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KMS Spectra for Group Actions on Compact Spaces

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Abstract

Given a topologically free action of a countable group G on a compact metric space X, there is a canonical correspondence between continuous 1-cocycles for this group action and diagonal 1-parameter groups of automorphisms of the reduced crossed product C\(^*\)-algebra. The KMS spectrum is defined as the set of inverse temperatures for which there exists a KMS state. We prove that the possible KMS spectra depend heavily on the nature of the acting group G. For groups of subexponential growth, we prove that the only possible KMS spectra are \(\{0\}\), \([0,+\infty )\), \((-\infty ,0]\) and \({\mathbb {R}}\). For certain wreath product groups, which are amenable and of exponential growth, we prove that any closed subset of \({\mathbb {R}}\) containing zero arises as KMS spectrum. Finally, for certain nonamenable groups including the free group with infinitely many generators, we prove that any closed subset may arise. Besides uncovering a surprising relation between geometric group theoretic properties and KMS spectra, our results provide two simple C\(^*\)-algebras with the following universality property: any closed subset (containing, resp. not containing zero) arises as the KMS spectrum of a 1-parameter group of automorphisms of this C\(^*\)-algebra.

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Acknowledgements

The proof of Theorem A uses unpublished ideas developed by Klaus Thomsen and the first named author while working on [CT19], which handles the special case \(G={\mathbb {Z}}\). We are grateful to Klaus Thomsen for allowing us to include them in this article, and for discussions leading to the results in Sect. 5.

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Correspondence to Stefaan Vaes.

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Communicated by Y.  Ogata.

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Johannes Christensen Supported by a DFF-International Postdoctoral Grant. Stefaan Vaes Supported by FWO research project G090420N of the Research Foundation Flanders and by long term structural funding—Methusalem Grant of the Flemish Government.

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Christensen, J., Vaes, S. KMS Spectra for Group Actions on Compact Spaces. Commun. Math. Phys. 390, 1341–1367 (2022). https://doi.org/10.1007/s00220-021-04282-w

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