activity
20142025
most citedHybrid stars in the light of GW170817

98 citations · 734 across the 33 of their papers we have counts for

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Showing astro-ph.HEShow all

19 papers · 1 filter

astro-ph.HE2025

Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State

Bhaskar Biswas, Prasanta Char

We present new constraints on the neutron star equation of state (EOS) and mass distribution using a unified Bayesian inference framework that incorporates latest NICER measurement…

astro-ph.HE2025★ 4 cited

Stellar properties indicating the presence of hyperons in neutron stars

Andreas Bauswein, Aristeidis Nikolaidis, Georgios Lioutas +7

We describe distinctive stellar features indicating the presence of hyperons in neutron stars as compared to purely nucleonic systems. A strongly negative curvature of the mass-rad…

astro-ph.HE2024

Structural response of neutron stars to rapid rotation and its impact on the braking index

Avishek Basu, Prasanta Char, Rana Nandi

Pulsars are rotating neutron stars that are observed to be slowing down, implying a loss of their rotational energy. There can be several different physical mechanisms involved in…

astro-ph.HE2024★ 2 cited

Compact object of HESS J1731-347 and its implication on neutron star matter

Prasanta Char, Bhaskar Biswas

In this work, we investigate the impact of the possibility of a small, subsolar mass compact star, such as the recently reported central compact object of HESS J1731-347, on the eq…

astro-ph.HE2021★ 17 cited

Speed of sound in dense matter and two families of compact stars

Silvia Traversi, Prasanta Char, Giuseppe Pagliara +1

The existence of massive compact stars implies that the conformal limit of the speed of sound is violated if those stars have a crust of ordi…

astro-ph.HE2020★ 63 cited

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…