The free energy of the large-N fermionic Chernx2013Simons theory in the 'temporal' gauge

Abstract

Most of the computational evidence for the Bosex2013Fermi duality of fundamental fields coupled to U(N) Chernx2013Simons theories originates in large-N calculations performed in the light-cone gauge. This gauge is ill-suited to computations in curved spacetimes, like the evaluation of the partition function on g× S1 for arbitrary genus g. In this paper, we use another gauge, the 'temporal' gauge, to set up the computation of this partition function. In the large-N limit, and the special case g=R2, we take the computation through to the end by setting up and solving the gap equations, generalizing tricks explored in arXiv:1410.0558 to finite temperature. Our final results are in perfect agreement with earlier light-cone gauge results, providing a consistency check of both the formalism developed in this paper as well as previously performed light-cone gauge computations. In a follow-up paper, we will report on using our formalism to explicitly compute the partition function on S2 × S1 for a finite-sized sphere.

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