Entanglement entropy in the O(N) model
Source: Phys. Rev. B 80, 115122 (2009); doi:10.1103/PhysRevB.80.115122
Published 23 September 2009
It is generally believed that in spatial dimension d>1, the leading contribution to the entanglement entropy S=−tr
A log
A scales as the area of the boundary of subsystem A. The coefficient of this “area law” is nonuniversal. However, in the neighborhood 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
=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 
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 Sn=
log tr 
in
and large-N expansions. For N
, this correction generally scales as N2 rather than the naively expected N. Moreover, the Renyi entropy has a phase transition as a function of n for d close to 3.
©2009 The American Physical Society
A log
A scales as the area of the boundary of subsystem A. The coefficient of this “area law” is nonuniversal. However, in the neighborhood 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
=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 
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 Sn=
and large-N expansions. For N
, this correction generally scales as N2 rather than the naively expected N. Moreover, the Renyi entropy has a phase transition as a function of n for d close to 3.
©2009 The American Physical Society
| History: | Received 28 May 2009; revised 12 August 2009; published 23 September 2009 |
| Permalink: |
http://link.aps.org/abstract/PRB/v80/e115122 |
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