The attractor mechanism, C-functions and aspects of holography in Lovelock gravity Mohamed M. Anber November 27 2007 HET bag-lunch.

Slides:



Advertisements
Similar presentations
Theories of gravity in 5D brane-world scenarios
Advertisements

Martín Schvellinger Instituto de Física de La Plata - CONICET Departamento de Física - UNLP The gauge/gravity duality and Non-Relativistic Quantum Field.
Brane-World Inflation
Holographic Superconductors with Higher Curvature Corrections Sugumi Kanno (Durham) work w/ Ruth Gregory (Durham) Jiro Soda (Kyoto) arXiv: , to.
A journey inside planar pure QED CP3 lunch meeting By Bruno Bertrand November 19 th 2004.
ASYMPTOTIC STRUCTURE IN HIGHER DIMENSIONS AND ITS CLASSIFICATION KENTARO TANABE (UNIVERSITY OF BARCELONA) based on KT, Kinoshita and Shiromizu PRD
Chanyong Park 35 th Johns Hopkins Workshop ( Budapest, June 2011 ) Based on Phys. Rev. D 83, (2011) arXiv : arXiv :
Extremal Single-charge Small Black holes Aninda Sinha DAMTP, Cambridge University, UK hep-th/ (to appear in CQG) with Nemani Suryanarayana(Perimeter),
Gerard ’t Hooft Spinoza Institute Utrecht University CMI, Chennai, 20 November 2009 arXiv:
Microscopic entropy of the three-dimensional rotating black hole of BHT massive gravity of BHT massive gravity Ricardo Troncoso Ricardo Troncoso In collaboration.
Entanglement in Quantum Critical Phenomena, Holography and Gravity Dmitri V. Fursaev Joint Institute for Nuclear Research Dubna, RUSSIA Banff, July 31,
Mohamed Anber HEP Bag Lunch April 1st With Lorenzo Sorbo
AdS4/CFT3+gravity for Accelerating Conical Singularities arXiv: arXiv: Mohamed Anber HET Bag Lunch Novemberr 12th.
The 2d gravity coupled to a dilaton field with the action This action ( CGHS ) arises in a low-energy asymptotic of string theory models and in certain.
Strings and Black Holes David Lowe Brown University AAPT/APS Joint Fall Meeting.
Entropy bounds Introduction Black hole entropy Entropy bounds Holography.
9 March Chung Yuan Christian University Chiang-Mei Chen Department of Physics, National Central University.
Holographic Description of Quantum Black Hole on a Computer Yoshifumi Hyakutake (Ibaraki Univ.) Collaboration with M. Hanada ( YITP, Kyoto ), G. Ishiki.
GAUGE/GRAVITY AND HEAVY ION PHYSICS How string theory might say something about strong coupling Wilke van der Schee June 29, 2011.
An introduction to the Gravity/Fluid correspondence and its applications Ya-Peng Hu College of Science, Nanjing University of Aeronautics and Astronautics,
Louisville March 22, 2006 Andrew Chamblin Memorial An AdS Thermal Properties of Strongly Coupled Gauge Theories with Fundamental Matter from Gauge/Gravity.
Black Holes, Entropy, and Information Gary Horowitz UCSB.
“Einstein Gravity in Higher Dimensions”, Jerusalem, Feb., 2007.
Einstein Field Equations and First Law of Thermodynamics Rong-Gen Cai (蔡荣根) Institute of Theoretical Physics Chinese Academy of Sciences.
A New Endpoint for Hawking Evaporation Gary Horowitz UCSB hep-th/ Gary Horowitz UCSB hep-th/
Shear viscosity of a highly excited string and black hole membrane paradigm Yuya Sasai Helsinki Institute of Physics and Department of Physics University.
On the exotic BTZ black holes Baocheng Zhang Based on papers PRL 110, ; PRD 88, Coauthor : P. K. Townsend KITPC,
Finite N Index and Angular Momentum Bound from Gravity “KEK Theory Workshop 2007” Yu Nakayama, 13 th. Mar (University of Tokyo) Based on hep-th/
Entanglement Entropy in Holographic Superconductor Phase Transitions Rong-Gen Cai Institute of Theoretical Physics Chinese Academy of Sciences (April 17,
Super Virasoro Algebras from Chiral Supergravity Ibaraki Univ. Yoshifumi Hyakutake Based on arXiv:1211xxxx + work in progress.
On Fuzzball conjecture Seiji Terashima (YITP, Kyoto) based on the work (PRD (2008), arXiv: ) in collaboration with Noriaki Ogawa (YITP)
Holographic Superconductors from Gauss-Bonnet Gravity Rong-Gen Cai Institute of Theoretical Physics Chinese Academy of Sciences (May 7, 2012) 2012 海峡两岸粒子物理和宇宙学研讨会,
Non-Supersymmetric Attractors Sandip Trivedi Tata Institute of Fundamental Research, Mumbai, India Madrid, June ‘07.
Light quark jet quenching in AdS/CFT Andrej Ficnar Columbia University Hot Quarks 2012 October 15, 2012.
Black holes sourced by a massless scalar KSM2105, FRANKFURT July, 21th 2015 M. Cadoni, University of Cagliari We construct asymptotically flat black hole.
II Russian-Spanish Congress “Particle and Nuclear Physics at all scales and Cosmology”, Saint Petersburg, Oct. 4, 2013 RECENT ADVANCES IN THE BOTTOM-UP.
Department of Physics, National University of Singapore
Non-Supersymmetric Attractors Sandip Trivedi Tata Institute of Fundamental Research, Mumbai, India Irvine, June’06.
Comments on entanglement entropy in the dS/CFT correspondence Yoshiki Sato ( Kyoto U. ) PRD 91 (2015) 8, [arXiv: ] 9th July.
Gravitational collapse of massless scalar field Bin Wang Shanghai Jiao Tong University.
Holographic QCD in the medium
Black Holes and the Fluctuation Theorem Susumu Okazawa ( 総研大, KEK) with Satoshi Iso and Sen Zhang, arXiv: work in progress.
Higher spin AdS 3 holography and superstring theory Yasuaki Hikida (Rikkyo University) Based on collaborations with T. Creutzig (U. of Alberta) & P. B.
On String Theory Duals of Lifshitz-like Fixed Point Tatsuo Azeyanagi (Kyoto University) Based on work arXiv: (to appear in JHEP) with Wei Li (IPMU)
Microscopic entropy of black holes : a two-dimensional approach M. Cadoni, Capri 2004 Abstract Two-dimensional gravity models allow in many situations.
Holographic Renormalization Group with Gravitational Chern-Simons Term Takahiro Nishinaka ( Osaka U.) (Collaborators: K. Hotta, Y. Hyakutake, T. Kubota.
Holographic Description of Quantum Black Hole on a Computer Yoshifumi Hyakutake (Ibaraki Univ.) Collaboration with M. Hanada ( YITP, Kyoto ), G. Ishiki.
B.-H.L, R. Nayak, K. Panigrahi, C. Park On the giant magnon and spike solutions for strings on AdS(3) x S**3. JHEP 0806:065,2008. arXiv: J. Kluson,
1 Bhupendra Nath Tiwari IIT Kanpur in collaboration with T. Sarkar & G. Sengupta. Thermodynamic Geometry and BTZ black holes This talk is mainly based.
Gravity effects to the Vacuum Bubbles Based on PRD74, (2006), PRD75, (2007), PRD77, (2008), arXiv: [hep-th] & works in preparation.
Hawking radiation as tunneling from squashed Kaluza-Klein BH Ken Matsuno and Koichiro Umetsu (Osaka city university) (Kyoto sangyo university) Phys. Rev.
Based on Phys. Rev. D 92, (R) (2015) 中科大交叉学科理论研究中心
Boundary conditions for SU(2) Yang-Mills on AdS 4 Jae-Hyuk Oh at 2012 workshop for string theory and cosmology, Pusan, Korea. Dileep P. Jatkar and Jae-Hyuk.
On the exotic BTZ black holes Baocheng Zhang Based on papers PRL 110, ; PRD 88, Collaborated with Prof. P. K. Townsend 郑州,
University of Oslo & Caltech
Gauge/gravity duality in Einstein-dilaton theory Chanyong Park Workshop on String theory and cosmology (Pusan, ) Ref. S. Kulkarni,
“Applied” String Theory Pinaki Banerjee The Institute of Mathematical Sciences, Chennai Department of Physics, Visva Bharati 12 th July, 2013.
Dept.of Physics & Astrophysics
3 rd Karl Schwarzschild Meeting, Germany 24 July 2017
Quantum Mechanical Models for Near Extremal Black Holes
Scale vs Conformal invariance from holographic approach
Unitarity constraints on h/s
Thermodynamic Volume in AdS/CFT
A rotating hairy BH in AdS_3
Charged black holes in string-inspired gravity models
Andrej Ficnar Columbia University
Solutions of black hole interior, information paradox and the shape of singularities Haolin Lu.
Gravity from Entanglement and RG Flow
Kaluza-Klein Black Holes in 5-dim. Einstein-Maxwell Theory
Traversable wormholes in 4 dimensions
Presentation transcript:

The attractor mechanism, C-functions and aspects of holography in Lovelock gravity Mohamed M. Anber November HET bag-lunch

Outline  Introduction: the attractor mechanism  Lovelock gravity  The attractor mechanism in Gauss-Bonnet gravity in 5-D  Entropy and C-function in Einstein gravity  Entropy and C-functions in Lovelock gravity  Covariant formulation and Raychadhuri’s equation

Introduction  Black holes radiate: Bekenstein-Hawking entropy  Many approaches to count the number of states: still open question  Quantum gravity may be the resolution to this problem  String theory may be the way toward quantum gravity: black holes in string theory

Introduction  Black holes in string theory: string theory or M-theory Compactified to lower dimensions, Torous, Calabi Yau  The right entropy for SUSY black holes!!  Calabi Yau Moduli fields: massless and dangerous.  Far from the BH, moduli can take a range of continuous values. CAN ENTROPY DEPEND ON THIS BIZARRE BEHAVIOUR?  The answer is No!!, Resolution is the attractor mechanism  Near horizon

Introduction  What is the attractor mechanism?  All moduli fields are attracted to the same value at the horizon irrespective of their values at asymptotic infinity.  Entropy depends only on few parameters : Mass, angular momentum and not on the value of these moduli at infinity Attractor position Damped pendulum

Introduction  Is there a similar behavior for the non-supersymmetric case? Yes!!  Proven for classical Einstein gravity in 4-D and 5-D.

Outline Introduction: the attractor mechanism Introduction: the attractor mechanism  Lovelock gravity  The attractor mechanism in Gauss-Bonnet gravity in 5-D  Entropy and C-function in Einstein gravity  Entropy and C-functions in Lovelock gravity  Covariant formulation and Raychadhuri’s equation

Lovelock gravity  Possibility for higher dimensional space!!  The most general second order gravity in higher dimensional space.  It contains Gauss-Bonnet term: the result of compactifying certain string theories.

Lovelock gravity  Pure Lovelock of order m  Einstein Gravity  Not all terms survive in a given dimension: D=5, only m=2 (Gauss-Bonnet) survive, m=3 is a topological term

Lovelock gravity  Equation of motion  General Lovelock gravity: sum over all m

Outline Introduction: the attractor mechanism Introduction: the attractor mechanism Lovelock gravity Lovelock gravity  The attractor mechanism in Gauss-Bonnet gravity in 5-D  Entropy and C-function in Einstein gravity  Entropy and C-functions in Lovelock gravity  Covariant formulation and Raychadhuri’s equation

The attractor mechanism in Gauss-Bonnet gravity M. Anber and D. Kastor JHEP 0710:084,2007  Phenomenological Lagrangian  Spherically symmetric solution

The attractor mechanism in Gauss-Bonnet gravity  Equations of motion  Point like electric charge

The attractor mechanism in Gauss-Bonnet gravity  Effective potential  Moduli field equation  A solution: constant V_eff \phi

The attractor mechanism in Gauss-Bonnet gravity  Attractor: positive  The procedure for testing the attractor 1-Start with 2-Find black hole solution using

The attractor mechanism in Gauss-Bonnet gravity 3-Use perturbation theory to find the perturbed solution for the moduli fields about near the horizon 4-Use the perturbed Value of the moduli as a source to the Correction of a and b

The attractor mechanism in Gauss-Bonnet gravity 5-Use numerical technique to test if the solution is singularity free up to infinity

The attractor mechanism in Gauss-Bonnet gravity  Black hole solution at  Extremal : near horizon  Specific model of the potential

The attractor mechanism in Gauss-Bonnet gravity  Perturbation of  Same attractor behavior for a(r) and b(r)

The attractor mechanism in Gauss-Bonnet gravity  Numerical Results

The attractor mechanism in Gauss-Bonnet gravity

 Non-Extremal black hole: No Attractor !!

Outline Introduction: the attractor mechanism Introduction: the attractor mechanism Lovelock gravity Lovelock gravity The attractor mechanism in Gauss-Bonnet gravity in 5-D The attractor mechanism in Gauss-Bonnet gravity in 5-D  Entropy and C-function in Einstein gravity  Entropy and C-functions in Lovelock gravity  Covariant formulation and Raychadhuri’s equation

Entropy: Revisited  Entropy in Lovelock gravity (Myers and Jacobson 1993)  Any possible connection with quantum field theory?  ‘t Hooft and Susskind, Holographic principle in Einstein gravity ( Given a closed surface, we can represent all that happens inside it by degrees of freedom on this surface itself.)  Manifestation of the holographic principle AdS/CFT (Maldacena 1998)

Entropy: Revisited  Conformal description of horizon’s states (Solodukhin 1999) Use the near horizon coordinates (x-x_h) 5- The resulting near horizon theory is conformal

Entropy: Revisited 6-Use the light cone coordinates 7- Define Virasoro generators 8- Calculate Poisson’s bracket 9- quantize the calculations extension to Lovelock gravity (Cvitan, Pallua and Prester 2002)

C-functions in 2-D field theories  C-functions in the renormalization group flow in 2- D quantum field theories (Zamolodchikov 1986)  C-function is a function of the coupling of the theory that is monotonically increasing with energy.  For fixed points of the flow, corresponding to the extrema of this function, the C-function reduces to the central charge of Virasoro algebra E C

Holographic C-functions  AdS/CFT (Avarez, Gomez 1999, Susskind and Witten 1998) r AdS C(r )

C-functions in asymptotically flat Einstein gravity  C-functions in spherically symmetric and asymptotically flat spacetime (Goldstein et al 2006)  C-function (null energy condition is satisfied)

C-functions in asymptotically flat Einstein gravity  Conditions for the C-function 1-It can be evaluated on any spherical surface concentric with The horizon 2-When evaluated on the horizon of a black hole it equals its entropy 3-If certain physical conditions and certain boundary conditions are satisfied, then C is a non-decreasing function along the outward radial direction Can we find similar functions in Lovelock gravity?

Outline Introduction: the attractor mechanism Introduction: the attractor mechanism Lovelock gravity Lovelock gravity The attractor mechanism in Gauss-Bonnet gravity in 5-D The attractor mechanism in Gauss-Bonnet gravity in 5-D Entropy and C-function in Einstein gravity Entropy and C-function in Einstein gravity  Entropy and C-functions in Lovelock gravity  Covariant formulation and Raychadhuri’s equation

C-function in Lovelock gravity (pure) (M. Anber and D. Kastor, in progress)  Spherically symmetric metric in D=n+2 dimensions  Particular combination

C-function in Lovelock gravity (pure)  we obtain  Constraints : only local maxima, asymptotically flat.  Result: b(r) is monotonic

C-function in Lovelock gravity (pure)  But the C-function has to reduce to entropy when evaluated on horizon  C-function of the first kind

C-function in Lovelock gravity (pure)  C-function of the second kind!!  Proof outline: 1- take the derivative w.r.t r and use equations of motion to simplify the result 2- Existing of extrema require that one finds a solution for dC/dr 3-There is no solution (m=even!!)

C-function in Lovelock gravity (general)  General C-functions of the first kind  Proof of monotonicity: No solution for C’=0.

C-function in Lovelock gravity (general)  General C-functions of the second kind: Difficult to prove the monotonocity for general theory (general polynomial)  We can proove the monotonicity for Gauss-Bonnet gravity

C-function in Lovelock gravity (general)  Physical interpretation of two different C-functions!!  More C-Functions are possible??

Outline Introduction: the attractor mechanism Introduction: the attractor mechanism Lovelock gravity Lovelock gravity The attractor mechanism in Gauss-Bonnet gravity in 5-D The attractor mechanism in Gauss-Bonnet gravity in 5-D Entropy and C-function in Einstein gravity Entropy and C-function in Einstein gravity Entropy and C-functions in Lovelock gravity Entropy and C-functions in Lovelock gravity  Covariant formulation and Raychadhuri’s equation

Raychadhuri’s equation  Einstein gravity Raychadhuri’s equation Covariant holography Singularity theorems Covariant C-function Second law of thermo- dynamics n

Raychadhuri’s equation  Can we find appropriate to generalize Raychadhuri’s equation to the Lovelock gravity?

Summary and Conclusion  We have discussed the Attractor mechanism: Gauss-Bonnet gravity (Many other theories are investigated). What about brane-wrold scenarios?  C-functions in Lovelock gravity: two kinds!!. Physical interpretation (CFT??)  C-functions in Randall-Sundrum model ( with Gauss-Bonnet term)?  Covariant formulation of holographic principle in Lovelock gravity and generalized Raychadhuri’s equation.

Thank You