English

Holographic complexity is nonlocal

High Energy Physics - Theory 2018-02-15 v2 General Relativity and Quantum Cosmology

Abstract

We study the "complexity equals volume" (CV) and "complexity equals action" (CA) conjectures by examining moments of of time symmetry for AdS3\rm AdS_3 wormholes having nn asymptotic regions and arbitrary (orientable) internal topology. For either prescription, the complexity relative to nn copies of the M=0M=0 BTZ black hole takes the form ΔC=αcχ\Delta C = \alpha c \chi , where cc is the central charge and χ\chi is the Euler character of the bulk time-symmetric surface. The coefficients αV=4π/3\alpha_V = -4\pi/3, αA=1/6\alpha_A = 1/6 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 αV\alpha_V, αA\alpha_A 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 αA\alpha_A, which requires the associated complexity to decrease when handles are added to our wormhole.

Keywords

Cite

@article{arxiv.1801.01137,
  title  = {Holographic complexity is nonlocal},
  author = {Zicao Fu and Alexander Maloney and Donald Marolf and Henry Maxfield and Zhencheng Wang},
  journal= {arXiv preprint arXiv:1801.01137},
  year   = {2018}
}

Comments

17 pages, 4 figures; v2: minor modifications

R2 v1 2026-06-22T23:35:48.445Z