English

Collective Excitations in Hot QCD Plasma

Nuclear Theory 2017-12-19 v3 High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

We study the long wavelength excitations in rotating QCD fluid in presence of an external magnetic field at finite vector and axial charge densities. We consider the fluctuations of vector and axial charge currents coupled to energy and momentum fluctuations and compute the SO(3)SO(3) covariant dispersion relations of the six corresponding hydrodynamic modes. Among them, there are always two scalar Chiral Magnetic-Vortical-Heat (CMVH) waves; In the absence of magnetic field (vorticity) these waves reduce to CVH (CMH) waves. While CMVH waves are the mixed of CMH and CVH waves, they have generally different velocities compared to the sum of velocities of the latter waves. The other four modes, which are made out of scalar-vector fluctuations, are mixed Sound-Alfv\'en waves. We show that in the direction parallel to both magnetic field and vorticity, these four modes are the two ordinary sound modes together with two Chiral Alfv\'en waves (CAW).

Cite

@article{arxiv.1612.08614,
  title  = {Collective Excitations in Hot QCD Plasma},
  author = {Navid Abbasi and Davood Allahbakhshi and Ali Davody and Seyed Farid Taghavi},
  journal= {arXiv preprint arXiv:1612.08614},
  year   = {2017}
}

Comments

34 pages, 3 figures, 4 tables, v2: one table removed, anomalous transport coefficients corrected, a subsection on Chiral Heat Wave added, references added, v3: PRD version

R2 v1 2026-06-22T17:35:07.804Z