(Translated by https://www.hiragana.jp/)
Phys. Rev. D 100, 046004 (2019) - Nonequilibrium approach to holographic superconductors using gradient flow
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Nonequilibrium approach to holographic superconductors using gradient flow

P. Mikula, M. E. Carrington, and G. Kunstatter
Phys. Rev. D 100, 046004 – Published 5 August 2019

Abstract

We study a charged scalar field in a bulk 3+1-dimensional anti–de Sitter (AdS) spacetime with a planar black hole background metric. Through the AdS/CFT correspondence this is equivalent to a strongly coupled field theory in 2+1 dimensions describing a superconductor. We use the gradient flow method and solve the flow equations numerically between two fixed points: a vacuum solution and a hairy black hole solution. We study the corresponding flow on the boundary between a normal metal phase and a superconducting phase. We show how the gradient flow moves fields between two fixed points in a way that minimizes the free energy of the system. At the fixed points of the flow the AdS/CFT correspondence provides an equivalence between the Euclidean on-shell action in the bulk and the free energy of the boundary, but it does not tell us about fields away from equilibrium. However, we can formally link static off-shell configurations in the bulk and in the boundary at the same point along the flow. For quasistatic evolution at least, it may be reasonable to think of this link as an extension of the AdS/CFT correspondence.

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  • Received 12 March 2019

DOI:https://doi.org/10.1103/PhysRevD.100.046004

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsCondensed Matter, Materials & Applied Physics

Authors & Affiliations

P. Mikula1,2,3,4,*, M. E. Carrington1,4,†, and G. Kunstatter2,4,‡

  • 1Department of Physics, Brandon University, Brandon, Manitoba R7A 6A9, Canada
  • 2Department of Physics, University of Winnipeg, Winnipeg, Manitoba R3B 2E9, Canada
  • 3Department of Physics and Astronomy, University of Manitoba, Winnipeg, Manitoba R3T 2N2, Canada
  • 4Winnipeg Institute for Theoretical Physics, Winnipeg, Manitoba, Canada

  • *pnmikula@gmail.com
  • carrington@brandonu.ca
  • gkunstatter@uwinnipeg.ca

Article Text

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Issue

Vol. 100, Iss. 4 — 15 August 2019

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