15 citations · 61 across the 7 of their papers we have counts for
7 papers
Density-induced dark-baryon conversion in admixed hypernuclear neutron stars
Niyar Prabhat Kalita, Vivek Baruah Thapa, Bhanu Prakash Pant +2
We investigate density-induced conversion of neutrons into a neutral dark baryon in cold, charge-neutral, -equilibrated neutron-star matter containing hyperons and all $Δ(12…
Modeling large glitches with core superfluidity in a Hybrid star
Yogeesh N., Anil Kumar, Monika Sinha
Many pulsars exhibit a peculiar behaviour in their pulse profile of a sudden increase in their rotational period, which is popularly known as a pulsar glitch. Some of them show gia…
Imprints of Non-Symmetric Dark Matter Halos on Magnetars: A Two-Fluid Perspective
Asit karan, Anil Kumar, Monika Sinha +1
In this study, we investigate the impact of dark matter on the structure and deformation of magnetars. We assume a perturbative approach for the magnetic field deformation and that…
Bayesian Inference of dense matter equation of state of neutron star with antikaon condensation
Vishal Parmar, Vivek Baruah Thapa, Anil Kumar +2
In this paper, we employ the Density Dependent Relativistic Hadron (DDRH) field theoretical Model in a Bayesian analysis to investigate the equation of state (EOS) of dense matter…
Exploring non-radial oscillation modes in dark matter admixed neutron stars
Pratik Thakur, Anil Kumar, Vivek Baruah Thapa +2
Because of their extreme densities and consequently, gravitational potential, compact objects such as neutron stars can prove to be excellent captors of dark matter particles. Cons…
Non-radial oscillations in newly born compact star considering effects of phase transition
Anil Kumar, Pratik Thakur, Monika Sinha
The massive stars end their lives by supernova explosions leaving central compact objects that may evolve into neutron stars. Initially, after birth, the star remains hot and gradu…
Universal relations for compact stars with exotic degrees of freedom
Anil Kumar, Manoj Kumar Ghosh, Pratik Thakur +2
The nature of the highly dense matter inside the supernova remnant compact star is not constrained by terrestrial experiments and hence modeled phenomenologically to accommodate th…