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 · Bharat Kumar · S. K. Patra
May 31, 2018#1nucl-thPRC296 citations
Author
Kumar, Bharat
INSPIRE profile1851815ORCID0000-0003-1964-057X
7 papers·1,560 citations in this corpus
New relativistic effective interaction for finite nuclei, infinite nuclear matter and neutron stars
Bharat Kumar🇮🇳 · S. K. Patra🇮🇳 · B. K. Agrawal🇮🇳
Nov 15, 2017#15nucl-thPRC152 citations
Relative mass distributions of neutron-rich thermally fissile nuclei within statistical model
Bharat Kumar · M.T. Senthil kannan · M. Balasubramaniam · B. K. Agrawal · S. K. Patra
Apr 27, 2017#6nucl-thPRC7 citations
Ternary fission within the temperature dependent relativistic mean field approach
M.T. Senthil Kannan · Bharat Kumar · M. Balasubramaniam · B. K. Agrawal · S. K. Patra
Dec 7, 2016#2nucl-thPRC11 citations
Tidal deformability of neutron and hyperon star with relativistic mean field equations of state
Bharat Kumar🇮🇳 · S. K. Biswal🇮🇳 · S. K. Patra🇮🇳
Sep 29, 2016#3nucl-thPRC71 citations
Properties of superheavy nuclei with Z = 124
M. S. Mehta · Harvinder Kaur · Bharat Kumar · S. K. Patra
Oct 29, 2015#5nucl-thPRC21 citations
Examining the stability of thermally fissile Th and U isotopes
Bharat Kumar · S. K. Biswal · S. K. Singh · S. K. Patra
Aug 4, 2015#2nucl-thPRC11 citations
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