Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Holographic zero sound at non-zero temperature and baryon density in the Sakai-Sugimoto model Matthias Ihl Centro de Fı́sica do Porto Faculdade de Ciências da Universidade do Porto Vienna Theory Lunch Seminar, 11. 03. 2014 Holographic zero sound in the S-S model 1/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Outline of the talk Based on recent paper: B. DiNunno, M. Ihl, N. Jokela, J. Pedraza, arXiv:1403.1827 Goal: Explaining the title. Holographic zero sound at non-zero temperature and baryon density in the Sakai-Sugimoto model I What is holography? I Introduction to the Sakai-Sugimoto model. I Landau-Fermi liquids, zero sound I Zero sound in Sakai-Sugimoto at non-zero T and µ I Results Holographic zero sound in the S-S model 2/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... What is holography? I I I I Holography refers to a duality between a string theory (in the bulk) and a field theory (on the boundary) . Compare to hologram: 3D information stored in 2D picture. Original example: Maldacena duality (conjecture). N = 4 SYM in 3 + 1 dim. is dual to type IIB strings on AdS5 . Strong-weak coupling duality. Holographic zero sound in the S-S model 3/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... What is holography? AdS/CFT and AdS/CMT I AdS/CFT: Classical (weakly-coupled) theory of gravity e.g. IIB SUGRA on AdS5 × S 5 ⇔ Strongly-coupled field theory e.g. N = 4 SU(N) SYM. I Allows us to compute strongly-coupled field theory properties from gravity AdS/CFT Dictionary: Field theory ⇔ Gravity I I I I I Operators O, e.g. T µν , J µ (global sym.) ⇔ Fields φ, e.g. gµν , Aµ Expectation values ⟨O⟩ ⇔ limr →∞ φ = J + Equilibrium state ⇔ Solutions to EOMs ⟨O⟩ r + ... AdS/CMT: Application to Condensed Matter Theory, such as high-Tc superconductivity, strange metals, non-Fermi liquids, graphene etc. Holographic zero sound in the S-S model 4/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Towards (large Nc ) QCD I Original Maldacena duality: N = 4 SYM, highly symmetric. I Break some (or all) of SUSY and conformal sym. e.g., introduce non-zero temperature. I Add flavor degrees of freedom =⇒ Fundamental matter, quarks, mesons. Probe limit: Nf ≪ Nc flavor branes, no backreaction on geometry, “quenched” approx. [Karch, Katz hep-th/0205236] I Semi-realistic models of chiral symmetry breaking, deconfinement transition: e.g., Sakai-Sugimoto, [hep-th/0412141] Holographic zero sound in the S-S model 5/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Sakai-Sugimoto model of holographic QCD I I I I Introduction [Aharony, Sonnenschein, Yankielowicz hep-th/0604161] String theory dual to a field theory with chiral symmetry breaking at T = 0. IIA string theory on circle x 4 , Nc D4-branes filling 01234-directions, Nf D8-branes at x4 = 0, Nf D8-branes at du x4 = L, dx = 0 at u = u0 , U-shaped embedding x4 (u). 4 Global chiral symmetry visible as gauge theory on D8 − D8-branes. Massless spectrum of 3+1 U(Nc ) gauge theory coupled to Nf massless fermions. Holographic zero sound in the S-S model 6/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Sakai-Sugimoto model of holographic QCD Finite temp.: confinement/deconfinement transition Holographic zero sound in the S-S model 7/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Sakai-Sugimoto model of holographic QCD Phase diagram Holographic zero sound in the S-S model 8/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Landau’s Fermi liquid theory and zero sound I (non-interacting fermions: ground state is a filled Fermi sphere.) I with interactions: ground state still filled Fermi sphere of degenerate fermionic quasiparticles, provided T ≪ µ. I Quasiparticles interact over short distances ⇒ excitations more complicated. I Also: ω, k ≪ µ, excitations remain close to Fermi surface. I T=0: If quasiparticle interaction repulsive, get bosonic, longitudinal, gapless collective excitation corresponding to shape oscillations of the Fermi surface. This is the zero sound mode. I Can be characterised by dispersion relation: ωT =0 (k) = ωTR =0 (k) − iΓT =0 (k). Holographic zero sound in the S-S model 9/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Landau’s Fermi liquid theory and zero sound I I I I What happens at T ̸= 0? Thermal excitations become important for ω ∼ T , 2 thermal collisions dominate for ω ∼ Tµ . ⇒ LFLT predicts 3 different regimes: collisionless quantum (A), collisionless thermal (B) and hydrodynamic (C). Behaviour of damping rate ΓT (k) different in each regime: I (A): ΓT (k) = Γ0 (k) ∼ I (B): ΓT (k) = Γ0 (k) + ( )2 (C): ΓT (k) ∼ µ Tω . I I I k2 µ , independent 2 c Tµ . of T . Has been experimentally observed in liquid Helium-3. Question: What are the low energy properties of holographic quantum liquids (field th. states at large density of matter). How does our holographic quantum liquid at strong coupling behave compared to the (weakly-coupled) LFLT? Similarities/differences? Holographic zero sound in the S-S model 10/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... What do we want to compute? I Bosonic excitations are encoded in retarded Green’s functions of bosonic operators, GR (ω, k). Dominant poles yield dispersion relation ω(k), and correspond to field theory excitations. (Smaller imaginary part means longer-lived modes). I Can compute these from gravity by fluctuating the relevant fields around their background value and solving their equations of motion. I We will be mostly interested in (longitudinal) massless excitations coupling to the (charge) density operator which correspond to zero sound (and diffusion). Holographic zero sound in the S-S model 11/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Holographic zero sound in the Sakai-Sugimoto model. I Introduce baryon density/chemical potential by turning on a flux Ftu ̸= 0 on the world volume of the D8-branes (Au = 0): ) ( ∫ ∞ d 1 3 13 d2 du ∂u At = µ = At (u → ∞) = F , , ,− 5 . 3/2 2 1 2 10 10 uH uH 3πuH I Want to study the (longitudinal) massless excitation coupled to the density operator. This requires analyzing the linearized e.o.m.s that follow from the quadratic DBI action describing the fluctuations of the gauge fields living on the D8/D8-branes. Expand (kµ = (−ω, k, 0, 0)) ∫ d 4 k ikµ x µ µ e at (kµ , u), At (x , u) = At (u) + (2π)4 ∫ d 4 k ikµ x µ Ax (x µ , u) = e ax (kµ , u), (2π)4 I Holographic zero sound in the S-S model 12/24 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Holographic zero sound in the Sakai-Sugimoto model. I I I DBI action yields 2 equations for at and ax and one constraint equation. Introduce gauge invariant quantity E (kµ , u) := kat (kµ , u) + ωax (kµ , u) Resulting equation for E (u): ) ( 15u 4 ω 2 G ′ (u) 5 + 2 E ′ (u) E ′′ (u) + − + 2 u 2g (u) k − ω 2 G (u) ( ( )) R 3 u 2 k 2 − ω 2 G (u) − E (u) = 0, g 2 (u)f (u) where f (u) = 1 − with TH = 3uH 1/2 4πR 3/2 Holographic zero sound in the S-S model 13/24 ( uH )3 u , g (u) := and µ b= d 1/5 . 2R 3/2 √ d 2 + u 5 , G (u) = g 2 (u) , u 5 f (u) Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Holographic zero sound in the √ Sakai-Sugimoto model. I I I Change of coordinates: y = 2 rescaling y 7→ yH ye, eµ k yH kµ 7→ (dimensionless). Asymptotic behavior: near boundary, 2 local solutions: y ) + BZ II (e y ), with exponents 0 and 3. E (e y ) = AZ I (e at horizon, choose incoming-wave solution: E (e y ) = (1 − ye)−i ω̃/6 R(e y ), where R(e y ) regular at horizon. General prescription to find retarded Green’s functions: Derive boundary action twice w.r.t. source E (±k, 0) = A(±k). 9/2 2 2 B Result: GRxx (ω, k) = 6NTy R3 k 2ω−ω2 A = ωk 2 GRtt (ω, k). H I R3 u , Spectral functions: χ(ω, k) = −2Im (GR (ω, k)) . Need to numerically study quasi normal modes of the E (u) equation above; precisely those solutions satisfying incoming-wave bdy. cond. at horizon and vanish at boundary =⇒ poles of GR (ω, k). Holographic zero sound in the S-S model 14/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Quasinormal modes and dispersion relation. I Obtain dispersion relation ω(k) from the dominant poles of the correlation functions (for fixed parameters T and µ,and a given k). I Zero temperature result: [Kulaxizi, Parnachev arXiv:0811.2262] √ 2 ( ) −1+2γ+ln k π ω(k) = ± 25 k + 103/2 µ̂2 10 k 3 − i 103/2 k3 + O k5 . µ̂2 I Instability of the whole system (from transveral mode sector coupling to Chern-Simons term): for high densities, i.e. µ e ≈ 3.714 and above, the model becomes unstable towards formation of baryon charge density waves (spatially modulated phases). TH =0 Holographic zero sound in the S-S model 15/24 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Quasinormal modes and dispersion relation. Ω Non-zero temperatures (increasing) 0.01 0.00 - 0.01 0.05 0.10 0.15 k 0.20 - 0.02 - 0.03 - 0.04 - 0.05 - 0.06 Figure: Real (red dashed curve) and imaginary (blue and black solid curve) parts of the dispersion relation ω̃(k̃) for µ̃ = 5. The black solid curve indicates the more stable, longer-lived solution, with less negative imaginary part. Holographic zero sound in the S-S model 16/24 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Quasinormal modes and dispersion relation. Ω Non-zero temperatures (increasing) 0.5 0.0 - 0.5 0.5 1.0 1.5 2.0 2.5 3.0 k - 1.0 - 1.5 - 2.0 - 2.5 - 3.0 Figure: Real (red dashed curve) and imaginary (blue and black solid curve) parts of the dispersion relation ω̃(k̃) for µ̃ = 1.2. The black solid curve indicates the more stable, longer-lived solution, with less negative imaginary part. Holographic zero sound in the S-S model 17/24 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Quasinormal modes and dispersion relation. Ω Non-zero temperatures (increasing) 0.5 0.0 - 0.5 0.5 1.0 1.5 2.0 2.5 3.0 k - 1.0 - 1.5 - 2.0 - 2.5 - 3.0 Figure: Real (red dashed curve) and imaginary (blue and black solid curve) parts of the dispersion relation ω̃(k̃) for µ̃ = 0.8. At large k̃, the zero sound mode (blue solid curve) is the most stable one, but for lower k̃ another quasi-normal mode (black solid curve) becomes more stable. Holographic zero sound in the S-S model 18/24 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Behavior of ΓT I I I I Four different regimes region I (collisionless quantum): ΓT is a constant (independent of TH ) and essentially the same as for zero temperature, Γ0 . region II (collisionless thermal): ΓT ∼ TH3 . region IIIa (crossover between collisionless thermal and hydrodynamical): ΓT ∼ TH−3 . region IIIb (hydrodynamical): ΓT ∼ TH−1 , in complete agreement with high temperature diffusion result ˛ ˛ k2 . ω(k)˛ ∼ −i 2πT TH →∞ H Log GT G0 10 8 6 4 2 -8 Holographic zero sound in the S-S model 19/24 -6 -4 -2 2 -Log Μ Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Behavior of the spectral function ΧΩ2 k =5 70 000 ΧΩ2 k =5 60 000 60 000 50 000 50 000 40 000 40 000 30 000 30 000 20 000 20 000 10 000 10 000 0 0 0 2 4 Ω 6 8 10 3.00 3.05 3.10 3.15 Ω 3.20 3.25 3.30 Figure: Spectral function χxx (ω̃) (normalized by ω̃ 2 ) in region I, collisionless quantum regime, for ke = 5 and µ̃ = 10 (red), µ̃ = 15 (blue), µ̃ = 20 (orange). The sharp, distinct peaks correspond to the zero sound mode. Note that decreasing µ̃ corresponds to raising the temperature, so that the highest peak occurs for the lowest temperature and largest µ̃. Holographic zero sound in the S-S model 20/24 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Behavior of the spectral function ΧΩ2 k =0.5 10 ΧΩ2 k =0.5 1.5´106 8 1.0´106 6 500 000 0 0.300 4 2 0.305 0.310 0.315 Ω 0.320 0.325 0.330 0.335 2 4 Ω 6 8 10 Figure: Spectral function χxx (ω̃) (normalized by ω̃ 2 ) in region II, collisionless thermal regime, for ke = 0.5 and µ̃ = 11 (red), µ̃ = 13 (blue), µ̃ = 15 (orange). Holographic zero sound in the S-S model 21/24 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Results ....... Behavior of the spectral function ΧΩ2 k =0.01 25 ΧΩ2 k =0.01 8´107 20 6´107 15 4´107 10 2´107 5 0 0 0.000 0.002 0.004 0.006 0.008 Ω 0.010 0.012 0.014 5 10 Ω 15 20 Figure: Spectral function χxx (ω̃) (normalized by ω̃ 2 ) in region III, hydrodynamic regime, for ke = 0.01 and µ̃ = 5 (red), µ̃ = 10 (blue), µ̃ = 15 (orange). The hydrodynamic diffusive contribution becomes dominant compared to the remnants of the zero sound mode. Holographic zero sound in the S-S model 22/24 25 Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Absence of a Fermi surface I I Discontinuity in distribution fct. shows up as singularity at k = 2kF in the retarded Green’s ( ) ( function ) at small frequency ω: GR (ω → 0, k) ∼ 2kkF − 1 ln 2kkF − 1 . Can evaluate GR numerically in this limit, but no sign of discontinuity/Fermi surface. 40 30 Re@GR D Ω = 0 20 10 0 0 Holographic zero sound in the S-S model 23/24 1 2 k 3 4 5 Results ....... Introduction .... Sakai-Sugimoto ... LFLT .. Hol. 0-sound .... Conclusions and Outlook I I I I I Some properties of our model compatible with LFLT; spec. 5/3 heat Cv ∼ T at low T , eq. of state ∼ nB as expected for non-relativistic fermions. Stable zero sound mode with non-standard k 3 -dependence of ΓT at low and moderate T . Found interesting crossover regime between collisionless thermal and hydro regime where ΓT ∼ T −3 . No sharp Fermi surface: Either flavour back reaction effect, or no Fermi surface at all. Further research necessary to decide whether holographic QCD has a true low energy description in terms of quasiparticle excitations of a Fermi surface, or it is a novel type of strongly-coupled quantum liquid phase without Fermi surface. Thank you! Holographic zero sound in the S-S model 24/24 Results .......
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