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NSR database version of April 11, 2024.

Search: Author = T.R.Routray

Found 24 matches.

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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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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
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1994BE39      J.Phys.(London) G20, 1615 (1994)

B.Behera, T.R.Routray

Energy Density Formalism and Semiclassical Nuclear Properties

doi: 10.1088/0954-3899/20/10/008
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1988BE24      J.Phys.(London) G14, 1073 (1988)

B.Behera, T.R.Routray

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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