We discuss the machine-learning inference and uncertainty quantification for the equation of
state (EOS) of the neutron star matter directly using the NS probability distribution from the …

Deconfined quark matter at asymptotically high densities is weakly coupled, due to the
asymptotic freedom of quantum chromodynamics. In this weak-coupling regime, bulk …

Nonperturbative inequalities constrain the thermodynamic pressure of quantum
chromodynamics (QCD) with its phase-quenched version, a sign-problem-free theory …

Measurements of neutron star masses, radii, and tidal deformability have direct connections
to nuclear physics via the equation of state (EoS), which for the cold, catalyzed matter in …

Recent inference results of the sound velocity in the cores of neutron stars are summarized.
Implications for the equation of state and the phase structure of highly compressed baryonic …

The past years have witnessed tremendous progress in understanding the properties of
neutron stars and of the dense matter in their cores, made possible by electromagnetic …

I explore various scenarios for the phase transition within neutron-star matter. I do so by
generating large model-agnostic ensemble using Gaussian processes, both with and …

Abstract PSR J2215+ 5135 (J2215) is a" redback" spider pulsar, where the intrabinary shock
(IBS) wraps around the pulsar rather than the stellar-mass companion. Spider orbital light …

We investigate the behavior of the dense and cold (normalized) quantum chromodynamics
(QCD) trace anomaly, Δ, in the interior of twin neutron stars (obtained from several sets of …

Understanding the properties and physical phase of the dense strongly interacting matter
present in the cores of neutron stars or created in their binary mergers remains one of the …