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Semi-Universality of O(N)O(N) model on S1×S2S^1\times S^2

Published 22 Sep 2026 in hep-th | (2609.25622v1)

Abstract: We study the thermal partition function of the critical large-NN O(N)O(N) model on rotating S<sup>1×</sup>S<sup>2S<sup>1\times</sup> S<sup>2. Rotation makes the saddle latitude dependent, with its leading profile governed by the local temperature. Using a Weyl-covariant hydrostatic expansion, we determine the partition function through four-derivative order in high-temperature and semi-universal limits. In the near-light-speed limit, the geometry around the equator reduces to a pp-wave and captures the expected semi-universal behavior of the partition function. We compute the corresponding theory-dependent residue directly on this limiting geometry, both at high and low temperatures. The high-temperature result agrees with the near-light-speed limit of the sphere calculation, while the low-temperature expansion reveals interaction-dependent corrections arising from the response of the saddle to the thermal source.

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