REVIEW
Three dimensional Janus and time-dependent black holes
High Energy Physics - Theory · Submitted 11 Jan 2007 · 24 references
Pith's verdict: A clean, modest extension of the Janus program to AdS3 plus a genuinely useful family of exact time-dependent black holes; the soft spots are presentational, not structural.
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Referee report
The paper
The paper claims
The Janus deformation of AdS$_3$ is shown to fit inside ten-dimensional type IIB supergravity, with a two-dimensional interface CFT as its proposed dual and a family of time-dependent black holes as a by-product.
The reading
What carries the argument
The load-bearing device is the reduction of the ten-dimensional Janus ansatz to three-dimensional Einstein gravity coupled to a scalar with a negative cosmological constant, $I = (1/16pi G_3)int d^3x sqrt{g}(R_3 - g^{ab}partial_a varphi partial_b varphi + 2)$, followed by the observation that the resulting equation for the scale factor is the energy-conservation law of a particle in the potential $V(f) = -4f(f^2 - f + gamma^2/2)$. Integrability of that first-order equation is what makes the whole construction exact: the solution is written as $f = alpha_+^2 / mathrm{sn}^2(alpha_+(mu+mu_0),k)$ with $k = alpha_-/alpha_+$, and the dilaton follows from $varphi' = gamma/f^{1/2}$. The second device is a slicing substitution: because only $R_{ab} = -2g_{ab}$ is used, the $AdS_3$ factor can be swapped for any three-metric with the same Ricci tensor, which is how the BTZ black hole and the higher-dimensional cosmological black holes are generated almost for free. The third device is the identification of the operator dual to the dilaton in the D1-D5 orbifold CFT, taken to be the marginal operator $O_varphi = -(1/4pi)sum_{i,a} :partial X^{i,a} barpartial X^{i,a}:$.
Extended reading notes
Core claim
The paper's central claim is that the three-dimensional Janus geometry embeds into type IIB supergravity on $AdS_3$ times $S^3$ times $M_4$ (with $M_4$ either $T^4$ or $K3$). The ansatz is $ds^2 = e^{2varphi}(dmu^2 + ds^2_{AdS_2}) + e^{2varphi}ds^2_{S^3} + e^{-2varphi}ds^2_4$ with a dilaton depending only on the slicing coordinate and a three-form flux proportional to the $AdS_2$ and $S^3$ volume forms. The ten-dimensional equations collapse to $f'^2 = 4f^3 - 4f^2 + 2gamma^2 f$, the zero-energy condition for a particle moving in an effective cubic potential, which is integrable. For $gamma^2 < 1/2$ the coordinate runs over a finite interval and the dilaton takes two distinct constant values $varphi_pm$ at the two ends, so the boundary is two half-planes glued at a line and the dual is an interface CFT with a marginal deformation active in one half. The authors further show that the same slicing trick, applied with a BTZ metric or with $-dtau^2 + cos^2tau, ds^2_Sigma$ in place of $AdS_3$, yields exact black-hole solutions whose horizon area grows monotonically in time and whose two disconnected boundaries carry couplings $e^{varphi_+}$ and $e^{varphi_-}$.
Load-bearing premise
The identification of the operator dual to the six-dimensional dilaton as the normal-ordered marginal operator $-(1/4pi)sum :partial X barpartial X:$ is, in the authors' own words, a natural guess, and the whole interface-CFT reading rests on it.
Editorial extensions
If this is right
- The Janus deformation of the $AdS_3/CFT_2$ correspondence is a concrete, exactly solvable example of an interface CFT, in the lowest dimension where the dual orbifold CFT is under perturbative control.
- The one-point function of the dual marginal operator is predicted at leading order in the deformation, $langle O_varphi rangle = -gamma Q_1 Q_5, epsilon(x)/(4pi x^2)$, giving a number that conformal perturbation theory on the field-theory side can be checked against.
- The deformed energy-momentum tensor vanishes, $langle T_{ab}rangle = 0$, so the deformation does not change the central charge even though the asymptotic $AdS_3$ radius appears to differ on the two sides; the dilaton factors cancel against the behaviour of the three-dimensional Newton constant.
- Time-dependent black holes with a running dilaton exist in three and higher dimensions, with horizon area growing monotonically from a minimum to $2pi r_0$ (three dimensions) or $V_Sigma$ (higher dimensions), and reduce to the static $M=0$, $k=-1$ topological black hole when the deformation is switched off.
- The three- and five-dimensional members of this family embed into ten-dimensional type IIB supergravity, so their duals are ordinary gauge-theory-like CFTs rather than lower-dimensional toy models.
Reading between the lines
- Because the boundary metric of the higher-dimensional black holes can be chosen either as a cosmological $cos^2tau$ slicing or as flat $R times Sigma$, the same bulk solution can be read as a dual description of either a big-bang/big-crunch cosmology or a thermalization process starting far from equilibrium; the authors mention the second reading but do not compute anything with it.
- The two-boundary structure of the Janus black hole resembles a traversable-wormhole geometry with unequal couplings on the two ends, which suggests asking whether the dual state is entangled across the two boundaries and whether the growth of horizon area is dual to entanglement growth.
- Since the SL(2,R) symmetry of the classical supergravity can rotate the dilaton into an axion, the natural next case has both the gauge coupling and the theta angle jumping at the interface; the authors note this but do not write the rotated solution.
- The construction only uses $R_{ab} = -2g_{ab}$ for the sliced factor, so any three-dimensional Einstein metric with negative cosmological constant should work as a seed; this suggests a broader family of Janus black holes with rotation or with different horizon topologies than the ones written down here.
Original abstract
We show that the three dimensional Janus geometry can be embedded into the type IIB supergravity and discuss its dual CFT description. We also find exact solutions of time dependent black holes with a nontrivial dilaton field in three and higher dimensions as an application of the Janus construction.
The compiled record
The paper's own sentences, arranged, kept beside the review and separate from it. Each label is drawn from a closed vocabulary; the number beside it is the probability the classifier gave that label. Numbers in the tables are the authors', checked by code. No sentence in this record was written by a model.
The abstract, sentence by sentence
We show that the three dimensional Janus geometry can be embedded into the type IIB supergravity and discuss its dual CFT description. We also find exact solutions of time dependent black holes with a nontrivial dilaton field in three and higher dimensions as an application of the Janus construction.
background contribution method result interpretation main claim
| # | sentence | role | the authors' own work | states the main conclusion | strength |
|---|---|---|---|---|---|
| s0 | We show that the three dimensional Janus geometry can be embedded into the type IIB supergravity and discuss its dual CFT description. | contribution 0.94 | 0.93 | 0.54 | asserted 1.00 |
| s1 | We also find exact solutions of time dependent black holes with a nontrivial dilaton field in three and higher dimensions as an application of the Janus construction. | result 0.80 | 0.96 | 0.26 | asserted 1.00 |
What was examined, and what was not
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Figures
Figures reproduced from arXiv:hep-th/0701108 by the authors.
References
How later papers used it
67 later papers cite it
1 paper by the same authors is listed below: 1 built on it.
Builds on it 1 of 4 papers with this label · 1 by the same authors
By the same authors
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Presented a half-BPS solution that is a supersymmetric generalization of the solution found in this paper, with explicit expressions for solutions having n AdS_3 x S^3 regions when the surface has genus zero and one boundary component.
Half-BPS Solutions locally asymptotic to AdS_3 x S^3 and interface conformal field theories (2009) (same authors) · 0.97 · paraphrased: the licence does not allow quoting
How the literature uses it
64 arXiv papers cite this in 121 sentences
Papers citing it · 64 sentences without a confident label
Builds on it 4 papers
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This is the generalization of the dilatonic Janus solution with a 3 dimensional metric [ref] , or in our notation $d=0$.
Universal Behavior of Entanglement Entropies in Interface CFTs from General Holographic Spacetimes · Half-BPS Six Dimensional (0,4) Supergravity Solution · 0.87
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In particular, we present a half-BPS solution which is a supersymmetric generalization of the solution found in [ref] and we give explicit expressions for solutions having $n$ $AdS_3 ×S^3$ regions as long as $Σ$ has genus zero and one boundary component.
Half-BPS Solutions locally asymptotic to AdS_3 x S^3 and interface conformal field theories · Introduction · 0.97
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In this section, let us construct a time-dependent black hole, analogous to the one discussed in [ref] .
Time-like Janus Solution -- holographic global quantum quench -- · Finite Temperature · 0.84
Uses its method or tool 2 papers
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First by choosing the conformal factor $h^2= cos^2τ/f(μ)$, the boundary metric for the CFT is given by [ref] ds^2_B = -dt^2 + ds^2_Σ .
Time dependent black holes and thermal equilibration · Correspondence · 0.82
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In the presence of the exactly marginal perturbation, we can employ the Janus solution [ref] as the gravity dual to $ρ^(2)1|2_A$.
SVD Entanglement Entropy · Holographic SVD entropy from Janus Solution · 0.83
Uses its data or values 3 papers
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In addition, the area of the horizon is given by [ref] 𝒜 (τ) = 2 πL r_h α_+ sin≤π/2 - τ/sn ≤α_+ ≤π/2 - τ, k t_B →∞⟶ 2 πL r_h .
Volume complexity for Janus $\mathrm{AdS}_3$ geometries · Time dependence of the volume · 0.93
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In the explicit example of 3D Janus solution given in [ref] , the metric reads e^2h(ρ)=1/2+1-2γ^2/2cosh(2ρ), where $γ$ parameterizes the Janus deformation.
Aspects of Pseudo Entropy in Field Theories · Holographic Pseudo Entropy in Gapless Phases via Janus Solutions · 0.87
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In an explicit example of 3D Janus solution of Einstein-dilaton theory [ref] , we have e^2h(ρ)=1/2+1-2γ^2/2cosh(2ρ).
Pseudo Entropy in Free Quantum Field Theories · Holographic Analysis · 0.83
Compares with it 2 papers
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These two equations agree with those of the so-called Janus solutions [ref] which are spacelike deformations in AdS space.
Janus Deformation of de Sitter Space and Transitions in Gravitational Algebras · Deformation of dS Space · 0.86
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If we choose the sourceless part as in [ref] , then the temperature of the two black holes always agree.
Holographic R\'enyi relative divergence in JT gravity · Conclusion and discussions · 0.93
Cites it as support 1 paper
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Even for the time dependent case, the areal entropy seems to represent the entanglement entropy as discussed in Refs. [ref] .
Entropy of universe as entanglement entropy · Our proposal · 0.99
Cites it as background 34 papers
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In the following section we will review the time dependent black hole solution of [ref] .
Time dependent black holes and thermal equilibration · Introduction · 0.83
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To investigate this question further, we concentrate on another type of black hole with a causal shadow called the three-dimensional time-dependent Janus black hole,[ There is also a static type of Janus deformation of BTZ black hole [ref] .] which is a one parameter deformation of the BTZ black hole and a solution of the Einstein-scalar theory [ref] .
Holographic Entanglement and Causal Shadow in Time-Dependent Janus Black Hole · Introduction · 0.88
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Prime examples of the correspondence [ref] involve a $d$ dimensional CFT perturbed by a scalar primary operator of dimension $Δ$ and its gravity dual described by the $d+1$ dimensional Euclidean Janus geometry [ref] .
Quantum Information Metric on $\mathbb{R} \times S^{d-1}$ · Introduction · 0.93
Discussion
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