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{{Short description|Theoretical Physics}}
{{String theory}}

The '''Ryu–Takayanagi conjecture''' is a conjecture within [[holographic principle|holography]] that posits a quantitative relationship between the [[Entropy of entanglement|entanglement entropy]] of a [[conformal field theory]] and the geometry of an associated [[Anti-de Sitter space|anti-de Sitter]] spacetime.<ref name = ryu-takayanagi>{{Cite journal|last1=Ryu|first1=Shinsei|last2=Takayanagi|first2=Tadashi|date=2006-08-21|title=Aspects of Holographic Entanglement Entropy|journal=Journal of High Energy Physics|volume=2006|issue=8|pages=045|doi=10.1088/1126-6708/2006/08/045|issn=1029-8479|arxiv=hep-th/0605073|bibcode=2006JHEP...08..045R|s2cid=14858887}}</ref><ref>{{Citation|last=Stanford Institute for Theoretical Physics|title=Gravity and Entanglement|date=2015-10-15|url=https://www.youtube.com/watch?v=WQU9yOtWrQk|accessdate=2017-05-07}}</ref> The formula characterizes "holographic screens" in the bulk; that is, it specifies which regions of the bulk geometry are "responsible to particular information in the dual CFT".<ref name="introduction">
{{citation
 | last = Fukami
 | first = Masaya
 | title = Introduction to the Ryu–Takayanagi Formula
 | pages = 2
 | date = March 2018
 | url =http://theory.uchicago.edu/~sethi/Teaching/P483-W2018/Intro%20to%20the%20RT.pdf }}
</ref> The conjecture is named after [[Shinsei Ryu]] and [[Tadashi Takayanagi]], who jointly published the result in 2006.<ref>
{{cite journal
 | last1 = Ryu | first1 = Shinsei
 | last2 = Takayanagi| first2 = Tadashi
 | title = Holographic Derivation of Entanglement Entropy from AdS/CFT
 | journal = Phys. Rev. Lett.
 | volume = 96
 | issue = 18
 | pages = 181602
 | date = May 2006
 | doi = 10.1103/PhysRevLett.96.181602| pmid = 16712357
 | arxiv = hep-th/0603001
 | s2cid = 119441463
 }}</ref> As a result, the authors were awarded the 2015 [[Breakthrough Prize in Fundamental Physics]] for "fundamental ideas about entropy in quantum field theory and quantum gravity",<ref>
{{cite web
 | url = https://breakthroughprize.org/News/21
 | title = Recipients of the 2015 Breakthrough Prizes in Fundamental Physics and Life Sciences Announced
 | website = www.breakthroughprize.org
 | access-date = 3 Aug 2018}}</ref> and awarded the 2024 [[Dirac Medal (ICTP)|Dirac Medal of the ICTP]] for "their insights on quantum entropy in quantum gravity and quantum field theories".<ref>{{cite web|title=ICTP Announces 2024 Dirac Medallists Four physicists recognized for their contributions to quantum entropy|url=https://www.ictp.it/news/2024/8/ictp-announces-2024-dirac-medallists|access-date=10 September 2024}}</ref> The formula was generalized to a [[General covariance|covariant]] form in 2007.<ref>{{cite journal
 | last1 = Hubeny | first1 = Veronika E.
 | last2 = Rangamani| first2 = Mukund
 | last3 = Takayanagi| first3 = Tadashi
 | title = A Covariant Holographic Entanglement Entropy Proposal
 | journal = JHEP
 | volume = 2007
 | issue = 7
 | pages = 062
 | date = 23 July 2007
 | doi = 10.1088/1126-6708/2007/07/062| arxiv = 0705.0016
 | bibcode = 2007JHEP...07..062H
 | s2cid = 15206042
 }}</ref>

==Motivation==

The [[Black hole thermodynamics|thermodynamics of black holes]] suggests certain relationships between the [[entropy]] of black holes and their geometry. Specifically, the Bekenstein–Hawking area formula conjectures that the entropy of a black hole is proportional to its surface area:

:<math>S_\text{BH} = \frac{k_\text{B} A}{4\ell_\text{P}^2}</math>

The Bekenstein–Hawking entropy <math>S_\text{BH}</math> is a measure of the information lost to external observers due to the presence of the horizon. The horizon of the black hole acts as a "screen" distinguishing one region of the [[spacetime]] (in this case the exterior of the black hole) that is not affected by another region (in this case the interior). The Bekenstein–Hawking area law states that the area of this surface is proportional to the entropy of the information lost behind it.

The Bekenstein–Hawking entropy is a statement about the gravitational entropy of a system; however, there is another type of entropy that is important in quantum information theory, namely the [[Entropy of entanglement|entanglement (or von Neumann) entropy]]. This form of entropy provides a measure of how far from a pure state a given quantum state is, or, equivalently, how entangled it is. The entanglement entropy is a useful concept in many areas, such as in condensed matter physics and quantum many-body systems. Given its use, and its suggestive similarity to the Bekenstein–Hawking entropy, it is desirable to have a holographic description of entanglement entropy in terms of gravity.

==Holographic preliminaries==

{{main| Holographic principle}}

The holographic principle states that gravitational theories in a given dimension are dual to a [[gauge theory]] in one lower dimension. The [[AdS/CFT correspondence]] is one example of such duality. Here, the field theory is defined on a fixed background and is equivalent to a quantum gravitational theory whose different states each correspond to a possible spacetime geometry. The conformal field theory is often viewed as living on the boundary of the higher dimensional space whose gravitational theory it defines. The result of such a duality is a dictionary between the two equivalent descriptions. For example, in a CFT defined on <math>d</math> dimensional [[Minkowski space]] the vacuum state corresponds to pure AdS space, whereas the thermal state corresponds to a planar black hole.<ref name=vr>{{cite book
 | last1 = Van Raamsdonk| first1 = Mark
 | title = New Frontiers in Fields and Strings
 | pages = 297–351
 | chapter = Lectures on Gravity and Entanglement
 | date = 31 August 2016
 | arxiv = 1609.00026
 | doi = 10.1142/9789813149441_0005
 | isbn = 978-981-314-943-4
 | s2cid = 119273886
 }}</ref> Important for the present discussion is that the thermal state of a CFT defined on the <math>d</math> dimensional sphere corresponds to the <math>d+1</math> dimensional Schwarzschild black hole in AdS space.

The Bekenstein–Hawking area law, while claiming that the area of the black hole horizon is proportional to the black hole's entropy, fails to provide a sufficient microscopic description of how this entropy arises. The holographic principle provides such a description by relating the black hole system to a quantum system which does admit such a microscopic description. In this case, the CFT has discrete eigenstates and the thermal state is the canonical ensemble of these states.<ref name=vr/> The entropy of this ensemble can be calculated through normal means, and yields the same result as predicted by the area law. This turns out to be a special case of the Ryu–Takayanagi conjecture.

==Conjecture==

Consider a spatial slice <math> \Sigma </math> of an AdS space time on whose boundary we define the dual CFT. The Ryu–Takayanagi formula states:

{{NumBlk|:|<math>S_A = \frac{\text{Area of } \gamma_A}{4G} </math>|{{EquationRef|1}}}}

where <math> S_A</math> is the entanglement entropy of the CFT in some spatial sub-region <math> A \subset \partial \Sigma</math> with its complement <math>B</math>, and <math>\gamma_A</math> is the Ryu–Takayanagi surface in the bulk.<ref name=ryu-takayanagi /> This surface must satisfy three properties:<ref name=vr />

#  <math> \gamma_A </math> has the same boundary as <math> A </math>. 
#  <math> \gamma_A </math> is [[Homology (mathematics)|homologous]] to A. 
#  <math> \gamma_A </math> extremizes the area. If there are multiple extremal surfaces,  <math> \gamma_A </math> is the one with the least area.

Because of property (3), this surface is typically called the ''minimal surface'' when the context is clear. Furthermore, property (1) ensures that the formula preserves certain features of entanglement entropy, such as <math> S_A = S_B </math> and <math> S_{A_1 + A_2} \geq S_{A_1 \cup A_2} </math>.{{clarify|date=June 2024}} The conjecture provides an explicit geometric interpretation of the entanglement entropy of the boundary CFT, namely as the area of a surface in the bulk.

==Example==
In their original paper, Ryu and Takayanagi show this result explicitly for an example in <math> \text{AdS}_3 / \text{CFT}_2 </math> where an expression for the entanglement entropy is already known.<ref name=ryu-takayanagi /> For an <math> \text{AdS}_3 </math> space of radius <math> R </math>, the dual CFT has a [[central charge]] given by

{{NumBlk|:|<math>c = \frac{3R}{2G}</math>|{{EquationRef|2}}}}

Furthermore, <math> \text{AdS}_3  </math> has the [[Metric (general relativity)|metric]]

<math>
ds^2 = R^2(-\cosh{\rho^2 dt^2} + d\rho^2 + \sinh{\rho^2 d\theta^2})
</math>

in <math>(t, \rho, \theta) </math> (essentially a stack of [[Poincaré disk model|hyperbolic disks]]). Since this metric diverges at <math> \rho \to \infty </math>, <math> \rho </math> is restricted to <math> \rho \leq \rho_0 </math>. This act of imposing a maximum <math> \rho </math> is analogous to the corresponding CFT having a UV cutoff. If <math> L </math> is the length of the CFT system, in this case the circumference of the cylinder calculated with the appropriate metric, and <math> a </math> is the lattice spacing, we have

<math> e^{\rho_0} \sim L/a</math>.

In this case, the boundary CFT lives at coordinates <math>(t, \rho_0, \theta) = (t, \theta) </math>. Consider a fixed <math> t </math> slice and take the subregion A of the boundary to be <math> \theta \in [0, 2\pi l / L]</math> where <math> l </math> is the length of <math> A </math>. The minimal surface is easy to identify in this case, as it is just the geodesic through the bulk that connects <math> \theta = 0 </math> and <math> \theta = 2 \pi l/L</math>. Remembering the lattice cutoff, the length of the geodesic can be calculated as

{{NumBlk|:|<math> \cosh{(L_{\gamma_A} / R)} = 1 + 2\sinh^2 \rho_0 \sin^2 \frac{\pi l}{L}</math>|{{EquationRef|3}}}}

If it is assumed that <math> e^{\rho_0} >> 1</math>, then using the Ryu–Takayanagi formula to compute the entanglement entropy. Plugging in the length of the minimal surface calculated in ({{EquationNote|3}}) and recalling the central charge ({{EquationNote|2}}), the entanglement entropy is given by

{{NumBlk|:|<math> S_A = \frac{R}{4G}\log{(e^{2\rho_0} \sin^2 \frac{\pi l}{L})} =\frac{c}{3} \log{(e^{\rho_0} \sin{\frac{\pi l}{L}} )} </math>|{{EquationRef|4}}}}

This agrees with the result calculated by usual means.<ref>{{Cite journal
|last1=Calabrese|first1=Pasquale
|last2=Cardy|first2=John
|date=2004-06-11
|title=Entanglement entropy and quantum field theory
|journal=Journal of Statistical Mechanics: Theory and Experiment
|volume=P06002
|issue=6
|pages=P06002
|doi=10.1088/1742-5468/2004/06/P06002
|arxiv=hep-th/0405152|bibcode=2004JSMTE..06..002C
|s2cid=15945690
}}</ref>

==References==
{{Reflist}}

{{quantum gravity}}

{{DEFAULTSORT:Ryu-Takayanagi conjecture}}
[[Category:Conjectures]]
[[Category:String theory]]