NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = T.R.Routray Found 24 matches. 2023BA18 Phys.Rev. C 108, 015802 (2023) P.Bano, S.P.Pattnaik, M.Centelles, X.Vinas, T.R.Routray Correlations between charge radii differences of mirror nuclei and stellar observables NUCLEAR STRUCTURE 34,36S, 34,38Ar, 36Ca, 38Ca, 54Fe, 54Ni; calculated rms proton radii differences of mirror nuclei and correlation with neutron skin thickness, slope of the symmetry energy, tidal deformability and neutron star radius correlation to charge radii difference in mirror pairs and neutron skin thickness. Investigated isospin-symmetry breaking effect leading to a linear correlation between the proton rms radii difference in mirror pairs and neutron skin thickness. Simple effective interaction (SEI) finite-range model.
doi: 10.1103/PhysRevC.108.015802
2022BA29 Phys.Rev. C 106, 024313 (2022) P.Bano, X.Vinas, T.R.Routray, M.Centelles, M.Anguiano, L.M.Robledo Finite-range simple effective interaction including tensor terms NUCLEAR STRUCTURE 68,70,72,74,76,78Ni; calculated ground-state energies, neutron and proton single-particle levels around the Fermi level. 58,59,60,61,62,63,64,65,66,67,68,69,70Ni; calculated rms charge radii, isotope shifts. 69,71,73,75,77,79Cu; calculated ground-state energies. 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132Sn; calculated energy differences between 1h11/2 and 1g7/2 proton orbitals, single-particle neutron energies and their occupation probabilities. 132Sn, 134Te, 136Xe, 138Ba, 140Ce, 142Nd, 144Sm, 146Gd, 148Dy, 150Er; calculated energy differences between 1i13/2 and 1h9/2 neutron single-particle levels, and single-particle proton energies and their occupation probabilities in N=82 isotones. 91Zr, 93Mo, 95Ru, 97Pd, 99Cd, 101Sn; calculated neutron single-particle levels in N=51 isotones relative to the 2d5/2 level. Calculations based on simple effective interaction (SEI) with and without the addition of a short-range tensor force to SEI and SIII-T, SLy5-T, SAMi-T Skyrme and D1MTd Gogny effective interaction. Comparison with available experimental data.
doi: 10.1103/PhysRevC.106.024313
2021BE07 Phys.Scr. 96, 035302 (2021) D.Behera, S.K.Tripathy, T.R.Routray, B.Behera Nuclear symmetry energy parameters from neutron skin thickness in 208Pb and electric dipole polarizability in 68Ni, 120Sn and 208Pb NUCLEAR STRUCTURE 68Ni, 120Sn, 208Pb; calculated neutron skin thikness using the framework of droplet model with finite range effective interactions; deduced the density slope parameter of nuclear symmetry energy at saturation and at subsaturation densities.
doi: 10.1088/1402-4896/abd8a4
2021RO19 Phys.Rev. C 104, L011302 (2021) T.R.Routray, P.Bano, M.Anguiano, M.Centelles, X.Vinas, L.M.Robledo Reexamination of the N=50 and Z=28 shell closure NUCLEAR STRUCTURE 68,70,72,74,76,78Ni; calculated proton single-particle levels around the Fermi level. 69,71,73,75,77,79Cu; calculated energies and spins of the ground states, and energies of the first excited states. Quasilocal density functional theory (QLDFT) using Skyrme forces SAMi-T and SLy5 with the tensor part, D1M Gogny force, and simple effective interaction (SEI) model. Comparison with HFB calculations, and with experimental energies and spins of the first excited states.
doi: 10.1103/PhysRevC.104.L011302
2020BE31 Phys.Scr. 95, 105301 (2020) D.Behera, S.K.Tripathy, T.R.Routray, B.Behera Nuclear symmetry energy and neutron skin thickness of 208Pb using a finite range effective interaction NUCLEAR STRUCTURE 208Pb; analyzed available data; deduced a correlation between the neutron skin thickness in 208Pb and the density slope parameter at the subsaturation density.
doi: 10.1088/1402-4896/abb253
2019GO15 Phys.Rev. C 100, 015806 (2019) C.Gonzalez-Boquera, M.Centelles, X.Vinas, T.R.Routray Core-crust transition in neutron stars with finite-range interactions: The dynamical method
doi: 10.1103/PhysRevC.100.015806
2017MA43 Eur.Phys.J. A 53, 151 (2017) K.Madhuri, D.N.Basu, T.R.Routray, S.P.Pattnaik Crustal moment of inertia of glitching pulsars with the KDE0v1 Skyrme interaction
doi: 10.1140/epja/i2017-12338-x
2016BE06 J.Phys.(London) G43, 045115 (2016) B.Behera, X.Vinas, T.R.Routray, L.M.Robledo, M.Centelles, S.P.Pattnaik Deformation properties with a finite-range simple effective interaction NUCLEAR STRUCTURE Z=8-108; calculated binding energies and charge radii of even-even nuclei, potential energy surfaces, fission barriers, deformation properties. Finite-range simple effective interaction within the Hartree-Fock-Bogoliubov mean-field approach. Comparison with experimental data.
doi: 10.1088/0954-3899/43/4/045115
2016RO24 J.Phys.(London) G43, 105101 (2016) T.R.Routray, X.Vinas, D.N.Basu, S.P.Pattnaik, M.Centelles, L.B.Robledo, B.Behera Exact versus Taylor-expanded energy density in the study of the neutron star crust-core transition
doi: 10.1088/0954-3899/43/10/105001
2015BE09 J.Phys.(London) G42, 345103 (2015) B.Behera, X.Vinas, T.R.Routray, M.Centelles Study of spin polarized nuclear matter and finite nuclei with finite range simple effective interaction NUCLEAR STRUCTURE A<220; calculated charge radii and its uncertainty, neutron-proton effective mass splitting. Spin polarized pure neutron matter and symmetric nuclear matter (SNM).
doi: 10.1088/0954-3899/42/4/045103
2012RO17 Eur.Phys.J. A 48, 77 (2012) T.R.Routray, A.Mishra, S.K.Tripathy, B.Behera, D.N.Basu Proton radioactivity half-lives with Skyrme interactions RADIOACTIVITY 105Sb, 109I, 112,113Cs, 135Tb, 145,147Tm, 150,151Lu, 155,156,157Ta, 159,160,161Re, 164,165,166,167Ir, 171Au, 177Tl, 185Bi(p); calculated T1/2 using energy density formalism with different Skyrme interactions. Compared to the data.
doi: 10.1140/epja/i2012-12077-6
2011BE38 J.Phys.(London) G38, 115104 (2011) B.Behera, T.R.Routray, S.K.Tripathy Neutron-proton effective mass splitting and thermal evolution in neutron-rich matter
doi: 10.1088/0954-3899/38/11/115104
2011RO36 Eur.Phys.J. A 47, 92 (2011) T.R.Routray, S.K.Tripathy, B.B.Dash, B.Behera, D.N.Basu Proton radioactivity with a Yukawa effective interaction RADIOACTIVITY 105Sb, 109I, 112,113Cs, 145,147Tm, 150,151Lu, 155,156,157Ta, 160,161Re, 164,165,166,167Ir, 171Au, 177Tl, 185Bi(p); calculated T1/2 using finite-range effective NN interaction of single Yukawa term.
doi: 10.1140/epja/i2011-11092-5
2010BH09 Phys.Rev. C 82, 064602 (2010) M.Bhuyan, R.N.Panda, T.R.Routray, S.K.Patra Application of relativistic mean field and effective field theory densities to scattering observables for Ca isotopes NUCLEAR REACTIONS 40,42,44,48Ca(polarized p, p), E=300, 800, 1000 MeV; calculated proton and neutron density distributions, σ(θ), analyzing powers, spin observable Q value as function of scattering angle using relativistic mean field (RMF) theory with NL3 and G2 parameter sets. Comparison with experimental data.
doi: 10.1103/PhysRevC.82.064602
2009RO16 Nucl.Phys. A826, 223 (2009) T.R.Routray, J.Nayak, D.N.Basu Cluster radioactivity in very heavy nuclei: a new perspective RADIOACTIVITY 212,213,214Po, 215At(α); 221Fr, 221,222,223,224,226Ra, 225Ac(14C); 228Th(16O); 230U(22Ne); 230Th, 231Pa, 232,233,234U(24Ne); 233U(25Ne); 234U(26Ne); 234U, 236,238Pu(28Mg); 238Pu(30Mg), (32Si); 242Cm(34Si); calculated T1/2, cluster preformation probability, related features using a folding density dependent model.
doi: 10.1016/j.nuclphysa.2009.06.018
2007BE53 Nucl.Phys. A794, 132 (2007) B.Behera, T.R.Routray, A.Pradhan, S.K.Patra, P.K.Sahu Nuclear mean field and equation of state of asymmetric nuclear matter
doi: 10.1016/j.nuclphysa.2007.07.002
2007PA47 J.Phys.(London) G45, 055202 (2007);Addendum: J.Phys.(London) G45, 119401 (2007) S.P.Pattnaik, T.R.Routray, X.Vinas, D.N.Basu, M.Centelles, K.Madhuri, B.Behera Influence of the nuclear matter equation of state on the r-mode instability using the finite-range simple effective interaction
doi: 10.1088/1361-6471/aab7c5
2005BE31 Nucl.Phys. A753, 367 (2005) B.Behera, T.R.Routray, A.Pradhan, S.K.Patra, P.K.Sahu Momentum and density dependence of the isospin part of nuclear mean field and equation of state of asymmetric nuclear matter
doi: 10.1016/j.nuclphysa.2005.03.002
2002BE12 Nucl.Phys. A699, 770 (2002) B.Behera, T.R.Routray, B.Sahoo, R.K.Satpathy Momentum Dependence of the Mean Field and Equation of State of Nuclear Matter
doi: 10.1016/S0375-9474(01)01285-4
2000RO15 J.Phys.(London) G26, 887 (2000) T.R.Routray, B.Sahoo, R.K.Satpathy, B.Behera Nuclear Equation of State with Finite-Range Effective Interactions
doi: 10.1088/0954-3899/26/6/311
1998BE75 J.Phys.(London) G24, 2073 (1998) B.Behera, T.R.Routray, R.K.Satpathy Momentum and Density Dependence of the Mean Field in Nuclear Matter
doi: 10.1088/0954-3899/24/11/009
1997BE17 J.Phys.(London) G23, 445 (1997) B.Behera, T.R.Routray, R.K.Satpathy Causal Violation of the Speed of Sound and the Equation of State of Nuclear Matter
doi: 10.1088/0954-3899/23/4/005
1994BE39 J.Phys.(London) G20, 1615 (1994) Energy Density Formalism and Semiclassical Nuclear Properties
doi: 10.1088/0954-3899/20/10/008
1988BE24 J.Phys.(London) G14, 1073 (1988) A Simple Microscopic Approach to the Nuclear Giant Monopole and Quadrupole Resonances NUCLEAR STRUCTURE 16O, 40Ca, 90Zr, 120Sn, 208Pb; calculated giant monopole, quadrupole resonance energies.
doi: 10.1088/0305-4616/14/8/010
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