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Entanglement Entropy in the O(N) model

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arxiv 0904.4477 v1 pith:XO4WARGY submitted 2009-04-28 cond-mat.stat-mech hep-thquant-ph

classification cond-mat.stat-mechhep-thquant-ph
keywords entropycorrectionentanglementepsilonfixedpointuniversalarea
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It is generally believed that in spatial dimension d > 1 the leading contribution to the entanglement entropy S = - tr rho_A log rho_A scales as the area of the boundary of subsystem A. The coefficient of this "area law" is non-universal. However, in the neighbourhood of a quantum critical point S is believed to possess subleading universal corrections. In the present work, we study the entanglement entropy in the quantum O(N) model in 1 < d < 3. We use an expansion in epsilon = 3-d to evaluate i) the universal geometric correction to S for an infinite cylinder divided along a circular boundary; ii) the universal correction to S due to a finite correlation length. Both corrections are different at the Wilson-Fisher and Gaussian fixed points, and the epsilon -> 0 limit of the Wilson-Fisher fixed point is distinct from the Gaussian fixed point. In addition, we compute the correlation length correction to the Renyi entropy S_n = (log tr rho^n_A)/(1-n) in epsilon and large-N expansions. For N -> infinity, this correction generally scales as N^2 rather than the naively expected N. Moreover, the Renyi entropy has a phase transition as a function of n for d close to 3.

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Cited by 2 Pith papers

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  1. Lattice studies of entanglement entropy in $O(N)$ models at finite densities

    hep-lat 2026-02 conditional novelty 6.0 of 10

    A worm-algorithm boundary-deformation method computes ∂ℓ entanglement entropy in finite-density O(N) models, with initial O(4) results in 3D and an internal consistency check.

  2. Manifestation of quantum entanglement between harmonic oscillators in de Sitter

    gr-qc 2025-06 reject novelty 6.0 of 10

    In de Sitter space, two harmonic oscillators coupled by a massless scalar field develop late-time entanglement that is sizeable when frequency and separation are near the Hubble scale, and tiny otherwise.

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