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NSR database version of April 27, 2024.

Search: Author = T.K.Jha

Found 14 matches.

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2024TH01      Phys.Rev. C 109, 025805 (2024)

P.Thakur, B.K.Sharma, A.Ashika, S.Srivishnu, T.K.Jha

Influence of the symmetry energy and σ-cut potential on the properties of pure nucleonic and hyperon-rich neutron star matter

doi: 10.1103/PhysRevC.109.025805
Citations: PlumX Metrics


2022PA35      Phys.Rev. C 106, 055806 (2022)

N.K.Patra, B.K.Sharma, A.Reghunath, A.K.H.Das, T.K.Jha

Effect of the σ-cut potential on the properties of neutron stars with or without a hyperonic core

doi: 10.1103/PhysRevC.106.055806
Citations: PlumX Metrics


2020SH23      Nucl.Phys. A1002, 121974 (2020)

B.K.Sharma, S.Sathees, M.K.Meghaa, T.K.Jha

Effect of Λμ coupling on liquid gas phase transition in warm asymmetric nuclear matter

doi: 10.1016/j.nuclphysa.2020.121974
Citations: PlumX Metrics


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
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2018MA58      Phys.Rev. C 98, 035804 (2018)

T.Malik, N.Alam, M.Fortin, C.Providencia, B.K.Agrawal, T.K.Jha, B.Kumar, S.K.Patra

GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability

doi: 10.1103/PhysRevC.98.035804
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2017MA56      Phys.Rev. C 96, 035803 (2017)

T.Malik, K.Banerjee, T.K.Jha, B.K.Agrawal

Nuclear symmetry energy with mesonic cross-couplings in the effective chiral model

doi: 10.1103/PhysRevC.96.035803
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2010JH01      Phys.Rev. C 82, 025803 (2010)

T.K.Jha, H.Mishra, V.Sreekanth

Bulk viscosity in a hyperonic star and r-mode instability

doi: 10.1103/PhysRevC.82.025803
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2008JH02      Phys.Rev. C 77, 045801 (2008)

T.K.Jha, H.Mishra, V.Sreekanth

Attributes of a rotating neutron star with a hyperon core

doi: 10.1103/PhysRevC.77.045801
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2008JH03      Phys.Rev. C 78, 065802 (2008)

T.K.Jha, H.Mishra

Constraints on nuclear matter parameters of an effective chiral model

doi: 10.1103/PhysRevC.78.065802
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2006JH02      Phys.Rev. C 74, 055803 (2006); Erratum Phys.Rev. C 75, 029903 (2007)

T.K.Jha, P.K.Raina, P.K.Panda, S.K.Patra

Neutron star matter in an effective model

doi: 10.1103/PhysRevC.74.055803
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2004ME13      Pramana 62, 841 (2004)

M.S.Mehta, T.K.Jha, S.K.Patra, R.K.Gupta

Potential energy surfaces for N = Z, 20Ne-112Ba nuclei

NUCLEAR STRUCTURE 20Ne, 24Mg, 28Si, 32S, 36Ar, 40Ca, 44Ti, 48Cr, 52Fe, 56Ni, 60Zn, 64Ge, 68Se, 72Kr, 76Sr, 80Zr, 84Mo, 88Ru, 92Pd, 96Cd, 100Sn, 104Te, 108Xe, 112Ba; calculated energy vs deformation. Deformed relativistic mean field approach.

doi: 10.1007/BF02706133
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2004NA22      Pramana 62, 827 (2004)

Z.Naik, B.K.Sharma, T.K.Jha, P.Arumugam, S.K.Patra

Shape change in Hf, W and Os-isotopes: A non-relativistic Hartree-Fock versus relativistic Hartree approximation

NUCLEAR STRUCTURE Hf, W, Os; calculated binding energies, quadrupole deformation parameters. Comparison of relativistic and nonrelativistic approaches.

doi: 10.1007/BF02706132
Citations: PlumX Metrics


2004SA08      Nucl.Phys. A733, 169 (2004)

P.K.Sahu, T.K.Jha, K.C.Panda, S.K.Patra

Hot nuclear matter in asymmetry chiral sigma model

doi: 10.1016/j.nuclphysa.2003.11.061
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2003JH01      Pramana 61, 517 (2003)

T.K.Jha, M.S.Mehta, S.K.Patra, B.K.Raj, R.K.Gupta

A relativistic mean-field study of magic numbers in light nuclei from neutron to proton drip-lines

NUCLEAR STRUCTURE 11Li, 12Be, 13B, 14,20,22C, 15,23N, 16,24O, 17,25F, 18,26Ne, 19,27Na, 20,28Mg; calculated single-particle level energies; A=4-44; calculated one- and two-neutron separation energies; deduced shell closure and drip-line features.

doi: 10.1007/BF02705475
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