SLIDE 3 Black holes, holographic principle Analogy with Bekenstein-Hawking area law: a black hole carries an entropy that is proportional to its horizon area A.
Relevance of the EE and its scaling
Efficiency of simulations Efficiency of 1D algorithms such as DMRG is based on the Area law behaviour
(U. Schollwöck, Rev. Mod. Phys. 77 259 (2005))
Characterization of quantum phases Universal behavior near critical points. Indicator of phases that cannot be described by local
- rder parameters (informations about central charge, topological charge, Kondo length …)
(X. G. Wen, Phys. Rev. B 40 7387 (1989)), (E. Witten, Adv. Theory Math. 2 253 (1998)), (E. Nussinov et al. , Ann. Phys. 322 977 (2009))
Nonequilibrium dynamics, quenches Propagation of excitation after a quench
SA(t) ∝ ∂(A)