Research Projects

As PI

Neutron Stars as potential continuous gravitational wave emitter . (DAE-BRNS 2013-16)
Project Outcome:
1. GW170817: constraining the nuclear matter equation of state from the neutron star tidal deformability, by Tuhin Malik, N. Alam, M. Fortin, C. Providência, B.K. Agrawal, T.K. Jha, Bharat Kumar, S.K. Patra. Published in Phys.Rev. C 98, 035804 (2018).
2. Nuclear symmetry energy with mesonic cross couplings in the effective chiral model by Tuhin Malik, Kinjal Banerjee, T. K. Jha and B. K. Agrawal. Phys.Rev. C 96, 035803 (2017).
3. Massive Neutron stars and their Implication by T K Jha and Keshab C. Panda. Pramana 82 (2014) 831 [Conference]

As PI

Detectable continuous gravitational waves (CWG) from rapidly rotating Neutron stars. (BITS Research Initiation Grant 2012-13)

As Co-PI

Aspects of some astrophysical systems like supernovae and neutron stars in the light of new physics. (DAE BRNS)

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