In this review, we provide an up-to-date account of quantitative bottom-up holographic
descriptions of the strongly coupled quark–gluon plasma (QGP) produced in relativistic …

In this paper we provide a first physical interpretation for the Event Horizon Telescopeʼs
(EHT) 2017 observations of Sgr A*. Our main approach is to compare resolved EHT data at …

Astrophysical black holes are expected to be described by the Kerr metric. This is the only
stationary, vacuum, axisymmetric metric, without electromagnetic charge, that satisfies …

Relativistic dissipative fluid dynamics finds widespread applications in high-energy nuclear
physics and astrophysics. However, formulating a causal and stable theory of relativistic …

We present the first generalization of Navier-Stokes theory to relativity that satisfies all of the
following properties:(a) the system coupled to Einstein's equations is causal and strongly …

In this paper we provide a first physical interpretation for the Event Horizon Telescope's
(EHT) 2017 observations of Sgr A*. Our main approach is to compare resolved EHT data at …

The Event Horizon Telescope (EHT) has opened a new window on supermassive black
holes. With the advent of millimeter and submillimeter very long baseline interferometry …

We investigate the impact of a mean field model for the α Ω dynamo potentially active in the
postmerger phase of a binary neutron star coalescence. We do so by deriving equations for …

Hydrodynamics can be formulated in terms of a perturbative series in derivatives of the
temperature, chemical potential, and flow velocity around an equilibrium state. Different …

In nuclear matter in neutron stars the flavor content (eg, proton fraction) is subject to weak
interactions, establishing flavor (β-) equilibrium. During the merger of two neutron stars there …