86 citations · 334 across the 22 of their papers we have counts for
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Masses of Heavy Quarkonium states in magnetized matter -- effects of PV mixing and (inverse) magnetic catalysis
Ankit Kumar, Amruta Mishra
We study the in-medium masses of the heavy quarkonium (charmonium and bottomonium) states in isospin asymmetric nuclear matter in presence of an external magnetic field. The mass m…
QCD sum rule analysis of Heavy Quarkonium states in magnetized matter -- effects of (inverse) magnetic catalysis
Pallabi Parui, Sourodeep De, Ankit Kumar +1
The masses of the and states of heavy quarkonia are investigated in the magnetized, asymmetric nuclear medium, accounting for the Dirac sea effects, using a combined appr…
Continuous-Variable Entanglement through Central Forces: Application to Gravity between Quantum Masses
Ankit Kumar, Tanjung Krisnanda, P. Arumugam +1
We describe a complete method for a precise study of gravitational interaction between two nearby quantum masses. Since the displacements of these masses are much smaller than the…
Pasta properties of the neutron star within effective relativistic mean-field model
Vishal Parmar, H. C. Das, Ankit Kumar +3
We study the properties of pasta structures and their influence on the neutron star observables employing the effective relativistic mean-field (E-RMF) model. The compressible liqu…
Thermal Relaxation of Dark Matter Admixed Neutron Star
Ankit Kumar, H. C. Das, S. K. Patra
Motivated by the various theoretical studies regarding the efficient capturing of dark matter by neutron stars, we explore the possible indirect effects of captured dark matter on…
Constraining the parameterized neutron star equation of state with astronomical observations
Jaikhomba Singha, S. Mullai Vaneshwar, Ankit Kumar
We utilise the phenomenologically parameterized piecewise polytropic equations of state to study various neutron star properties. We investigate the compliance of these equations o…
Dark Matter Effects on the Compact Star Properties
H. C. Das, Ankit Kumar, Bharat Kumar +1
The neutron star properties are generally determined by the equation of state of -equilibrated dense matter. In this work, we consider the interaction of fermionic dark matter (…