Bharat Kumar
Bharat Kumar
University of Tsukuba, Japan
Verified email at iopb.res.in - Homepage
TitleCited byYear
GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability
Tuhin Malik, N. Alam, M. Fortin, C. ProvidÍncia, B. K. Agrawal, T. K. Jha ...
Phys. Rev. C 98 98 (2018), 035804, 2018
632018
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
162018
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
142015
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
122017
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
122015
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
32017
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
32016
Inferring neutron star properties from GW170817 with universal relations
B Kumar, P Landry
Phys. Rev. D 99 (2019), 123026, 2019
22019
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
12016
Curvature of a neutron star
B Kumar, SK Biswal, SK Patra
Proceedings of the DAE-BRNS Symp. on Nucl. Phys 61 (2016), 916, 2016
12016
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
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Articles 1–20