On the origin of the $Nc^1$ scaling in the confined but chirally symmetric phase at high T
L. Ya. Glozman

TL;DR
This paper explains the Nc^1 scaling of energy density in high-temperature, confined, chirally symmetric QCD matter by using a large Nc model, showing that dense, overlapping meson-like states dominate this phase.
Contribution
It provides a theoretical explanation for the Nc^1 scaling in the stringy fluid phase using a solvable large Nc model, linking it to meson-like state fluctuations.
Findings
Energy density scales as Nc^1 in the stringy fluid phase.
Meson-like states become infinitely large at chiral restoration.
Excitation energies of quark-antiquark systems are Nc-independent.
Abstract
There is lattice evidence that the QCD matter above the chiral restoration temperature Tch and below the deconfinement temperature Td, called stringy fluid, is characterized by an approximate chiral spin symmetry, which is a symmetry of confinement in QCD with light quarks. The energy density, pressure and entropy density in the stringy fluid scale as Nc^1, which is in contrast to the Nc^0 scaling in the hadron gas and to the Nc^2 scaling in the quark-gluon plasma. Here we clarify the origin of the Nc^1 scaling. We employ a solvable field-theoretical large chirally symmetric and confining model. In vacuum the confining potential induces a spontaneous breaking of chiral symmetry. The mesons are spatially localized states of quarks and antiquarks. Still in the confining regime the system undergoes the chiral restoration phase transition at because of Paili blocking of the…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
