Abstract
The Boltzmann–Gibbs–von Neumann entropy of a large part (of linear size ) of some (much larger) -dimensional quantum systems follows the so-called area law (as for black holes), i.e., it is proportional to . Here we show, for , that the (nonadditive) entropy satisfies, for a special value of , the classical thermodynamical prescription for the entropy to be extensive, i.e., . Therefore, we reconcile with classical thermodynamics the area law widespread in quantum systems. Recently, a similar behavior was exhibited in mathematical models with scale-invariant correlations [C. Tsallis, M. Gell-Mann, and Y. Sato, Proc. Natl. Acad. Sci. U.S.A.102 15377 (2005)]. Finally, we find that the system critical features are marked by a maximum of the special entropic index .
- Received 16 March 2008
DOI:https://doi.org/10.1103/PhysRevE.78.021102
©2008 American Physical Society