• Open Access

Holographic complexity and charged scalar fields

Musema Sinamuli and Robert B. Mann
Phys. Rev. D 99, 106013 – Published 24 May 2019

Abstract

We construct a time-dependent expression of the computational complexity of a quantum system, which consists of two conformal complex scalar field theories in d dimensions coupled to constant electric potentials and defined on the boundaries of a charged anti–de Sitter black hole in (d+1) dimensions. Using a suitable choice of the reference state, Hamiltonian gates, and the metric on the manifold of unitaries, we find that the complexity grows linearly for a relatively large interval of time. We also remark that for scalar fields with very small charges the rate of variation of the complexity cannot exceed a maximum value known as the Lloyd bound.

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  • Received 15 February 2019

DOI:https://doi.org/10.1103/PhysRevD.99.106013

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)

Quantum Information, Science & TechnologyGravitation, Cosmology & AstrophysicsParticles & Fields

Authors & Affiliations

Musema Sinamuli1,* and Robert B. Mann2,1,†

  • 1Perimeter Institute for Theoretical Physics, Waterloo, Ontario N2L 2Y5, Canada
  • 2Department of Physics and Astronomy, University of Waterloo, Waterloo, Ontario N2L 3G1, Canada

  • *cmusema@perimeterinstitute.ca
  • rbmann@uwaterloo.ca

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Vol. 99, Iss. 10 — 15 May 2019

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