English

Vacuum structure of Yang-Mills theory as a function of $\theta$

High Energy Physics - Theory 2018-09-26 v3 High Energy Physics - Phenomenology

Abstract

It is believed that in SU(N)SU(N) Yang-Mills theory observables are NN-branched functions of the topological θ\theta angle. This is supposed to be due to the existence of a set of locally-stable candidate vacua, which compete for global stability as a function of θ\theta. We study the number of θ\theta vacua, their interpretation, and their stability properties using systematic semiclassical analysis in the context of adiabatic circle compactification on R3×S1\mathbb{R}^3 \times S^1. We find that while observables are indeed N-branched functions of θ\theta, there are only N/2\approx N/2 locally-stable candidate vacua for any given θ\theta. We point out that the different θ\theta vacua are distinguished by the expectation values of certain magnetic line operators that carry non-zero GNO charge but zero 't Hooft charge. Finally, we show that in the regime of validity of our analysis YM theory has spinodal points as a function of θ\theta, and gather evidence for the conjecture that these spinodal points are present even in the R4\mathbb{R}^4 limit.

Keywords

Cite

@article{arxiv.1804.06848,
  title  = {Vacuum structure of Yang-Mills theory as a function of $\theta$},
  author = {Kyle Aitken and Aleksey Cherman and Mithat Ünsal},
  journal= {arXiv preprint arXiv:1804.06848},
  year   = {2018}
}

Comments

33 pages, 6 figures. v3: added references