Disordered metals without quasiparticles, and charged black holes

Transcription

1 HARVARD Disordered metals without quasiparticles, and charged black holes String Theory: Past and Present (SpentaFest) International Center for Theoretical Sciences, Bengaluru January 11-13, 2017 Subir Sachdev Talk online: sachdev.physics.harvard.edu

2 Quantum matter with quasiparticles: Landau quasi-particles & holes Phonon Magnon Roton Plasmon Polaron Exciton Laughlin quasiparticle Bogoliubovon Anderson-Higgs mode Massless Dirac Fermions Weyl fermions.

3 Quantum matter with quasiparticles: Most generally, a quasiparticle is an additive excitation: Quasiparticles can be combined to yield additional excitations, with energy determined by the energies and densities of the constituents. Such a procedure yields all the low-lying excitations. Then we can apply the Boltzmann-Landau theory to make predictions for dynamics.

4 Quantum matter without quasiparticles: No quasiparticle structure to excitations. But how can we be sure that no quasiparticles exist in a given system? Perhaps there are some exotic quasiparticles inaccessible to current experiments.. Consider how rapidly the system loses phase coherence, reaches local thermal equilibrium, or becomes chaotic

5 Local thermal equilibration or phase coherence time, ' : There is an lower bound on ' in all many-body quantum systems as T! 0, ' >C ~ k B T, where C is a T -independent constant. Systems without quasiparticles have ' ~/(k B T ). In systems with quasiparticles, ' is parametrically larger at low T ; e.g. in Fermi liquids ' 1/T 2, and in gapped insulators ' e /(k BT ) where is the energy gap. K. Damle and S. Sachdev, PRB 56, 8714 (1997) S. Sachdev, Quantum Phase Transitions, Cambridge (1999)

6 A bound on quantum chaos: In classical chaos, we measure the sensitivity of the position at time t, q(t), to variations in the initial position, q(0), i.e. we measure =({q(t),p(0)} P.B.) By analogy, we define L as the Lyapunov time over which the wavefunction of a quantum system is scrambled by an initial perturbation. This scrambling can be measured by [Â(x, t), ˆB(0, 0)] 2 exp 1 where v B is the butterfly velocity. This time L was argued to obey lower bound 1 ~ L 2 k B T. There is no analogous bound in classical mechanics. L apple t x v B A. I. Larkin and Y. N. Ovchinnikov, JETP 28, 6 (1969) J. Maldacena, S. H. Shenker and D. Stanford, arxiv: ,

7 A bound on quantum chaos: In classical chaos, we measure the sensitivity of the position at time t, q(t), to variations in the initial position, q(0), i.e. we measure =({q(t),p(0)} P.B.) By analogy, we define L as the Lyapunov time over which the wavefunction of a quantum system is scrambled by an initial perturbation. This scrambling can be measured by [Â(x, t), ˆB(0, 0)] 2 exp 1 where v B is the butterfly velocity. This time L was argued to obey lower bound 1 ~ L 2 k B T. There is no analogous bound in classical mechanics. L apple t x v B Quantum matter without quasiparticles A. I. Larkin and Y. N. Ovchinnikov, JETP 28, 6 (1969) fastest possible many-body quantum chaos J. Maldacena, S. H. Shenker and D. Stanford, arxiv: ,

8 Disordered metals There is an extensive theory of metals in the presence of disorder and interactions (Altshuler, Aronov, Lee, Ramakrishnan, Finkelstein ) However the theory is only reliable in states in which quasiparticles are present. Often there is a flow to strong coupling, but it is invariably assumed that this leads to disordered insulators. But perhaps the strong coupling state is a metallic state without quasiparticles, in which the influence of disorder largely self averages.(there are many experimental indications this may be the case)

9 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2

10 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons L = ~ 2 k B T L = ~ 2 k B T L = ~ 2.48 k B T Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2 L : the Lyapunov time to reach quantum chaos

11 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons Same low energy theory Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2

12 SYK model H = 1 (2N) 3/2 NX i,j,k,`=1 J ij;k` c i c j c k c` µ X i c i c i c i c j + c j c i =0, c i c j + c j c i = ij Q = 1 X c N i c i 3 4 i J 3,5,7,13 J 4,5,6, J 8,9,12,14 J ij;k` are independent random variables with J ij;k` = 0 and J ij;k` 2 = J 2 N!1yields critical strange metal. 14 A. Kitaev, unpublished; S. Sachdev, PRX 5, (2015) 12 S. Sachdev and J. Ye, PRL 70, 3339 (1993)

13 SYK model Feynman graph expansion in J ij.., and graph-by-graph average, yields exact equations in the large N limit: G(i!) = 1 i! + µ (i!) G( =0 )=Q., ( ) = J 2 G 2 ( )G( ) Low frequency analysis shows that the solutions must be gapless and obey (z) =µ 1 Ap z +..., G(z) = A pz for some complex A. The ground state is a non-fermi liquid, with a continuously variable density Q. S. Sachdev and J. Ye, Phys. Rev. Lett. 70, 3339 (1993)

14 SYK and AdS2 Non-zero GPS entropy as T! 0, S(T! 0) = NS Not a ground state degeneracy: due to an exponentially small (in N) many-body level spacing at all energies down to the ground state energy. A. Georges, O. Parcollet, and S. Sachdev, PRB 63, (2001) This entropy, and other dynamic correlators of the SYK models, imply that the SYK model is holographically dual to black holes with an AdS 2 horizon. The Bekenstein- Hawking entropy of the black hole equals NS 0 : GPS = BH. S. Sachdev, PRL 105, (2010)

15 SYK and AdS2 Non-zero GPS entropy as T! 0, S(T! 0) = NS Not a ground state degeneracy: due to an exponentially small (in N) many-body level spacing at all energies down to the ground state energy. A. Georges, O. Parcollet, and S. Sachdev, PRB 63, (2001) This entropy, and other dynamic correlators of the SYK models, imply that the SYK model is holographically dual to black holes with an AdS 2 horizon. The Bekenstein- Hawking entropy of the black hole equals NS 0 : GPS = BH. S. Sachdev, PRL 105, (2010)

16 SYK and AdS2 GPS BH entropy entropy AdS 2 T 2 ds 2 =(d 2 dt 2 )/ 2 + d~x 2 Gauge field: A =(E/ )dt charge density Q T 2 = 1 ~x Einstein-Maxwell theory + cosmological constant S. Sachdev, PRL 105, (2010) Mapping to SYK applies when temperature 1/(size of T 2 )

17 SYK and AdS2 1 G(i!) =, ( ) = J 2 G 2 ( )G( ) i! + µ (i!) 1 A (z) =µ z +..., G(z) = pz Ap S. Sachdev and J. Ye, Phys. Rev. Lett. 70, 3339 (1993)

18 SYK and AdS2 1 G(i!) =, ( ) = J 2 G 2 ( )G( ) i! X + Xµ (i!) 1 A (z) =µ z +..., G(z) = pz Ap X At frequencies J, thei! + µ can be dropped, and without it equations are invariant under the reparametrization and gauge transformations = f( ) G( 1, 2 )=[f 0 ( 1 )f 0 ( 2 )] ( 1, 2 )=[f 0 ( 1 )f 0 ( 2 )] 1/4 g( 1 ) g( 2 ) e G( 1, 2) 3/4 g( 1 ) g( 2 ) e ( 1, 2) where f( ) and g( ) are arbitrary functions. A. Kitaev, unpublished S. Sachdev, PRX 5, (2015)

19 SYK and AdS2 Let us write the large N saddle point solutions of S as G s ( 1 2 ) ( 1 2 ) 1/2 s ( 1 2 ) ( 1 2 ) 3/2. The saddle point will be invariant under a reperamaterization f( ) when choosing G( 1, 2 )=G s ( 1 2 ) leads to a transformed G( e 1, 2) =G s ( 1 2 ) (and similarly for ). It turns out this is true only for the SL(2, R) transformations under which f( ) = a + b c + d, ad bc =1. So the (approximate) reparametrization symmetry is spontaneously broken down to SL(2, R) by the saddle point. A. Kitaev, unpublished

20 SYK and AdS2 Connections of SYK to gravity and AdS 2 horizons Reparameterization and gauge invariance are the symmetries of the Einstein-Maxwell theory of gravity and electromagnetism SL(2,R) is the isometry group of AdS 2. ds 2 =(d 2 + d 2 )/ 2 is invariant under 0 + i 0 = a( + i )+b c( + i )+d with ad bc = 1. A. Kitaev, unpublished

21 SYK and AdS2 Same long-time e ective action for energy and number fluctuations, involving Schwarzian derivatives of f( ). AdS 2 T 2 ds 2 =(d 2 dt 2 )/ 2 + d~x 2 Gauge field: A =(E/ )dt charge density Q T 2 = 1 ~x Einstein-Maxwell theory + cosmological constant Mapping to SYK applies when temperature 1/(size of T 2 ) J. Maldacena, D. Stanford, and Zhenbin Yang, arxiv: ; K. Jensen, arxiv: ; J. Engelsoy, T.G. Mertens, and H. Verlinde, arxiv:

22 Coupled SYK models J jklm J 0 jklm j k l m j k l m Figure 1: A chain of coupled SYK sites: each site contains N 1 fermion with SYK interaction. The coupling between nearest neighbor sites are four fermion interaction with two from each site. Yingfei Gu, Xiao-Liang Qi, and D. Stanford, arxiv: R. Davison, Wenbo Fu, A. Georges, Yingfei Gu, K. Jensen, S. Sachdev, arxiv

23 SYK and AdS2 AdS 2 T 2 ds 2 =(d 2 dt 2 )/ 2 + d~x 2 Gauge field: A =(E/ )dt charge density Q T 2 = 1 ~x Einstein-Maxwell theory + cosmological constant Mapping to SYK applies when temperature 1/(size of T 2 ) S. Sachdev, PRL 105, (2010)

24 Coupled SYK and AdS4 Y. Bardoux, M. M. Caldarelli, and C. Charmousis, JHEP 05 (2012) 054; D. Vegh, arxiv: ; R. A. Davison, PRD 88 (2013) ; M. Blake and D. Tong, PRD 88 (2013), ; T. Andrade and B. Withers, JHEP 05 (2014) 101; M. Blake, PRL 117, (2016). AdS 2 R 2 ds 2 =(d 2 dt 2 )/ 2 + d~x 2 Gauge field: A =(E/ )dt charge density Q R 2 R. Davison, Wenbo Fu, A. Georges, Yingfei Gu, K. Jensen, S. Sachdev, arxiv = 1 ~x S = Z d 4 x p ĝ ˆR +6/L X i=1 (@ ˆ' i ) ˆF µ ˆF µ!, Einstein-Maxwell-axion theory with saddle point ˆ' i = kx i leading to momentum disspation

25 Coupled SYK and AdS4 Matching correlators for thermoelectric di usion, and quantum chaos L = ~/(2 k B T ), v B T 1/2, and thermal di usivity D E = v 2 B L AdS 2 R 2 ds 2 =(d 2 dt 2 )/ 2 + d~x 2 Gauge field: A =(E/ )dt charge density Q R 2 R. Davison, Wenbo Fu, A. Georges, Yingfei Gu, K. Jensen, S. Sachdev, arxiv = 1 ~x S = Z d 4 x p ĝ ˆR +6/L X i=1 (@ ˆ' i ) ˆF µ ˆF µ Einstein-Maxwell-axion theory with saddle point ˆ' i = kx i leading to momentum disspation!,

26 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2

27 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons L = ~ 2 k B T L = ~ 2 k B T Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2 L : the Lyapunov time to reach quantum chaos

28 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons L = ~ 2 k B T v B T 1/2 L = ~ 2 k B T v B T 1/2 Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2 L : the Lyapunov time to reach quantum chaos v B : the butterfly velocity for the spatial propagation of chaos

29 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons L = ~ 2 k B T v B T 1/2 D E = v 2 B L L = ~ 2 k B T v B T 1/2 D E = v 2 B L Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2 L : the Lyapunov time to reach quantum chaos v B : the butterfly velocity for the spatial propagation of chaos

30 Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models L = ~ 2 k B T v B T 1/2 D E = v 2 B L Black holes with AdS2 horizons L = ~ 2 k B T v B T 1/2 D E = v 2 B L A. A. Patel and S. Sachdev, arxiv: L = ~ 2.48 k B T Nv5/3 F 1/3 T 4/3 1/3 v B e D (r i~a) 2 E =0.42vB 2 L ia 2m Fermi surface coupled to a gauge field µ + 1 2g 2 (r ~a)2 L : the Lyapunov time to reach quantum chaos v B : the butterfly velocity for the spatial propagation of chaos

31 L : the Lyapunov time to reach quantum chaos v B : the butterfly velocity for the spatial propagation of chaos Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models Black holes with AdS2 horizons Thermal di usivity, D E : D E = (universal number) vb 2 L in all three models Fermi surface coupled to a gauge field ia (r i~a) 2 2m µ + 1 2g 2 (r ~a)2

32 Quantum chaos is intimately linked to the loss of phase coherence from electron-electron interactions. As the time derivative of the local phase is determined by the local energy, phase fluctuations and chaos are linked to interaction-induced energy fluctuations, and hence thermal di usivity.

33 L : the Lyapunov time to reach quantum chaos v B : the butterfly velocity for the spatial propagation of chaos Quantum matter without quasiparticles: The Sachdev-Ye-Kitaev (SYK) models L = ~ 2 k B T v B T 1/2 D E = v 2 B L Black holes with AdS2 horizons L = ~ 2 k B T v B T 1/2 D E = v 2 B L L = ~ 2.48 k B T Nv5/3 F 1/3 T 4/3 1/3 v B e D (r i~a) 2 E =0.42vB 2 L ia 2m Fermi surface coupled to a gauge field µ + 1 2g 2 (r ~a)2