions NUCLEAR REACTIONS 209Bi(136Xe, X), E=1130 MeV; 209Bi(84Kr, X), E=600 MeV; calculated scattering angle, energy loss, mass transfer. Classical dynamical model, damped HI collisions.
doi: 10.1016/0375-9474(79)90106-4
1978BI05 Phys.Rev.Lett. 40, 1123 (1978) J.R.Birkelund, J.R.Huizenga, J.N.De, D.Sperber Heavy-Ion Fusion Based on the Proximity Potential and One-Body Friction NUCLEAR REACTIONS 27Al(16O, X), 58,60,62,64Ni, 112,116,120,124Sn(35Cl, X), 109Ag(40Ar, X); calculated fusion σ.
doi: 10.1103/PhysRevLett.40.1123
1978DE06 Phys.Lett. 72B, 293 (1978) The Role of Deformation and Transfer in the Analysis of Strongly Damped Collisions NUCLEAR REACTIONS 209Bi(136Xe, X), E=712, 1130 MeV; calculated σ(Z), σ(θ).
doi: 10.1016/0370-2693(78)90122-3
1978DE24 Phys.Lett. 78B, 13 (1978) J.N.De, S.I.A.Garpman, A.Sherman, D.Sperber, K.Tam A Stochastic Model for Strongly Damped Collisions with Liquid Drop Driving Forces NUCLEAR REACTIONS 209Bi(136Xe, X), E=1130 MeV; calculated σ(E(Z), θ).
doi: 10.1016/0370-2693(78)90335-0
1978DE40 S.Afr.J.Phys. 1, 239 (1978) J.N.De, A.Sherman, D.Sperber, J.R.Birkelund, J.R.Huizenga Fusion-Excitation Functions as a Test of the Radial Dependence of the Proximity Potential NUCLEAR REACTIONS 27Al(35Cl, X), E(cm)=50-300 MeV; 232Th(40Ar, X), E(cm)=20-55 MeV; calculated σ(fusion, E); deduced radial dependence of ion-ion potential. Proximity potential model.
1977DE07 Phys.Lett. 66B, 315 (1977) Deep Inelastic Collisions: A Classical Description with Friction and Deformation NUCLEAR REACTIONS 209Bi(84Kr, X), E=600 MeV; calculated σ.
doi: 10.1016/0370-2693(77)90003-X
1976DE26 Z.Phys. A277, 385 (1976) J.N.De, D.H.E.Gross, H.Kalinowski A Classical Description of Deep Inelastic Collisions NUCLEAR REACTIONS 232Th(40Ar, X), E=379 MeV; 40Ca(40Ca, X), E=278 MeV; 209Bi(84Kr, X), E=525, 600 MeV; 208Pb(40Ca, X), E=288 MeV; 186W(63Cu, X), E=395 MeV; 197Au(63Cu, X), E=443, 365 MeV; calculated σ for deep inelastic scattering.
doi: 10.1007/BF01545976
1974DE50 Pramana 2, 199 (1974) Structure Calculations in 18O Nucleus NUCLEAR STRUCTURE 18O; calculated levels, B(E2), quadrupole moment.
doi: 10.1007/BF02847795
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