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Using 3D Stringy Gravity to Understand the Thurston Conjecture

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arxiv hep-th/0306279 v1 pith:5YJ7PPC4 submitted 2003-06-27 hep-th math.DG

classification hep-thmath.DG
keywords fieldtheorythurstonappearsconjecturedilatoneightflow
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We present a string inspired 3D Euclidean field theory as the starting point for a modified Ricci flow analysis of the Thurston conjecture. In addition to the metric, the theory contains a dilaton, an antisymmetric tensor field and a Maxwell-Chern Simons field. For constant dilaton, the theory appears to obey a Birkhoff theorem which allows only nine possible classes of solutions, depending on the signs of the parameters in the action. Eight of these correspond to the eight Thurston geometries, while the ninth describes the metric of a squashed three sphere. It therefore appears that one can construct modified Ricci flow equations in which the topology of the geometry is encoded in the parameters of an underlying field theory.

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  1. Primary scalar hair in Gauss-Bonnet black holes with Thurston horizons

    hep-th 2024-12 conditional novelty 5.0 of 10

    In Einstein-Gauss-Bonnet gravity at the Chern-Simons point, exact asymptotically locally AdS5 black holes with primary scalar hair exist for Nil, Solv, and SL(2,R) Thurston horizon geometries.

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