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Pushing and pinching charge at strong coupling Talk at Univ. of - PowerPoint PPT Presentation

Pushing and pinching charge at strong coupling Talk at Univ. of Liverpool Aristomenis Donos Durham University April 2015 Based on: 1311.3292, 1401.5077, 1406.4742 with J. P. Gauntlett 1406.1659 with M. Blake 1412.2003 with M. Blake and


  1. “Pushing and pinching charge at strong coupling” Talk at Univ. of Liverpool Aristomenis Donos Durham University April 2015 Based on: 1311.3292, 1401.5077, 1406.4742 with J. P. Gauntlett 1406.1659 with M. Blake 1412.2003 with M. Blake and D. Tong

  2. Outline 1 Introduction/Motivation 2 The Holographic Lab 3 Holographic Charge Oscillations 4 Summary / Outlook

  3. Outline 1 Introduction/Motivation 2 The Holographic Lab 3 Holographic Charge Oscillations 4 Summary / Outlook

  4. Introduction/Motivation Some fun homework for the holographista: Part I Incoherent transport Anomalous scaling of Hall angle Part II Charge screening in holographic theories

  5. Charge transport in real materials Drude peak σ Incoherent metal Mott insulator ω eV Materials with charged d.o.f. can be Coherent metals with a well defined Drude peak Insulators Incoherent conductors of electricity Interactions expected to become important in the incoherent phase → Possible description in AdS/CFT?

  6. The Cuprates The Cuprates are real life example of : Incoherent transport Anomalous scaling of conductivity and Hall angle with T θ H ∝ T − 2 ρ DC ∝ T,

  7. Anomalous Hall angle scaling Introducing a magnetic field B results in currents in two directions J x and J y . There is σ xx and σ yx Hall angle is θ H = σ xy /σ xx Fermi liquids + lattice Umklapp scattering lead to σ B =0 DC ∼ T − 2 , θ H ∼ T − 2 More generally, slow momentum relaxation predicts σ B =0 and DC θ H scale the same way with temperature [Hartnoll, Kovtun, Muller, Sachdev] Strange metals surprisingly have σ B =0 DC ∼ T − 1 , θ H ∼ T − 2 Holography evades that? Yes!

  8. Outline 1 Introduction/Motivation 2 The Holographic Lab 3 Holographic Charge Oscillations 4 Summary / Outlook

  9. AdS/CMT The recipe says: Field Theory Bulk Start with CFT d AdS d +1 Asymptotics Chemical potential µ U (1) electric charge Finite T Killing horizon 2-point function G JJ ( ω ) Bulk perturbation δA x , . . . Use Kubo’s formula σ ( ω ) = G JJ ( ω ) ıω

  10. Perfect Holographic Conductor Do it in D = 4 Einstein-Maxwell with AdS asymptotics: L EM = R − 1 4 F µν F µν + 12 4 = − U ( r ) dt 2 + U ( r ) − 1 dr 2 + r 2 � ds 2 dx 2 1 + dx 2 � 2 A = a ( r ) dt Background black hole has temperature T , energy E , pressure P , entropy s and charge q .

  11. Perfect Holographic Conductor To calculate conductivity need to source δA x = − e − ıωt E x ıω on the boundary Momentum ( δg tx ) couples because of background charge Infalling BC ( T s ) 2 q 2 ω << µ ⇒ σ = j/E x = ı E + P + ( E + P ) 2 ω [Hartnoll, Herzog] Conserved momentum → Infinite DC conductivity → Explicitly break translations on the boundary theory

  12. Classical Drude model (Missing) Physics at ω << µ Average momentum obeys p � = qE − 1 τ � ˙ τ � p � ⇒ � p � 0 = qE 1 − ıωτ σ = nq 2 J = nq � p � τ m ⇒ J = σ E ⇒ m 1 − ıωτ Without collisions τ → ∞ ⇒ σ = nq 2 δ ( ω ) + ı � � m ω

  13. Classical Drude model This is how it looks like 1.0 0.5 0.8 0.4 0.6 0.3 Re [ σ ] Im [ σ ] 0.4 0.2 0.2 0.1 0.0 0.0 0.00 0.05 0.10 0.15 0.20 0.00 0.05 0.10 0.15 0.20 ω ω

  14. Fourier/Ohm law Apart from electric currents one also has a thermal current Q More generally, transport coefficients are packaged in a matrix � J � � � � � σ αT E = Q αT ¯ κT ¯ − ( ∇ T ) /T With ∇ T a temperature gradient

  15. Holographic Lattice To add momentum dissipation introduce a UV - IR benign lattice: Keep UV fixed point ⇒ relevant deformation O ( x ) Drude physics ⇒ T = 0 horizon restores translations Charge density is a universal relevant operator ⇒ Impose A t = µ ( x ) − J t ( x ) r − 1 + · · · [Hartnoll, Hofman][Horowitz, Santos, Tong] µ ( x ) = µ 0 + A ( x ) , � A � L = 0 µ 0 ⇒ chemical potential, A ′ ( x ) ⇒ periodic electric field

  16. Inhomogeneous Lattices The task is: 1) Solve elliptic non-linear PDEs to find background rippled black holes 2) Solve non-elliptic linear PDEs to find perturbations around numerical background to extract conductivity [Horowitz, Santos, Tong] [D&G] ⇒

  17. Inhomogeneous Lattices The task is: 1) Solve elliptic non-linear PDEs to find background rippled black holes 2) Solve non-elliptic linear PDEs to find perturbations around numerical background to extract conductivity [Horowitz, Santos, Tong] [D&G]

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