Presentation on theme: "Holographic Superconductors with Higher Curvature Corrections Sugumi Kanno (Durham) work w/ Ruth Gregory (Durham) Jiro Soda (Kyoto) arXiv:0907.3203, to."— Presentation transcript:
Holographic Superconductors with Higher Curvature Corrections Sugumi Kanno (Durham) work w/ Ruth Gregory (Durham) Jiro Soda (Kyoto) arXiv:0907.3203, to appear in JHEP
Introduction 1 It would be very exciting if we could explain high temperature superconductivity from black hole physics. We verify this numerically and analytically. According to holographic superconductors, scalar condensation in black hole system exists. This deserves further study in relation to the “no-hair” theorem from gravity perspective. Holographic Superconductors Since the stringy corrections in the bulk corresponds to the fluctuations from large N limit in holographic superconductors, it is expected the stringy corrections make holographic condensation harder. Hartnoll, Herzog & Horowitz (2008) ・ the critical temperature is stable under stringy corrections. What we are interested in is if ・ the universal relation between and : is stable under stringy corrections. Horowitz & Roberts (2008) : The gap in the frequency dependent conductivity
Gauss-Bonnet Black Hole 2 Action BH solutions Hawking temperature Gauss-Bonnet term Coupling constant >0 Constant of integration related to the ADM mass of BH Asymptotically vanishes. Horizon is at When r H (=M ) decreases, temperature decreases (This is a nature of AdS spacetime) … Chern-Simons limit
Gauss-Bonnet Superconductors – probe limit 3 Action (Maxwell field & charged complex scalar field) EOMs Regularity at Horizon (2) : Asymtotic behaviors Boundary condition in the asymptoric AdS region (2) : EOMs are nonlinear and coupled Static ansatz: Mass of the scalar filed Need 4 boundary conditions Const. of Integrations Solutions are completely determined determined According to AdS/CFT, we can interpret, so we want to calculate However… We calculate this numerically first.
Numerical Results 4 Critical Temperature decrease The effect of is to make condensation harder. increase Chern-Simons limit
Towards analytic understanding 5 E.g.) The numerical solution for Near horizon Near asymptotic AdS region b.c. Matching at somewhere
Analytic approach 6 Change variable : EOMs Near horizon (z=1) Near asymotoric AdS region (z=0) Boundary Condition Region : Solutions in the asymptotic region Boundary Condition Now, match these solutions smoothly at
Results of analytic calculation 7 Solutions Condensation is expressed by : Critical temperature Go back to the original variable : Hawking temperature AdS/CFT dictionary gives a relation : at for Numerical result Good agreement! Typical mean field theory result for the second order phase transition.
Conductivity of our boundary theory 8 Electromagnetic perturbations If we see the asymptotic behavior of this solution, in the bulk AdS/CFT Gauge fieldFour-currenton the CFT boundary Consider perturbation of and its spatial components B.c. near the horizon : ingoing wave function The system is solvable. The conductivity is given by : General solution Arbitrary scale, which can be removed by an appropriate boundary counter term Need to solve numerically with this b.c. to obtain, asymptotically.
Conductivity and Universality 9 real imaginary pole exists The universal relation is unstable in the presence of GB correction. As increases, the gap frequency becomes large.
Summary 10 The higher curvature corrections make the condensation harder. The universal relation in conductivity is unstable under the higher curvature corrections. We have found a crude but simple analytical explanation of condensation. In the future, we will take into account the backreaction to the geometry.