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Metal - Insulator transition in holography Aristomenis Donos Imperial College London Talk at CCTP April, 2013 Based on arXiv:1212.2998 with S. Hartnoll Aristomenis Donos Metal - Insulator transition in holography Outline 1


  1. Metal - Insulator transition in holography Aristomenis Donos Imperial College London Talk at CCTP April, 2013 Based on arXiv:1212.2998 with S. Hartnoll Aristomenis Donos Metal - Insulator transition in holography

  2. Outline 1 Introduction/Motivation 2 Devising a Metal-Insulator transition in holography 3 A concrete example 4 Summary - Plans Aristomenis Donos Metal - Insulator transition in holography

  3. Outline 1 Introduction/Motivation 2 Devising a Metal-Insulator transition in holography 3 A concrete example 4 Summary - Plans Aristomenis Donos Metal - Insulator transition in holography

  4. Holographic Phases Analyse the behavior of strongly coupled CFTs when held at finite temperature and charge density and/or in a uniform magnetic field. Construct charged black hole solutions with AdS asymptotics Calculate the free energies and deduce the phase diagram What type of thermal phases are possible? What kind of zero temperature ground states can we have? Do we find interesting new behaviour in the far IR? e.g. Lifshitz, Schrodinger, hyperscaling violating, ..., something new?? Analyse hydrodynamics and transport Aristomenis Donos Metal - Insulator transition in holography

  5. Holographic phases Superconductivity/Superfluidity: [Gubser] , [Hartnoll, Herzog, Horowitz] A bulk charged scalar takes a VEV giving mass to the U (1) gauge field e.g. s-wave superconductors Higher rank charged fields take a VEV giving rise to anisotropic superfluidity order e.g. p-wave, d-wave superconductors Spatially modulated phases: [Domokos, Harvey] , [Nakamura, Oogiru, Park] , [AD, Gauntlett, Pantelidou] , [Bergman, Jokela, Lifschytz, Lippert] , [Iizuka, Kachru, Kundu, Narayan, Sircar, Trivedi] A neutral/charged bulk field takes a modulated VEV breaking spatial translations Current/Momentum density waves, CDWs, FFLO-like Aristomenis Donos Metal - Insulator transition in holography

  6. Metal-Insulator transition Drude peak σ Incoherent metal Mott insulator ω eV Materials with charged d.o.f. can be conductors or insulators At the transition a bad metallic phase can appear Strong coupling dynamics suggested to take place → answer in AdS/CFT? Aristomenis Donos Metal - Insulator transition in holography

  7. Linear response in holography Can we carry out such “experiments” in holography? Describes field theories at strong coupling Allows for the calculation of correlators e.g. G R O 1 O 2 ( ω, k ) by studying small perturbations around a black hole background Kubo’s formula for linear response allows the direct computation of the optical conductivity σ = 1 ıω G R J x J x ( ω, k = 0) Use to study transport of phases of holographic matter Aristomenis Donos Metal - Insulator transition in holography

  8. Holographic metals Consider bulk theory with metric g µν a cosmological constant and a U (1) gauge field A µ Study CFT → asymptote to AdS 4 Deform by chemical potential → A µ ≈ µ dt + · · · Finite temperature → regular Killing horizon In D = 4 Einstein-Maxwell theory L EM = √− g � 1 2 R + 6 − 1 � 4 F µν F µν the above translate to the AdS-RN black brane 4 = − g ( r ) dt 2 + g ( r ) − 1 dr 2 + r 2 � ds 2 dx 2 1 + dx 2 � 2 � r + + + µ 2 r + µ 2 r 2 � 1 − r + � � g = 2 r 2 − 2 r 2 + A = µ dt , 2 r 2 r 2 Aristomenis Donos Metal - Insulator transition in holography

  9. Holographic metals Calculate conductivity for the resulting charged medium [Hartnoll] 1.2 2.0 1.0 1.5 0.8 1.0 Re � Σ � 0.6 Im � Σ � 0.5 0.4 0.0 0.2 � 0.5 0.0 0 5 10 15 20 25 0 5 10 15 20 25 Ω � T Ω � T The chemical potential breaks the 1 + 2 dim Poincare group down to T t × E (2) The delta function Re [ σ ( ω )] ∝ δ ( ω ) reflects the translational invariance of the background → have to couple the current to heavy degrees of freedom → natural by breaking translations Aristomenis Donos Metal - Insulator transition in holography

  10. Outline 1 Introduction/Motivation 2 Devising a Metal-Insulator transition in holography 3 A concrete example 4 Summary - Plans Aristomenis Donos Metal - Insulator transition in holography

  11. Holographic metals At T = 0 the RN-AdS black brane becomes an interpolating solution × Finite entropy at T = 0, OK for field theories at large N (?) � Finite spectral weight at ω = 0, k � = 0 ! Einstein-Maxwell-Scalar theories have solutions conformal to AdS 2 × R 2 with zero entropy and finite spectral weight at ω = 0, k � = 0 [Charmousis, Gouteraux, Kim, Kiritsis, Meyer] , [Hartnoll, Shoughoulian] Aristomenis Donos Metal - Insulator transition in holography

  12. Holographic metals In order to maintain the same low and high energy physics we need to have a UV-IR benign lattice: Introduce a UV relevant deformation O ( x ) The IR operator should be irrelevant with respect to AdS 2 Solve the PDEs and show that the IR remains AdS 2 × R 2 Natural choice for the lattice operators is to have a non-uniform chemical potential in a spatial direction: µ ( x ) = µ 0 + A 0 cos( k L x ) Can check that only involves irrelevant AdS 2 operators in Einstein-Maxwell theory with dimensions ∆ i ( k L , µ 0 ) > 1 / 2. Aristomenis Donos Metal - Insulator transition in holography

  13. Holographic metals Calculating the conductivity with respect to the background deformed by the lattice resolves the low ω delta function to a Drude peak Re � Σ � Im � Σ � 3.5 1.5 3.0 2.5 1.0 2.0 1.5 0.5 1.0 0.5 Ω Ω 0.2 0.4 0.6 0.8 1.0 1.2 1.4 0.2 0.4 0.6 0.8 1.0 1.2 1.4 Μ Μ The resistivity ρ = Re [ σ (0)] − 1 is a power law ρ ∝ T ∆( k L ,µ ) for small T [Hartnoll, Hofman] Mid-infrared power law | σ | ∝ ω − 2 / 3 + C [Horowitz, Santos, Tong] Aristomenis Donos Metal - Insulator transition in holography

  14. Metal-Insulator transition In Einstein-Maxwell the picture inferred from the AdS 2 spectrum ∆ i ( k L , µ 0 ) > 1 / 2 is In order to flow to an insulator, localization effects have to be important The translation breaking lattice has to break the translations of the E (2) group in the IR. One way is if ∆ i ( k L , µ 0 ) < 1 / 2 for some values of k L . Aristomenis Donos Metal - Insulator transition in holography

  15. Outline 1 Introduction/Motivation 2 Devising a Metal-Insulator transition in holography 3 A concrete example 4 Summary - Plans Aristomenis Donos Metal - Insulator transition in holography

  16. Technical simplification We consider theories deformed by chemical potential µ and a lattice. To avoid having to solve PDEs: Consider 1 + 3 dimensional CFTs ⇒ 5 bulk dimensions Uniform potential µ breaks the Poincare group to T t × E (3), we still need to break translations of E (3) To reduce the problem to ODEs keep the constant bulk radius slices homogeneous → Keep ∂ x 2 , ∂ x 3 and p − 1 ∂ x 1 + ( x 2 ∂ x 3 − x 3 ∂ x 2 ) Give a helical structure to preserve a Bianchi VII 0 subgroup Aristomenis Donos Metal - Insulator transition in holography

  17. The model Consider model with a metric g µν , a U (1) gauge field A µ and a (not too massive) 1-form B µ 4 W ab W ab − m 2 d 5 x √− g � R + 12 − 1 4 F ab F ab − 1 � � 2 B a B a S = − κ � B ∧ F ∧ W 2 A µ used to deform by a uniform chemical potential B µ used to introduce helical “lattice” CS coupling κ helps to flow to an insulating geometry Will consider m 2 = 0 Aristomenis Donos Metal - Insulator transition in holography

  18. The ansatz Making the consistent ansatz A = a ( r ) dt , B = w ( r ) ω 2 , ds 2 = − U ( r ) dt 2 + dr 2 U ( r ) + e 2 v 1 ( r ) ω 2 1 + e 2 v 2 ( r ) ω 2 2 + e 2 v 3 ( r ) ω 2 3 with the left-invariant Killing one-forms ω 2 + i ω 3 = e ipx 1 ( dx 2 + idx 3 ) ω 1 = dx 1 , yields a non-linear system of ODEs for the radial functions. Basic ingredients for a metallic state are captured: AdS 5 with a = w = 0, U = r 2 and v i = ln r √ AdS 2 × R 3 with w = 0, a = 2 6 r , U = 12 r 2 and v i = 0 Aristomenis Donos Metal - Insulator transition in holography

  19. RG flows Close to the AdS 5 the boundary conditions are fixed by the deformation parameters µ , λ and p w = λ + β − λ p 2 / 2 log r a = µ + ν r 2 + · · · , + · · · , r 2 U = r 2 − ǫ/ 3 + p 2 λ 2 / 6 log r + · · · r 2 v i = log r + g i + s i λ 2 p 2 / 24 log r + · · · r 4 In the IR of the geometry we impose boundary conditions for the existence of a regular black horizon at temperature T What are the possible zero temperature IR behaviors? Always AdS 2 × R 3 with varying λ and p ? Aristomenis Donos Metal - Insulator transition in holography

  20. RG flows Instructive to find the spectrum of operators on AdS 2 × R 3 . Perturb the background as √ U = 12 r 2 (1 + ε u 1 r δ ) , v i = v o (1 + ε v i 1 r δ ) , a = 2 6 r (1 + ε a 1 r δ ) w = ε w 1 r δ for small ε and find the values for δ . They come in pairs δ ( i ) ± ( p ) = − 1 / 2 ± ν ( i ) ( p ), for stable solutions ν ( i ) ( p ) ≥ 0 To “shoot out” from AdS 2 × R 3 we need to use to modes with δ ( i ) + ( p ) ≥ 0 If one of the modes is relevant δ ( j ) + ( p ) < 0, a flow cannot exist Aristomenis Donos Metal - Insulator transition in holography

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