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astro-ph.HE2024
Causality and perturbative-QCD constraints on first-order phase transitions in neutron stars
Asim kumar Saha, Ritam Mallick
Causality bounds the compactness and maximum mass of neutron stars. We generalise this bound to equations of state (EOSs) with a first-order phase transition between maximally stif…
astro-ph.SR2024
The prospect of confining the equation of state of neutron star with future mass and radius measurement
Asim Kumar Saha, Ritam Mallick
Simultaneous measurement of mass and radius with high precision is essential to unravel the equation of state of matter at the centre of neutron stars. Measurement of massive pulsa…