General Relativity and the Cuprates Gary Horowitz UC Santa Barbara GH, J. Santos, D. Tong, 1204.0519, 1209.1098 GH and J. Santos, 1302.6586 Gary Horowitz.

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General Relativity and the Cuprates Gary Horowitz UC Santa Barbara GH, J. Santos, D. Tong, , GH and J. Santos, Gary Horowitz UC Santa Barbara GH, J. Santos, D. Tong, , GH and J. Santos,

Gauge/gravity duality can reproduce many properties of condensed matter systems, even in the limit where the bulk is described by classical general relativity: 1)Fermi surfaces 2)Non-Fermi liquids 3)Superconducting phase transitions 4)… It is not clear why it is working so well.

Can one do more than reproduce qualitative features of condensed matter systems? Can gauge/gravity duality provide a quantitative explanation of some mysterious property of real materials? We will argue that the answer is yes!

Plan: Calculate the optical conductivity of a simple holographic conductor and superconductor with lattice included. Earlier work on the effects of a lattice by many groups, e.g., Kachru et al; Maeda et al; Hartnoll and Hofman; Zaanen et al.; Siopsis et al., Flauger et al Main result: We will find surprising similarities to the optical conductivity of some cuprates.

Note: (1) For (2) In the limit : This can be derived more generally from Kramers-Kronig relation.

Our gravity model We start with just Einstein-Maxwell theory: This is the simplest context to describe a conductor. We require the metric to be asymptotically anti-de Sitter (AdS)

Want finite temperature: Add black hole Want finite density: Add charge to the black hole. The asymptotic form of A t is μ is the chemical potential and ρ is the charge density in the dual theory.

Introduce the lattice by making the chemical potential be a periodic function: We numerically find solutions with smooth horizons that are static and translationally invariant in one direction.

Charge density for A 0 = ½, k 0 = 2, T/μ =.055 Solutions are rippled charged black holes.

To compute the optical conductivity using linear response, we perturb the solution Boundary conditions: ingoing waves at the horizon δg μν normalizable at infinity δA t ~ O(z), δA x = e -iωt [E/iω + J z + …] induced current Conductivity

Review: optical conductivity with no lattice (T/μ =.115)

With the lattice, the delta function is smeared out

The low frequency conductivity takes the simple Drude form:

Intermediate frequency shows scaling regime: Lines show 4 different temperatures:.033 < T/μ <.055

Comparison with the cuprates (van der Marel, et al 2003)

What happens in the superconducting regime? We now add a charged scalar field to our action: Gubser (2008) argued that at low temperatures, charged black holes would have nonzero Φ. Hartnoll, Herzog, GH (2008) showed this was dual to a superconductor (in homogeneous case).

The scalar field has mass m 2 = -2/L 2, since for this choice, its asymptotic behavior is simple: This is dual to a dimension 2 charged scalar operator O with source ϕ 1 and = ϕ 2. We set ϕ 1 = 0. For electrically charged solutions with only A t nonzero, the phase of Φ must be constant.

We keep the same boundary conditions on A t as before: Start with previous rippled charged black holes with Φ = 0 and lower T. When do they become unstable? Onset of instability corresponds to a static normalizable mode of the scalar field. This can be used to find T c.

Having found T c, we now find solutions for T < T c numerically. These are hairy, rippled, charged black holes. From the asymptotic behavior of Φ we read off the condensate as a function of temperature.

Condensate as a function of temperature Lattice amplitude grows from 0 (inner line) to 2.4 (outer line).

We again perturb these black holes as before and compute the conductivity as a function of frequency. Find that curves at small ω are well fit by adding a pole to the Drude formula The lattice does not destroy superconductivity (Siopsis et al, 2012; Iizuka and Maeda, 2012) Superfluid component Normal component

Fit to: superfluid density normal fluid density

The dashed red line through ρ n is a fit to: with Δ = 4 T c. This is like BCS with thermally excited quasiparticles but: (1)The gap Δ is much larger, and comparable to what is seen in the cuprates. (2)Some of the normal component remains even at T = 0 (this is also true of the cuprates).

Intermediate frequency conductivity again shows the same power law: T/T c = 1,.97,.86,.70 Coefficient B and exponent 2/3 are independent of T and identical to normal phase.

8 samples of BSCCO with different doping. Each plot includes T T c. No change in the power law. (Data from Timusk et al, 2007.)

Preliminary results on a full 2D lattice (T > T c ) show very similar results to 1D lattice. The optical conductivity in each lattice direction is nearly identical to the 1D results.

Our simple gravity model reproduces many properties of cuprates: Drude peak at low frequency Power law fall-off ω -2/3 at intermediate ω Gap 2Δ = 8 T c Normal component doesn’t vanish at T = 0

But key differences remain Our superconductor is s-wave, not d-wave Our power law has a constant off-set C …