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Quantum Criticality and Black Holes Talk online: sachdev.physics.harvard.edu Talk online: sachdev.physics.harvard.edu.

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Presentation on theme: "Quantum Criticality and Black Holes Talk online: sachdev.physics.harvard.edu Talk online: sachdev.physics.harvard.edu."— Presentation transcript:

1 Quantum Criticality and Black Holes Talk online: sachdev.physics.harvard.edu Talk online: sachdev.physics.harvard.edu

2 Markus Mueller, Harvard Lars Fritz, Harvard Subir Sachdev, Harvard Markus Mueller, Harvard Lars Fritz, Harvard Subir Sachdev, Harvard Particle theorists Condensed matter theorists Sean Hartnoll, KITP Christopher Herzog, Princeton Pavel Kovtun, Victoria Dam Son, Washington Sean Hartnoll, KITP Christopher Herzog, Princeton Pavel Kovtun, Victoria Dam Son, Washington

3 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

4 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

5 The cuprate superconductors

6 Antiferromagnetic (Neel) order in the insulator No entanglement of spins

7 Antiferromagnetic (Neel) order in the insulator Excitations: 2 spin waves (Goldstone modes)

8 Weaken some bonds to induce spin entanglement in a new quantum phase J J/

9 Ground state is a product of pairs of entangled spins. J J/

10 Excitations: 3 S=1 triplons J J/

11 J Excitations: 3 S=1 triplons

12 J J/ Excitations: 3 S=1 triplons

13 J J/ Excitations: 3 S=1 triplons

14 J J/ Excitations: 3 S=1 triplons

15 Quantum critical point with non-local entanglement in spin wavefunction

16 CFT3

17 TlCuCl 3

18 Pressure in TlCuCl 3

19 N. Cavadini, G. Heigold, W. Henggeler, A. Furrer, H.-U. Güdel, K. Krämer and H. Mutka, Phys. Rev. B 63 172414 (2001). “triplon” TlCuCl 3 at ambient pressure

20 Christian Ruegg, Bruce Normand, Masashige Matsumoto, Albert Furrer, Desmond McMorrow, Karl Kramer, Hans–Ulrich Gudel, Severian Gvasaliya, Hannu Mutka, and Martin Boehm, arXiv:0803.3720 TlCuCl 3 with varying pressure

21 S=1/2 insulator on the square lattice A.W. Sandvik, Phys. Rev. Lett. 98, 227202 (2007). R.G. Melko and R.K. Kaul, Phys. Rev. Lett. 100, 017203 (2008).

22 Phase diagram N. Read and S. Sachdev, Phys. Rev. Lett. 62, 1694 (1989). T. Senthil, A. Vishwanath, L. Balents, S. Sachdev and M.P.A. Fisher, Science 303, 1490 (2004). S=1/2 insulator on the square lattice A.W. Sandvik, Phys. Rev. Lett. 98, 227202 (2007). R.G. Melko and R.K. Kaul, Phys. Rev. Lett. 100, 017203 (2008).

23 Theory for loss of Neel order

24 Phase diagram S=1/2 insulator on the square lattice

25 RG flow of gauge coupling: CFT3

26 d-wave superconductor on the square lattice CFT3 R. K. Kaul, Y. B. Kim, S. Sachdev, and T. Senthil, Nature Physics 4, 28 (2008) R. K. Kaul, M.A. Metlitski, S. Sachdev, and C. Xu, arXiv:0804.1794

27 U(1) gauge theory with N =4 supersymmetry CFT3 N. Seiberg and E. Witten, hep-th/9607163 K.A. Intriligator and N. Seiberg, hep-th/9607207 A. Kapustin and M. J. Strassler, hep-th/9902033

28 SU(N) gauge theory with N =8 supersymmetry (SYM3)

29 Graphene

30

31 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

32 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

33 M. Greiner, O. Mandel, T. Esslinger, T. W. Hänsch, and I. Bloch, Nature 415, 39 (2002). Superfluid-insulator transition

34

35

36 Wave oscillations of the condensate (classical Gross- Pitaevski equation)

37 Dilute Boltzmann gas of particle and holes

38 CFT at T>0

39 D. B. Haviland, Y. Liu, and A. M. Goldman, Phys. Rev. Lett. 62, 2180 (1989) Resistivity of Bi films M. P. A. Fisher, Phys. Rev. Lett. 65, 923 (1990)

40 Density correlations in CFTs at T >0

41 K. Damle and S. Sachdev, Phys. Rev. B 56, 8714 (1997).

42 Density correlations in CFTs at T >0 K. Damle and S. Sachdev, Phys. Rev. B 56, 8714 (1997).

43 Density correlations in CFTs at T >0 S. Sachdev, Quantum Phase Transitions, Cambridge (1999).

44 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

45 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

46 Objects so massive that light is gravitationally bound to them. Black Holes

47 Objects so massive that light is gravitationally bound to them. Black Holes The region inside the black hole horizon is causally disconnected from the rest of the universe.

48 Black Hole Thermodynamics Bekenstein and Hawking discovered astonishing connections between the Einstein theory of black holes and the laws of thermodynamics

49 Black Hole Thermodynamics Bekenstein and Hawking discovered astonishing connections between the Einstein theory of black holes and the laws of thermodynamics

50 AdS/CFT correspondence The quantum theory of a black hole in a 3+1- dimensional negatively curved AdS universe is holographically represented by a CFT (the theory of a quantum critical point) in 2+1 dimensions Maldacena, Gubser, Klebanov, Polyakov, Witten 3+1 dimensional AdS space A 2+1 dimensional system at its quantum critical point

51 AdS/CFT correspondence The quantum theory of a black hole in a 3+1- dimensional negatively curved AdS universe is holographically represented by a CFT (the theory of a quantum critical point) in 2+1 dimensions Maldacena, Gubser, Klebanov, Polyakov, Witten 3+1 dimensional AdS space Quantum criticality in 2+1 dimensions Black hole temperature = temperature of quantum criticality

52 AdS/CFT correspondence The quantum theory of a black hole in a 3+1- dimensional negatively curved AdS universe is holographically represented by a CFT (the theory of a quantum critical point) in 2+1 dimensions Strominger, Vafa 3+1 dimensional AdS space Quantum criticality in 2+1 dimensions Black hole entropy = entropy of quantum criticality

53 AdS/CFT correspondence The quantum theory of a black hole in a 3+1- dimensional negatively curved AdS universe is holographically represented by a CFT (the theory of a quantum critical point) in 2+1 dimensions 3+1 dimensional AdS space Quantum criticality in 2+1 dimensions Quantum critical dynamics = waves in curved space Maldacena, Gubser, Klebanov, Polyakov, Witten

54 AdS/CFT correspondence The quantum theory of a black hole in a 3+1- dimensional negatively curved AdS universe is holographically represented by a CFT (the theory of a quantum critical point) in 2+1 dimensions 3+1 dimensional AdS space Quantum criticality in 2+1 dimensions Friction of quantum criticality = waves falling into black hole Son

55 P. Kovtun, C. Herzog, S. Sachdev, and D.T. Son, Phys. Rev. D 75, 085020 (2007) Collisionless to hydrodynamic crossover of SYM3

56 P. Kovtun, C. Herzog, S. Sachdev, and D.T. Son, Phys. Rev. D 75, 085020 (2007) Collisionless to hydrodynamic crossover of SYM3

57 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

58 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

59 The cuprate superconductors

60

61 Use coupling g to induce a transition to a VBS insulator

62 STM picture of a valence bond supersolid

63 Use coupling g to induce a transition to a VBS insulator CFT3 ? STM picture of a valence bond supersolid

64 Proposed generalized phase diagram

65 Nernst measurements

66 Nernst experiment Vortices move in a temperature gradient Phase slip generates Josephson voltage 2eV J = 2  h n V E J = B x v H eyey HmHm Nernst signal e y = E y /| T |

67 Nernst measurements CFT3 ?

68 Superfluid VBS Insulator Non-zero temperature phase diagram Coulomb interactions VBS Supersolid

69 Superfluid VBS Insulator Non-zero temperature phase diagram Coulomb interactions VBS Supersolid Quantum-critical dynamics in a magnetic field, at generic density, and with impurities

70 To the CFT of the quantum critical point, we add A chemical potential   A magnetic field B After the AdS/CFT mapping, we obtain the Einstein-Maxwell theory of a black hole with An electric charge  A magnetic charge A precise correspondence is found between general hydrodynamics of vortices near quantum critical points and solvable models of black holes with electric and magnetic charges S.A. Hartnoll, P.K. Kovtun, M. Müller, and S. Sachdev, Phys. Rev. B (2007)

71 From these relations, we obtained results for the transport co-efficients, expressed in terms of a “cyclotron” frequency and damping: S.A. Hartnoll, P.K. Kovtun, M. Müller, and S. Sachdev, Phys. Rev. B 76 144502 (2007)

72 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

73 1. CFT3s in condensed matter physics and string theory Antiferromagnetic ordering transitions, graphene.... 2. Quantum-critical transport Collisionless-t0-hydrodynamic crossover of CFT3s 3. Black Hole Thermodynamics Connections to quantum criticality 4. Generalized magnetohydrodynamics Quantum criticality and dyonic black holes 5. Experiments The cuprate superconductors and graphene

74 Y. Wang, L. Li, and N. P. Ong, Phys. Rev. B 73, 024510 (2006). Theory for LSCO Experiments

75 Measurement of (T small) Y. Wang et al., Phys. Rev. B 73, 024510 (2006).

76 LSCO Experiments Measurement of (T small) Y. Wang et al., Phys. Rev. B 73, 024510 (2006).

77 77 LSCO Experiments Measurement of (T small) Y. Wang et al., Phys. Rev. B 73, 024510 (2006). T-dependent cyclotron frequency! 0.035 times smaller than the cyclotron frequency of free electrons (at T=35 K) Only observable in ultra-pure samples where. → Prediction for  c :

78 Cyclotron resonance in graphene Conditions to observe resonance Negligible Landau quantization Hydrodynamic, collison-dominated regime Negligible broadening Relativistic, quantum critical regime } M. Mueller, and S. Sachdev, arXiv:0801.2970.

79

80 Theory for transport near quantum phase transitions in superfluids and antiferromagnets Exact solutions via black hole mapping have yielded first exact results for transport co- efficients in interacting many-body systems, and were valuable in determining general structure of hydrodynamics. Theory of Nernst effect near the superfluid- insulator transition, and connection to cuprates. Quantum-critical magnetotransport in graphene. Theory for transport near quantum phase transitions in superfluids and antiferromagnets Exact solutions via black hole mapping have yielded first exact results for transport co- efficients in interacting many-body systems, and were valuable in determining general structure of hydrodynamics. Theory of Nernst effect near the superfluid- insulator transition, and connection to cuprates. Quantum-critical magnetotransport in graphene. Conclusions


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