TK
T. K. Jha
Birla Institute of Technology and Science, Pilani - Goa Campus, Physical Research Laboratory, Sambalpur University, Gangadhar Meher University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Pulsars and Gravitational Waves Research · Nuclear physics research studies · Quantum Chromodynamics and Particle Interactions
Employment
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Birla Institute of Technology and Science Pilani - K K Birla Goa Campus ASSOCIATE PROFESSOR2009 - Present
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Physical Research Laboratory POST DOCTORAL FELLOW2007 - 2009
Education
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Sambalpur University M.Sc.
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Gangadhar Meher College B.Sc.
Projects & Funding
Projects & funding information is unavailable.
Publications (26)
- Magnetic Field Effects on the Structure of Neutron Stars Save
- Fundamental Oscillation Modes in Neutron Stars with Hyperons and Delta Baryons Save
- Towards Uncovering Dark Matter Effects on Neutron Star Properties: A Machine Learning Approach Save
- Establishing connection between neutron star properties and nuclear matter parameters through a comprehensive multivariate analysis Save
- Effect of the σ -cut potential on the properties of neutron stars with or without a hyperonic core Save
- Effect of the σ-cut potential on the properties of neutron stars with or without a hyperonic core Save
- Hyperon bulk viscosity and r-modes of neutron stars Save
- An Equation of State for Magnetized Neutron Star Matter and Tidal Deformation in Neutron Star Mergers Save
- Effect of Λv coupling on liquid gas phase transition in warm asymmetric nuclear matter Save
- Tides in merging neutron stars: Consistency of the GW170817 event with experimental data on finite nuclei Save
- Effects of hadron–quark phase transition on properties of neutron stars Save
- Deconfinement of nonstrange hadronic matter with nucleons and Δ baryons to quark matter in neutron stars Save
- Properties of Neutron stars with hyperon cores in parametrized hydrostatic conditions Save
- GW170817: Constraining the nuclear matter equation of state from the neutron star tidal deformability Save
- Nuclear symmetry energy with mesonic cross-couplings in the effective chiral model Save
- Massive neutron stars and their implications Save
- TSALLIS STATISTICS AND THE ROLE OF A STABILIZED RADION IN THE SUPERNOVAE SN1987A COOLING Save
- Bulk viscosity in a hyperonic star andr-mode instability Save
- Constraints on nuclear matter parameters of an effective chiral model Save
- Attributes of a rotating neutron star with a hyperon core Save