出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:We show that high-temperature perturbation theory describes extremely well the area law of
SU(N) spatial ’t Hooft loops, or equivalently the tension of the interface between different ZN
vacua in the deconfined phase. For SU(2), the disagreement between Monte Carlo data and
lattice perturbation theory for s˜ (T)=T2 is less than 2%, down to temperatures O(10) Tc. For
SU(N);N > 3, the ratios of interface tensions, (s˜k=s˜1)(T), agree with perturbation theory, which
predicts tiny deviations from the ratio of Casimirs, down to nearly Tc. In contrast, individual tensions
differ markedly from the perturbative expression. In all cases, the required precision Monte
Carlo measurements are made possible by a simple but powerful modification of the ’snake’ algorithm.