Holographic complexity is nonlocal
- 1. Department of Physics, University of California,Santa Barbara, CA 93106 (United States)
- 2. Department of Physics, McGill University, 3600 rue Université, Monteal H3A 2T8 (Canada)
- 3. School of Physics, Nankai University,Tianjin 300071 (China)
Description
We study the "complexity equals volume" (CV) and "complexity equals action" (CA) conjectures by examining moments of of time symmetry for wormholes having asymptotic regions and arbitrary (orientable) internal topology. For either prescription, the complexity relative to copies of the BTZ black hole takes the form , where is the central charge and is the Euler character of the bulk time-symmetric surface. The coefficients , defined by CV and CA are independent of both temperature and any moduli controlling the geometry inside the black hole. Comparing with the known structure of dual CFT states in the hot wormhole limit, the temperature and moduli independence of , implies that any CFT gate set defining either complexity cannot be local. In particular, the complexity of an efficient quantum circuit building local thermofield-double-like entanglement of thermal-sized patches does not depend on the separation of the patches so entangled. We also comment on implications of the (positive) sign found for , which requires the associated complexity to decrease when handles are added to our wormhole.
Availability note (English)
Available from http://dx.doi.org/10.1007/JHEP02(2018)072; Available from http://repo.scoap3.org/record/23737Additional details
Identifiers
- DOI
- 10.1007/JHEP02(2018)072;
- arXiv
- arXiv:1801.01137;
Publishing Information
- Journal Title
- Journal of High Energy Physics (Online)
- Journal Volume
- 2018
- Journal Issue
- 02
- Journal Page Range
- p. 72
- ISSN
- 1029-8479
INIS
- Country of Publication
- Germany
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49090019
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- ANTI DE SITTER SPACE; ASYMPTOTIC SOLUTIONS; BLACK HOLES; CONFORMAL INVARIANCE; DUALITY; HOLOGRAPHIC PRINCIPLE; QUANTUM ENTANGLEMENT; QUANTUM FIELD THEORY
- Descriptors DEC
- FIELD THEORIES; INVARIANCE PRINCIPLES; MATHEMATICAL SOLUTIONS; MATHEMATICAL SPACE; SPACE
Optional Information
- Copyright
- Copyright (c) OPEN ACCESS, © The Authors
- Notes
- PUBLISHER-ID: JHEP02(2018)072; ARXIV:1801.01137; OAI: oai:repo.scoap3.org:23737
- Funding organization
- SCOAP3, CERN, Geneva (Switzerland)