GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability Tuhin Malik, N. Alam, M. Fortin, C. Providência, B. K. Agrawal, T. K. Jha ... Phys. Rev. C 98 98 (2018), 035804, 2018 | 63 | 2018 |

New relativistic effective interaction for finite nuclei, infinite nuclear matter, and neutron stars Bharat Kumar, S. K. Patra, and B. K. Agrawal Phys. Rev. C 97 (2018), 045806, 2018 | 16 | 2018 |

Tidal deformability of neutron and hyperon star with relativistic mean field equations of state Bharat Kumar, S. K. Biswal and S. K. Patra Physical Review C 95 (2017), 015801, 2017 | 16* | 2017 |

Properties of superheavy nuclei with Z = 124 M .S. Mehta,Harvinder Kaur, Bharat Kumar and S. K. Patra Physical Review C 92 (2015), 054305, 2015 | 14 | 2015 |

New parameterization of the effective field theory motivated relativistic mean field model Bharat Kumar, S. K. Singh, B. K. Agrawal, S. K. Patra Nucl. Phys. A 966 (2017), 197, 2017 | 12 | 2017 |

Shape co-existence and Parity doublet in Zr isotopes Bharat Kumar,S. K. Singh and S. K. Patra International Journal of Modern Physics E 24 (2015), 1550017, 2015 | 12 | 2015 |

Examining the stability of thermally fissile Th and U isotopes Bharat Kumar, S. K. Biswal, S. K. Singh and S. K. Patra Physical Review C 92 (2015), 054314, 2015 | 11* | 2015 |

Constraints on the moment of inertia of PSR J0737-3039 from GW170817 Philippe Landry, and Bharat Kumar The Astrophysical Journal Letters 868 (2018), L22, 2018 | 10* | 2018 |

Ternary fission within the temperature dependent relativistic mean field approach M.T. Senthil kannan , Bharat Kumar , M. Balasubramaniam, B. K. Agrawal , and ... Phys. Rev. C 95 (2017), 064613, 2017 | 4* | 2017 |

Relative mass distributions of neutron-rich thermally fissile nuclei within a statistical model Bharat Kumar, M. T. Senthil Kannan, M. Balasubramaniam, B. K. Agrawal, and S ... Phys. Rev. C 96 (2017), 034623, 2017 | 3 | 2017 |

Effects of isovector scalar meson on neutron star both with and without hyperon SK Biswal, B Kumar, SK Patra International Journal of Modern Physics E 11 ((2016), 1650090, 2016 | 3 | 2016 |

Inferring neutron star properties from GW170817 with universal relations B Kumar, P Landry Phys. Rev. D 99 (2019), 123026, 2019 | 2 | 2019 |

Modes of decay in neutron-rich nuclei Bharat Kumar , S. K. Biswal, S. K. Singh, Chirashree Lahiri and S. K. Patra International Journal of Modern Physics E 25 (2016), 1650020, 2016 | 2* | 2016 |

Quest for magicity in hypernuclei M Ikram, B Kumar, SK Biswal, SK Patra arXiv preprint arXiv:1607.04865, 2016 | 1 | 2016 |

Curvature of a neutron star B Kumar, SK Biswal, SK Patra Proceedings of the DAE-BRNS Symp. on Nucl. Phys 61 (2016), 916, 2016 | 1 | 2016 |

Analysis of parity doublet in medium mass nuclei Bharat Kumar, S. K. Singh and S. K. Patra Proceedings of the DAE Symp. on Nucl. Phys. 59, 2014 | 1* | 2014 |

GW170817 constraints on the properties of a neutron star in the presence of WIMP dark matter Abdul Quddus, Grigorios Panotopoulos, Bharat Kumar, Shakeb Ahmad, S. K. Patra arXiv:1902.00929, 2019 | | 2019 |

Theoretical studies on structural and decay properties of Z=119 superheavy nuclei M. Ikram, Asloob A. Rather, A. A. Usmani, Bharat Kumar, S. K. Patra arXiv:1709.07311, 2017 | | 2017 |

Effective relativistic mean field model for finite nuclei and neutron stars Bharat Kumar, B. K. Agrawal, S. K. Patra DAE nuclear physics conference Dec. 2017, 2017 | | 2017 |

A Study of Multi- Λ Hypernuclei within Spherical Relativistic Mean-field Approach Asloob A. Rather, M. Ikram, A. A. Usmani, Bharat Kumar, S. K. Patra arXiv:1708.00409, 2017 | | 2017 |