Wiener-Hopf solution of the free energy TBA problem and instanton sectors in the O(3) sigma model.

Perturbation theory in asymptotically free quantum field theories is asymptotic. The factorially growing perturbative coefficients carry information about non-perturbative corrections, which can be related to renormalons and instantons. Using the Wiener-Hopf technique we determine the full analytic solution for the free energy density in the two dimensional O(N) sigma models. For N > 3 there are no instantons, and we found that the perturbative series carries all the information about the non-perturbative corrections. However, in the O(3) case, we identify several non-perturbative sectors that are not related to the asymptotics of the perturbative series. The number of sectors depends on the observables: for the ground-state energy density we identify three sectors, which we attribute to instantons. For the free energy density in the running perturbative coupling we found infinitely many sectors. [ABSTRACT FROM AUTHOR]