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NSR database version of May 2, 2024.

Search: Author = S.P.Pattnaik

Found 5 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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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
Citations: PlumX Metrics

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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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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