Bijay Agrawal
Also known as: B. K. Agrawal
SINP, Utkal University, Institute of Physics Bhubaneswar, Kurukshetra University
About
Prof. Bijay Agrawal. Completed the Doctor of Philosophy in P. HD in 1996/01 by Utkal University, Master in M. Sc. in 1988 by Kurukshetra University, Postgraduate Certificate in Post M. Sc. (Physics) in 1989 by Institute of Physics Bhubaneswar, and Bachelor in B. Sc. in 1986 by Kurukshetra University. Is Full Professor at Saha Institute of Nuclear Physics. Published 89 articles in journals. Works in the area(s) of Exact Sciences with emphasis on Physical Sciences with emphasis on Nuclear Physics. Broadly, he works in the domain of theoretical Nuclear Astrophysics, particularly the physics of dense matter relevant for a neutron star. His present interests focus on the understanding of neutron stars and the determination of constraints on the equation of state of dense hadronic matter. He has expertise in relativistic mean-field (RMF) models for both finite nuclei and infinite nuclear matter. He also worked to constrain the values of various nuclear matter parameters that predominantly govern the behavior of the EOS through their correlations with the properties of the neutron stars such as radii, tidal deformability, and maximum mass of the neutron stars. Recently his considerable effort in developing statistical tools combined with high-performance computing solutions to solve the demanding task of constraining the EOS of nuclear matter.
Employment
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SINP Sr. Professor
Education
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Utkal University Ph. D.? - 1996
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Institute of Physics Bhubaneswar Post M. Sc.? - 1989
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Kurukshetra University M.Sc? - 1988
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Kurukshetra University B. Sc.? - 1986
Projects & Funding
Projects & funding information is unavailable.
Publications (90)
- Bayesian reconstruction of nuclear matter parameters from the equation~of state of neutron star matter Save
- Nuclear level densities away from line of \ensuremathβ-stability Save
- Relativistic description of dense matter equation of state and compatibility with neutron star observables: a Bayesian approach Save
- Constraining nuclear matter parameters from correlation systematics: a mean-field perspective Save
- Empirical constraints on the high-density equation of state from multimessenger observables Save
- Pairing, quasi-spin and seniority Save
- Unveiling the correlations of tidal deformability with the nuclear symmetry energy parameters Save
- A systematic study of the factors affecting central depletion in nuclei Save
- Anti-bubble effect of temperature \& deformation: a systematic study for nuclei across all mass regions between A $=$ 20$-$300 Save
- Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei Save