pith. sign in

arxiv: 1103.2315 · v3 · pith:WRQNPA2Gnew · submitted 2011-03-11 · ✦ hep-th · hep-lat

Holographic Roberge-Weiss Transitions II: Defect Theories and the Sakai-Sugimoto Model

classification ✦ hep-th hep-lat
keywords theoriesdefectmodelmodelsroberge-weisssakai-sugimototransitionstemperature
0
0 comments X
read the original abstract

We extend the work of Aarts et al., including an imaginary chemical potential for quark number into the Sakai-Sugimoto model and codimension k defect theories. The phase diagram of these models are a function of three parameters, the temperature, chemical potential and the asymptotic separation of the flavour branes, related to a mass for the quarks in the boundary theories. We compute the phase diagrams and the pressure due to the flavours of the theories as a function of these parameters and show that there are Roberge-Weiss transitions in the high temperature phases, chiral symmetry restored for the Sakai-Sugimoto model and deconfined for the defect models, while at low temperatures there are no Roberge-Weiss transitions. In all the models we consider the transitions between low and high temperature phases are first order, hence the points where they meet the Roberge-Weiss lines are triple points. The pressure for the defect theories scales in the way we expect from dimensional analysis while the Sakai-Sugimoto model exhibits unusual scaling. We show that the models we consider are analytic in \mu^2 when \mu^2 is small.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. The Roberge-Weiss transition as a probe for conformality in many-flavor QCD

    hep-lat 2026-04 unverdicted novelty 7.0

    For eight-flavor QCD the Roberge-Weiss transition temperature vanishes in the chiral limit, placing the theory inside the conformal window.