On the rotator Hamiltonian for the SU$(N)\times$SU$(N)$ sigma-model in the delta-regime

Abstract

We investigate some properties of the standard rotator approximation of the SU$(N)\times$SU$(N)$ sigma-model in the delta-regime. In particular we show that the isospin susceptibility calculated in this framework agrees with that computed by chiral perturbation theory up to next-to-next to leading order in the limit $\ell =L_t/L\to \infty .$ The difference between the results involves terms vanishing like $1/\ell ,$ plus terms vanishing exponentially with $\ell$. As we have previously shown for the O($n$) model, this deviation can be described by a correction to the rotator spectrum proportional to the square of the quadratic Casimir invariant. Here we confront this expectation with analytic nonperturbative results on the spectrum in 2 dimensions for $N=3.$

36 pages, 2 figures