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NSR database version of April 29, 2024.

Search: Author = T.Malik

Found 10 matches.

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2022AD03      Phys.Rev. C 105, 015806 (2022)

S.M.Adil Imam, N.K.Patra, C.Mondal, T.Malik, B.K.Agrawal

Bayesian reconstruction of nuclear matter parameters from the equation of state of neutron star matter

doi: 10.1103/PhysRevC.105.015806
Citations: PlumX Metrics

2022MA41      Eur.Phys.J. A 58, 154 (2022)

T.Malik, H.Pais

Inner crust equations of state for CompOSE

doi: 10.1140/epja/s10050-022-00799-3
Citations: PlumX Metrics

2022MA50      Phys.Rev. C 106, L042801 (2022)

T.Malik, B.K.Agrawal, C.Providencia

Inferring the nuclear symmetry energy at suprasaturation density from neutrino cooling

doi: 10.1103/PhysRevC.106.L042801
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
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
Citations: PlumX Metrics

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
Citations: PlumX Metrics

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
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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
Citations: PlumX Metrics

2013BH07      Phys.Rev. C 88, 014313 (2013)

T.Bhattacharjee, D.Banerjee, S.K.Das, S.Chanda, T.Malik, A.Chowdhury, P.Das, S.Bhattacharyya, R.Guin

Spectroscopy of low-lying states in odd-odd ¹⁴⁶Eu

RADIOACTIVITY ¹⁴⁶Gd(EC)[from ¹⁴⁴Sm(α, 2n), E=32 MeV]; measured Eγ, Iγ, γγ-coin, level half-lives by γγ(t). ¹⁴⁶Eu; deduced levels, J, π, β feedings, logft, configurations. ¹⁵²Gd; measured half-life of 344-keV level by γγ(t). Mirror symmetric centroid difference (MSCD) method for half-life analysis. ^146,147Eu, ¹⁴⁹Gd(EC); observed γ rays. Comparison with large-basis shell-model calculations using OXBASH computer code.

doi: 10.1103/PhysRevC.88.014313
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