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AdS4/CFT3+gravity for Accelerating Conical Singularities arXiv:0809.2789 arXiv:0809.2789 Mohamed Anber HET Bag Lunch Novemberr 12th
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Outline AdS/CFT:overview AdS/CFT+gravity Gravity in 2+1 D Geometry of accelerating particles in 2+1 D Quantum corrections: weakly coupled CFT Backreaction from weakly coupled CFT: accelerating BH Strongly coupled CFT: the AdS construction Accelerating BH on the brane, what is the story? conclusion
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AdS/CFT: overview Holography (Bekenstein, Susskind, ‘t Hooft, Bousso): information in the bulk is encoded on a surface
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AdS/CFT: overview AdS space: Solution to Einstein’s equations with negative cosmological constant Conformal Field theory (CFT): Invariant under conformal transformations=Poincaré +scale invariance, Roughly speaking for odd dimensions Maldacena conjecture (AdS/CFT) (1997)
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AdS/CFT+gravity Extra Dimensions!! Kaluza–Klein compactification Randall-Sundrum model: large extra dimensions (brane ) On the RS brane: gravity+CFT(UV cutoff ) Provides a natural set up to study strongly coupled CFT systems in non-trivial gravitational backgrounds
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AdS/CFT+gravity Black holes (BH) localized on RS-branes: BH evaporation (classical BH+CFT corrections) Important for quantum gravity But no localized BH on RS 3-brane (4+1 D bulk) so far!! Emparan, Horowitz and Myers (EHM) (1999) found BHs on RS 2-brane (3+1 D bulk) Emparan, Fabbri and Kaloper interpretation: (EHM) BHs are quantum corrected BHs. How they did it? They compared the quantum corrections to a point mass in 2+1 D to (EHM) BHs Classical geometryCFT correctionsSemiclassical gravity
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Gravity in 2+1 D Gravity is not dynamical in 2+1 D Vacuum Solution: conical singularity, no BH
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Gravity in 2+1 D Why to study accelerating conical singularities? It provides a natural setup for a CFT kept at a finite temperature (Unruh effect) The presence of acceleration horizon may give us some idea about the more interesting case of BHs on the RS 3-brane. Finite temperature CFT: a clue about a possible confinement/de- confinement phase transition
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Geometry of accelerating particles in 2+1 D The presence of point particles in the accelerating frame with conical singularity acceleration
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Geometry of accelerating particles in 2+1 D The acceleration has to be provided by a strut strut particle
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Quantum corrections: weakly coupled CFT Lagrangian density Conformally coupled theory Acceleration finite temperature (Unruh effect) Euclidean time thermal Green’s function To find the quantum corrections to the classical spacetime: 1-solve for well behaved with appropriate BCs 2- regularize by subtracting 3-calculate the energy-momentum tensor (Casimir effect)
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Quantum corrections: weakly coupled CFT -Transparent BCs -Dirichlet BCs Strut position
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Backreaction from weakly coupled CFT: accelerating BH Semiclassical solution Before quantum corrections After quantum corrections: accelerating black hole Regular at the strut
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Backreaction from weakly coupled CFT: accelerating BH naked singularity!
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Strongly coupled CFT: the AdS construction The AdS-C metric stringsingularity horizon AdS boundary empty brane
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Strongly coupled CFT: the AdS construction Compute the extrinsic curvature Write down the Israel junction condition The induced metric on the brane induced metric K- K+ n Accelerating BH dressed with strongly coupled CFT
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Strongly coupled CFT: the AdS construction
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Accelerating BH on the brane, what is the story? Weak CFTStrong CFT classical geometry quantum corrections backreaction AdS+brane Before quantum corrections before=after Position of the string after=? Mass of the string after=? ? coordinate transformation
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Accelerating BH on the brane, what is the story? To compare the two solutions we use
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Accelerating BH on the brane, what is the story?
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Phase transition?
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conclusion AdS/CFT+gravity to understand strongly coupled CFT in non- tervial backgrounds More to understand about the number of degrees of freedom in strongly coupled CFT (suppressed? Why? What implications for the absent BH on the RS-3 brane?) Can we learn about realistic systems?
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Thank you
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