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Gravity/Spin-model correspondence and holographic superfluids

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arxiv 1007.4854 v2 pith:QL4I6T4U submitted 2010-07-27 hep-th cond-mat.supr-conhep-lat

classification hep-thcond-mat.supr-conhep-lat
keywords gravitycontinuouscorrespondencecorrespondsmodemodelsphasescaling
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We propose a general correspondence between gravity and spin models, inspired by the well-known IR equivalence between lattice gauge theories and the spin models. This suggests a connection between continuous type Hawking-phase transitions in gravity and the continuous order-disorder transitions in ferromagnets. The black-hole phase corresponds to the ordered and the graviton gas corresponds to the disordered phases respectively. A simple set-up based on Einstein-dilaton gravity indicates that the vicinity of the phase transition is governed by a linear-dilaton CFT. Employing this CFT we calculate scaling of observables near T_c, and obtain mean-field scaling in a semi-classical approximation. In case of the XY model the Goldstone mode is identified with the zero mode of the NS-NS two-form. We show that the second speed of sound vanishes at the transition also with the mean field exponent.

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  1. Improved Holographic QCD on a Curved Background: an Application of Dynamical System Theory in Holography

    hep-th 2025-05 conditional novelty 7.0 of 10

    For the critical exponent b=b_c, IHQCD (alpha=1/2) admits only regular endpoint-type solutions at positive curvature and singular acceptable solutions at negative curvature, so the curvature-driven transition occurs at R=0.

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