The drag force on a heavy quark in a rotating finite-density holographic plasma is purely tangential and anisotropic, with worldsheet regularity fixing the renormalised transverse force and selecting a co-rotating equilibrium in the equal-spin sector.
Heavy-Quark Potentials and AdS/QCD
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
abstract
We give an example of modeling phenomenological heavy-quark potentials in a five-dimensional framework nowadays known as AdS/QCD. In particular we emphasize the absence of infrared renormalons.
citation-role summary
background 1
method 1
citation-polarity summary
verdicts
UNVERDICTED 3representative citing papers
A physics-guided neural network embedding AdS5 Dirac equation and holographic Pomeron fits SLAC proton F2 data with chi-squared per degree of freedom of 0.91 and identifies a kinematic crossover at x approximately 0.19 while recovering Pomeron intercept of 1.0786.
Time-dependent holographic entanglement entropy and complexity are computed perturbatively for braneworld FLRW universes with radiation, matter, and exotic matter by using time-dependent brane positions in black brane bulk geometries.
citing papers explorer
-
Anisotropic drag force in finite-density QGP from charged rotating 5D black holes
The drag force on a heavy quark in a rotating finite-density holographic plasma is purely tangential and anisotropic, with worldsheet regularity fixing the renormalised transverse force and selecting a co-rotating equilibrium in the equal-spin sector.
-
Probing Proton Structure via Physics-Guided Neural Networks in Holographic QCD
A physics-guided neural network embedding AdS5 Dirac equation and holographic Pomeron fits SLAC proton F2 data with chi-squared per degree of freedom of 0.91 and identifies a kinematic crossover at x approximately 0.19 while recovering Pomeron intercept of 1.0786.
-
Holographic entanglement entropy and complexity for the cosmological braneworld model
Time-dependent holographic entanglement entropy and complexity are computed perturbatively for braneworld FLRW universes with radiation, matter, and exotic matter by using time-dependent brane positions in black brane bulk geometries.