TY - JOUR
T1 - A First Law of Entanglement Rates from Holography
AU - O'Bannon, Andy
AU - Probst, Jonas
AU - Rodgers, Ronnie
AU - Uhlemann, Christoph F.
N1 - 20 pages + 1 appendix, v2: version accepted to Phys. Rev. D
PY - 2016/12/22
Y1 - 2016/12/22
N2 - For a perturbation of the state of a Conformal Field Theory (CFT), the response of the entanglement entropy is governed by the so-called "first law" of entanglement entropy, in which the change in entanglement entropy is proportional to the change in energy. Whether such a first law holds for other types of perturbations, such as a change to the CFT Lagrangian, remains an open question. We use holography to study the evolution in time $t$ of entanglement entropy for a CFT driven by a $t$-linear source for a conserved $U(1)$ current or marginal scalar operator. We find that although the usual first law of entanglement entropy may be violated, a first law for the rates of change of entanglement entropy and energy still holds. More generally, we prove that this first law for rates holds in holography for any asymptotically $(d+1)$-dimensional Anti-de Sitter metric perturbation whose $t$ dependence first appears at order $z^d$ in the Fefferman-Graham expansion about the boundary at $z=0$.
AB - For a perturbation of the state of a Conformal Field Theory (CFT), the response of the entanglement entropy is governed by the so-called "first law" of entanglement entropy, in which the change in entanglement entropy is proportional to the change in energy. Whether such a first law holds for other types of perturbations, such as a change to the CFT Lagrangian, remains an open question. We use holography to study the evolution in time $t$ of entanglement entropy for a CFT driven by a $t$-linear source for a conserved $U(1)$ current or marginal scalar operator. We find that although the usual first law of entanglement entropy may be violated, a first law for the rates of change of entanglement entropy and energy still holds. More generally, we prove that this first law for rates holds in holography for any asymptotically $(d+1)$-dimensional Anti-de Sitter metric perturbation whose $t$ dependence first appears at order $z^d$ in the Fefferman-Graham expansion about the boundary at $z=0$.
KW - hep-th
U2 - 10.1103/PhysRevD.96.066028
DO - 10.1103/PhysRevD.96.066028
M3 - Article
JO - Physical Review D. Particles, Fields, Gravitation, and Cosmology
JF - Physical Review D. Particles, Fields, Gravitation, and Cosmology
SN - 1550-7998
ER -