98 citations · 734 across the 33 of their papers we have counts for
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GW190814: On the properties of the secondary component of the binary
Bhaskar Biswas, Rana Nandi, Prasanta Char +2
We show that the odds of the mass-gap (secondary) object in GW190814 being a neutron star (NS) improve if one allows for a stiff high-density equation of state (EoS) or a large spi…
Towards mitigation of apparent tension between nuclear physics and astrophysical observations by improved modeling of neutron star matter
Bhaskar Biswas, Prasanta Char, Rana Nandi +1
Observations of neutron stars (NSs) by the LIGO-Virgo and NICER collaborations have provided reasonably precise measurements of their various macroscopic properties. In this paper,…
Structure of Quark Star: A Comparative Analysis of Bayesian Inference and Neural Network Based Modeling
Silvia Traversi, Prasanta Char
In this work, we compare two powerful parameter estimation methods namely Bayesian inference and Neural Network based learning to study the quark matter equation of state with cons…
Bayesian Inference of Dense Matter Equation of State within Relativistic Mean Field Models using Astrophysical Measurements
Silvia Traversi, Prasanta Char, Giuseppe Pagliara
We present a Bayesian analysis to constrain the equation of state of dense nucleonic matter by exploiting the available data from symmetric nuclear matter at saturation and from ob…