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Polyakov loop

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Through Temperature, Potential energy and Topology

Definition

Thermal quantum field theory is formulated in Euclidean spacetime with a compactified imaginary temporal direction of length β. This length corresponds to the inverse temperature of the field β∝1/T. Compactification leads to a special class of topologically nontrivial Wilson loops that wind around the compact direction known as Polyakov loops. In SU(N) theories a straight Polyakov loop on a spatial coordinate x is given by

Φ(x)=1NtrPexp⁡[∫0βdx4A4(x,xf)],

where P is the path-ordering operator and A4 is the Euclidean temporal component of the gauge field. In lattice field theory this operator is reformulated in terms of temporal link fields U4(m,j) at a spatial position m as

Φ(m)=1Ntr[∏j=0NT−1U4(m,j)].

The continuum limit of the lattice must be taken carefully to ensure that the compact direction has fixed extent. This is done by ensuring that the finite number of temporal lattice points NT is such that β=NTa is constant as the lattice spacing a goes to zero.

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