Holographic Wilsonian RG and BH Sliding Membrane

Size: px
Start display at page:

Download "Holographic Wilsonian RG and BH Sliding Membrane"

Transcription

1 Holographic Wilsonian RG and BH Sliding Membrane based on by SJS,YZ (JHEP05:030,2011) related references: by N.Iqbal and H.Liu by Heemskerk and J.Polchinski by Faulkner,Liu and Rangamani July 7, 2011 ICTS-USTC,Hefei ang Zhou based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

2 Outline 1 Introduction: Membrane paradigm 2 Holographic Wilsonian RG (HWRG) 3 Equivalence 4 Double Trace Flow based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

3 Motivations Introduction: Membrane paradigm Map the Hamilton-Jacobi flow and Exact Wilson RG of Quantum Field Theory based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

4 Introduction: Membrane paradigm Motivations Map the Hamilton-Jacobi flow and Exact Wilson RG of Quantum Field Theory Interpolating physical quantities evaluating at horizon and at the boundary based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

5 Formulations Introduction: Membrane paradigm Many approaches to Holographic RG after 1997 (AdS=CFT, Maldacena) which I apologize for not listing here. (E.T.Akhmedov,V.Balasubramanian eta, Susskind and Witten,J.d.Boer and Verlinde 2 ) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

6 Introduction: Membrane paradigm Formulations Many approaches to Holographic RG after 1997 (AdS=CFT, Maldacena) which I apologize for not listing here. (E.T.Akhmedov,V.Balasubramanian eta, Susskind and Witten,J.d.Boer and Verlinde 2 ) Sliding membrane approach (2008, N.Iqbal and H.Liu) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

7 Introduction: Membrane paradigm Formulations Many approaches to Holographic RG after 1997 (AdS=CFT, Maldacena) which I apologize for not listing here. (E.T.Akhmedov,V.Balasubramanian eta, Susskind and Witten,J.d.Boer and Verlinde 2 ) Sliding membrane approach (2008, N.Iqbal and H.Liu) Wilsonian fluid/gravity (June.2010, Bredberg,Keeler,Lysov and Strominger.) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

8 Introduction: Membrane paradigm Formulations Many approaches to Holographic RG after 1997 (AdS=CFT, Maldacena) which I apologize for not listing here. (E.T.Akhmedov,V.Balasubramanian eta, Susskind and Witten,J.d.Boer and Verlinde 2 ) Sliding membrane approach (2008, N.Iqbal and H.Liu) Wilsonian fluid/gravity (June.2010, Bredberg,Keeler,Lysov and Strominger.) Holographic Wilsonian approach (Oct.2010,I.heemskerk and J.Polchinski; Oct.2010, T.Faulkner,M.Rangamani and H.Liu) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

9 Membrane paradigm Introduction: Membrane paradigm Black hole stretched horizon a fictitious membrane which means, to an external observer, a black hole appears to behave exactly like a dynamical fluid membrane. based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

10 Introduction: Membrane paradigm Membrane paradigm Black hole stretched horizon a fictitious membrane which means, to an external observer, a black hole appears to behave exactly like a dynamical fluid membrane. Viscous response: η = 1 16πG N (Damour,1978) (1) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

11 Introduction: Membrane paradigm Membrane paradigm Black hole stretched horizon a fictitious membrane which means, to an external observer, a black hole appears to behave exactly like a dynamical fluid membrane. Viscous response: Electric response: η = 1 16πG N (Damour,1978) (1) σ = 1 e 2 (Znajek,1978; Damour,1978) (2) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

12 Introduction: Membrane paradigm The idea is: In-falling boundary conditions can be viewed as physical properties of membrane located at the stretched horizon. based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

13 Introduction: Membrane paradigm The idea is: In-falling boundary conditions can be viewed as physical properties of membrane located at the stretched horizon. An action for membrane (Parikh and Wilczek 1998) is a surface term which cancel the boundary term action at the horizon. based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

14 Introduction: Membrane paradigm The idea is: In-falling boundary conditions can be viewed as physical properties of membrane located at the stretched horizon. An action for membrane (Parikh and Wilczek 1998) is a surface term which cancel the boundary term action at the horizon. For FFO to find a nonsingular field φ, near the horizon we have φ(r, t, x) = φ(τ, x) (3) where τ is the Eddington-Finklestein coordinate grr dτ = dt + dr. (4) g tt This implies in-falling condition r φ = grr g tt t φ at the horizon. based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

15 Introduction: Membrane paradigm For a massless scalar probe with action S scalar = 1 d d+1 x g 1 2 r>r h q(r) ( φ)2 (5) the membrane action is S surf = d d x γ( Π(r h, x) )φ(r h, x), Π mb Π(r h, x) g = rr r φ Σ γ γ q(r) (6) together with in-falling condition r φ = grr g tt t φ, give (orthonormal basis) ξ mb Π mb ˆt φ(r h) = 1 q(r h ) = 1 (ShearViscosity!) (7) 16πG N based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

16 Introduction: Membrane paradigm For a Maxwell field probe: S Maxwell = d d+1 x 1 g r>r h 4g(r) 2 F 2 (8) the membrane action is S surf = d d x γ( j µ )A µ, J µ γ mb j µ (9) γ Σ with in-falling condition F ri = grr g tt F ti, give σ mb = 1 g 2 (r h ) (MembraneConductivity!) (10) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

17 Sliding membrane Introduction: Membrane paradigm The idea is: View a cutoff surface at finite r c as a sliding membrane where the disturb and response can be defined. based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

18 Introduction: Membrane paradigm Sliding membrane The idea is: View a cutoff surface at finite r c as a sliding membrane where the disturb and response can be defined. For a massless scalar probe: ξ(r c, k µ ) = Π(r c, k µ ) iωφ(r c, k µ ) (11) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

19 Introduction: Membrane paradigm Sliding membrane The idea is: View a cutoff surface at finite r c as a sliding membrane where the disturb and response can be defined. For a massless scalar probe: ξ(r c, k µ ) = Π(r c, k µ ) iωφ(r c, k µ ) (11) For a Maxwell field probe: σ(r c, k µ ) = j i (r c, k µ ) F it (r c, k µ ) (12) based on by SJS,YZ (JHEP05:030,2011) Holographic Wilsonian related RG and references: BH Sliding Membrane July 7, by 2011 N.Iqbal ICTS-USTC,Hefei and H.Liu by/ Heem 28

20 Flow involving EOM Introduction: Membrane paradigm Using the definition, one can represent EOM: [ grr σ 2 r σ = iω (1 k2 g ii ) ] g tt Σ(r) ω 2 g tt Σ(r) (13) where Σ(r) = gg ii grr g tt (14) July 7, 2011 ICTS-USTC,Hefei 10 /

21 Flow involving EOM Introduction: Membrane paradigm Using the definition, one can represent EOM: [ grr σ 2 r σ = iω (1 k2 g ii ) ] g tt Σ(r) ω 2 g tt Σ(r) (13) where Σ(r) = gg ii grr g tt (14) Regular condition of (13) at the horizon infalling boundary condition. July 7, 2011 ICTS-USTC,Hefei 10 /

22 Flow involving EOM Introduction: Membrane paradigm Using the definition, one can represent EOM: [ grr σ 2 r σ = iω (1 k2 g ii ) ] g tt Σ(r) ω 2 g tt Σ(r) (13) where Σ(r) = gg ii grr g tt (14) Regular condition of (13) at the horizon infalling boundary condition. Smooth interpolation between Horizon value and Boundary value July 7, 2011 ICTS-USTC,Hefei 10 /

23 Flow involving EOM Introduction: Membrane paradigm Using the definition, one can represent EOM: [ grr σ 2 r σ = iω (1 k2 g ii ) ] g tt Σ(r) ω 2 g tt Σ(r) (13) where Σ(r) = gg ii grr g tt (14) Regular condition of (13) at the horizon infalling boundary condition. Smooth interpolation between Horizon value and Boundary value Even without any RG formulism, one does have flow equation for σ(r c )! July 7, 2011 ICTS-USTC,Hefei 10 /

24 Holographic Wilsonian RG (HWRG) Split path integral in the bulk Boundary Split: Z = DM kδ<1 DM kδ>1 e S = boundary boundary DM kδ<1 e S(δ) := exp( s(δ)) (15) ang Zhou July 7, 2011 ICTS-USTC,Hefei 11 /

25 Holographic Wilsonian RG (HWRG) Split path integral in the bulk Boundary Split: Z = DM kδ<1 DM kδ>1 e S = boundary boundary DM kδ<1 e S(δ) := exp( s(δ)) (15) Bulk Split: Z = Dφ z>ɛ Dφ z=ɛ Dφ z<ɛ e S IR(z>ɛ) S UV (z<ɛ) bulk = D φψ IR (ɛ, φ)ψ UV (ɛ, φ) (16) bulk July 7, 2011 ICTS-USTC,Hefei 11 /

26 Holographic Wilsonian RG (HWRG) Map between Boundary and Bulk Natural Map: Ψ IR (ɛ, φ) = DM kδ<1 exp { S 0 + 1κ 2 } d d x φ i (x)o i (x) (17) July 7, 2011 ICTS-USTC,Hefei 12 /

27 Holographic Wilsonian RG (HWRG) Map between Boundary and Bulk Natural Map: Ψ IR (ɛ, φ) = DM kδ<1 exp { S 0 + 1κ 2 } d d x φ i (x)o i (x) (17) s(δ) and S B : e s(δ) = D φe d d x φ(x)o(x) e S B (18) with S B = log Ψ UV (ɛ, φ z=ɛ ) (19) July 7, 2011 ICTS-USTC,Hefei 12 /

28 Holographic Wilsonian RG (HWRG) Holographic Wilsonian RGE Cutoff independent of full amplitude: 0 = d dɛ Z = d dɛ < e s(δ) > (20) July 7, 2011 ICTS-USTC,Hefei 13 /

29 Holographic Wilsonian RG (HWRG) Holographic Wilsonian RGE Cutoff independent of full amplitude: 0 = d dɛ Z = d dɛ < e s(δ) > (20) In the bulk level, IR dynamics plus a boundary action S B should be useful, since Wilson told us we need to integrate out the UV region. July 7, 2011 ICTS-USTC,Hefei 13 /

30 Holographic Wilsonian RG (HWRG) Holographic Wilsonian RGE Cutoff independent of full amplitude: 0 = d dɛ Z = d dɛ < e s(δ) > (20) In the bulk level, IR dynamics plus a boundary action S B should be useful, since Wilson told us we need to integrate out the UV region. Bulk HWRG equation then becomes: which gives. [ zh ] ɛ L + S B = 0 (21) ɛ ɛ S B = H IR (22) July 7, 2011 ICTS-USTC,Hefei 13 /

31 Holographic Wilsonian RG (HWRG) Holographic Wilsonian RGE ang Zhou Cutoff independent of full amplitude: 0 = d dɛ Z = d dɛ < e s(δ) > (20) In the bulk level, IR dynamics plus a boundary action S B should be useful, since Wilson told us we need to integrate out the UV region. Bulk HWRG equation then becomes: which gives. What is the power of above HWRG? [ zh ] ɛ L + S B = 0 (21) ɛ ɛ S B = H IR (22) July 7, 2011 ICTS-USTC,Hefei 13 /

32 Holographic Wilsonian RG (HWRG) Holographic Wilsionian RG flow One way to determine S B is taking use of ɛ S B [A µ, ɛ] + H IR [A µ, δs B δa µ ] = 0 (23) July 7, 2011 ICTS-USTC,Hefei 14 /

33 Holographic Wilsonian RG (HWRG) Holographic Wilsionian RG flow One way to determine S B is taking use of ɛ S B [A µ, ɛ] + H IR [A µ, δs B δa µ ] = 0 (23) For the Maxwell: S B = 1 d d k ( ) 2 (2π) d G 00 (k, ɛ)â 0 (k)â 0 ( k) + G ii (k, ɛ)â i (k)â i ( k) (24) July 7, 2011 ICTS-USTC,Hefei 14 /

34 Holographic Wilsonian RG (HWRG) Holographic Wilsionian RG flow One way to determine S B is taking use of ɛ S B [A µ, ɛ] + H IR [A µ, δs B δa µ ] = 0 (23) For the Maxwell: S B = 1 d d k ( ) 2 (2π) d G 00 (k, ɛ)â 0 (k)â 0 ( k) + G ii (k, ɛ)â i (k)â i ( k) (24) Using flow equation, we have flow equations for coefficients: ɛ G 00 = (G 00 ) 2 gg tt g zz + gg tt g ii k 2 ɛ G ii = (G ii ) 2 gg ii g zz gg tt g ii ω 2. (25) July 7, 2011 ICTS-USTC,Hefei 14 /

35 RG Solutions Holographic Wilsonian RG (HWRG) we want to find solutions for the RG equations (25). We start by assuming and 1 G 00 = 1 G 00 (0) ɛ G 00 (0) + k 2 1 G(1) 00 +, 1 G ii = 1 G(0) ii = (G 00 (0) )2 gg tt g zz, ɛg ii (0) + ω 2 1 G(1) ii + (26) (G ii (0) = )2 gg ii. (27) g zz We have the following solutions by imposing simple vanishing boundary conditions for G(1) 00, G (1) ii 1 z gg tt G(1) 00 (z) = g ii 1 z gg tt 0 G(0) 00, G(1) ii (z) = g ii 0 G(0) ii We see that k 2 and ω 2 correction are controlled by zero order solutions in the low frequency approximation.. (28) July 7, 2011 ICTS-USTC,Hefei 15 /

36 Holographic Wilsonian RG (HWRG) Flow for transport coefficient Define a transport coefficient: σ Ji E i = With the definition of current J i 0  i + i  0. (29) J µ δs B δa µ (30) July 7, 2011 ICTS-USTC,Hefei 16 /

37 Holographic Wilsonian RG (HWRG) Flow for transport coefficient Define a transport coefficient: σ Ji E i = With the definition of current From S B we have J i 0  i + i  0. (29) J µ δs B δa µ (30) Express σ by G 1 Â0 = G 00 J 0, 1 G ii = Âi J i. (31) 1 σ = i ( ) ω 2 ω G ii k2 G 00. (32) July 7, 2011 ICTS-USTC,Hefei 16 /

38 Conductivity Flow Holographic Wilsonian RG (HWRG) Using the flow equations for G coefficients we obtain ( ) ɛσ (σ iω = 2 1 k2 1 gg ii g zz ω 2 gg tt g zz ) gg tt g ii, (33) This is what we have in the sliding membrane paradigm! July 7, 2011 ICTS-USTC,Hefei 17 /

39 Conductivity Flow Holographic Wilsonian RG (HWRG) Using the flow equations for G coefficients we obtain ( ) ɛσ (σ iω = 2 1 k2 1 gg ii g zz ω 2 gg tt g zz ) gg tt g ii, (33) This is what we have in the sliding membrane paradigm! Under coordinate transformation z = 1/r, one has ɛ = r 2 r, g (z) g tt g ii = g (r) g tt g ii r 2, (34) 1 g (z) g zz g ii = 1 g (r) g rr g ii r 2. (35) July 7, 2011 ICTS-USTC,Hefei 17 /

40 Holographic Wilsonian RG (HWRG) Re Σ Im Σ Figure: r flow of AC conductivity, with d = 4 AdS-black hole background and ω = 2, 1.5, 1, from up to down in the left Figure and inversely in the right one. For d > 4 AdS-black hole, the behavior of solutions are similar. July 7, 2011 ICTS-USTC,Hefei 18 /

41 Equivalence Equivalence between HWRG and Sliding Membrane There are two RG flows. One is the flow given by the classical equation of motion, and the other is the flow from integrating out the geometry. Here we want to prove the equivalence of the two. July 7, 2011 ICTS-USTC,Hefei 19 /

42 Equivalence Equivalence between HWRG and Sliding Membrane There are two RG flows. One is the flow given by the classical equation of motion, and the other is the flow from integrating out the geometry. Here we want to prove the equivalence of the two. No split amplitude: Z 1 [φ 0 ] = Dφe S exp( S[φ c ]) (36) Split amplitude: Z 2 = bulk bulk D φψ IR (ɛ, φ)ψ UV (ɛ, φ), (37) ang Zhou July 7, 2011 ICTS-USTC,Hefei 19 /

43 Equivalence Equivalence between HWRG and Sliding Membrane There are two RG flows. One is the flow given by the classical equation of motion, and the other is the flow from integrating out the geometry. Here we want to prove the equivalence of the two. No split amplitude: Z 1 [φ 0 ] = Dφe S exp( S[φ c ]) (36) Split amplitude: Z 2 = Classical approximation: Ψ IR (ɛ, φ) = Ψ UV (ɛ, φ) = bulk bulk D φψ IR (ɛ, φ)ψ UV (ɛ, φ), (37) bulk bulk Dφ z>ɛ e S(z>ɛ) = e S IR[φ IR c ] (38) Dφ z<ɛ e S(z<ɛ) = e S UV [φ UV c ], (39) July 7, 2011 ICTS-USTC,Hefei 19 /

44 Sufficient: Equivalence Explicitly we write S ɛ [φ H, φ, φ 0 ] = S IR [φ IR c [φ H, φ]] + S UV [φ UV c [ φ, φ 0 ]]. (40) ang Zhou July 7, 2011 ICTS-USTC,Hefei 20 /

45 Sufficient: Equivalence Explicitly we write S ɛ [φ H, φ, φ 0 ] = S IR [φ IR c [φ H, φ]] + S UV [φ UV c [ φ, φ 0 ]]. (40) Z 2 = D φe Sɛ[ φ] = e Sɛ[φ H, φ,φ 0 ] (41) ang Zhou July 7, 2011 ICTS-USTC,Hefei 20 /

46 Sufficient: Equivalence Explicitly we write S ɛ [φ H, φ, φ 0 ] = S IR [φ IR c [φ H, φ]] + S UV [φ UV c [ φ, φ 0 ]]. (40) Z 2 = where φ is a solution for δs ɛ δ φ = δs UV δ φ D φe Sɛ[ φ] = e Sɛ[φ H, φ,φ 0 ] + δs IR δ φ (41) = 0, (42) which is nothing but Π IR = Π UV. Momentum continuity is ESSENTIAL for bulk classical calculation! ang Zhou July 7, 2011 ICTS-USTC,Hefei 20 /

47 Sufficient: Equivalence Explicitly we write S ɛ [φ H, φ, φ 0 ] = S IR [φ IR c [φ H, φ]] + S UV [φ UV c [ φ, φ 0 ]]. (40) Z 2 = where φ is a solution for δs ɛ δ φ = δs UV δ φ D φe Sɛ[ φ] = e Sɛ[φ H, φ,φ 0 ] + δs IR δ φ (41) = 0, (42) which is nothing but Π IR = Π UV. Momentum continuity is ESSENTIAL for bulk classical calculation! In order for Z 1 = Z 2, it is SUFFICIENT to have φ = φ c (z) z=ɛ so that φ = φ c. (43) We should also notice that it guarantees the ɛ independence of the Z 2 and S ɛ, i.e, dsɛ dɛ = 0! July 7, 2011 ICTS-USTC,Hefei 20 /

48 / :.-)*+, "#$%&' (! }~ klmnopqrstuvwxyz{j ^_àbcdefghi ]\ Necessary (on-shell) Equivalence What about the necessary part? ~ ϕ ϕh C A B ϕ0 ZH ε Z=0 Figure: Flows with (A) and without (C) the momentum continuity. The uniqueness of the smooth solution forbids a solution like B. July 7, 2011 ICTS-USTC,Hefei 21 /

49 / :.-)*+, "#$%&' (! }~ klmnopqrstuvwxyz{j ^_àbcdefghi ]\ Necessary (on-shell) Equivalence What about the necessary part? On-shell: ~ ϕ ϕh C A B ϕ0 ZH ε Z=0 Figure: Flows with (A) and without (C) the momentum continuity. The uniqueness of the smooth solution forbids a solution like B. July 7, 2011 ICTS-USTC,Hefei 21 /

50 Necessary (off-shell) Equivalence What about the off-shell case? July 7, 2011 ICTS-USTC,Hefei 22 /

51 Necessary (off-shell) Equivalence What about the off-shell case? Look at the RG again: ɛ S B [ φ] + H IR [ φ, δs B[ φ] ] = 0. (44) δ φ July 7, 2011 ICTS-USTC,Hefei 22 /

52 Necessary (off-shell) Equivalence What about the off-shell case? Look at the RG again: ɛ S B [ φ] + H IR [ φ, δs B[ φ] ] = 0. (44) δ φ Taking the derivative of eq. (??) with respect to φ we get ɛ Π φ = δh IR δ φ. (45) July 7, 2011 ICTS-USTC,Hefei 22 /

53 Necessary (off-shell) Equivalence What about the off-shell case? Look at the RG again: ɛ S B [ φ] + H IR [ φ, δs B[ φ] ] = 0. (44) δ φ Taking the derivative of eq. (??) with respect to φ we get ɛ Π φ = δh IR δ φ. (45) Momentum Continuity gives the ɛ dependence of φ Π φ = gg zz z φ(z) ɛ = gg zz ɛ ɛ φ (46) July 7, 2011 ICTS-USTC,Hefei 22 /

54 Necessary (off-shell) Equivalence What about the off-shell case? Look at the RG again: ɛ S B [ φ] + H IR [ φ, δs B[ φ] ] = 0. (44) δ φ Taking the derivative of eq. (??) with respect to φ we get ɛ Π φ = δh IR δ φ. (45) Momentum Continuity gives the ɛ dependence of φ Π φ = gg zz z φ(z) ɛ = gg zz ɛ ɛ φ (46) We recover the full EOM for φ! The equations (??) and (??) together with φ 0, φ H as the boundary condition of φ repeat the classical solution in whole bulk. July 7, 2011 ICTS-USTC,Hefei 22 /

55 Equivalence So far, we conclude that, in the bulk classical level, HWRG and sliding membrane are exactly equivalent. Basically, all bulk classical flows involve EOM. Still, the important question: how does the flow look like in boundary field theory language? ang Zhou July 7, 2011 ICTS-USTC,Hefei 23 /

56 Double Trace Flow Double Trace Flow We will obtain S B by computing on-shell UV action. Maxwell equations are written by z [ g ( z A µ µ A z ) ] + ν [ g ( ν A µ µ A ν ) ] = 0. (47) We assume A µ (z, k) = A (0) µ (z) + k 2 A (1) µ (z) + k µ k ν A (2) ν (z) + (48) and A z is independent on k. In the small momentum 0 limit, the first term will dominate and the above equation can be solved by ɛ z 0 C µ 1 = 1 Â (0) µ (z) A (0) µ (z 0 ) = z z 0 µ C1 gg zz dz. (49) g µµ (Â(0) µ (ɛ) A (0) µ,z 0 ) := f µ (Â(0) µ (ɛ) A (0) µ,z 0 ) (50) µµ dz gg zz g 1 ɛ 1 = f µ z 0 gg zz dz (51) g µµ July 7, 2011 ICTS-USTC,Hefei 24 /

57 Double Trace Flow Now, we want to integrate out z in region z 0 < z < ɛ. For the standard quadratic Maxwell action, we obtain the on-shell action as boundary term using the equations of motion: S on shell [z 0,ɛ] = 1 2 where we used z  (0) µ = d d x gg zz g µµ  c µ z  c ɛ µ = 1 z 0 2 d d x C µ ɛ 1 Âc µ. z 0 (52) C µ 1 gg zz g µµ. ϕ(x µ, z) = z z 0 A z dz, the gauge invariant field  (0) µ = A (0) µ µ ϕ. Using solution (??), we finally obtain the zero order on shell action S on shell [z 0,ɛ] = 1 d d x f µ ( µ (ɛ) A µ,z0 )( µ (ɛ) A µ,z0 ). (53) 2 µ This is S B at low frequency limit! If we set z 0 = 0. July 7, 2011 ICTS-USTC,Hefei 25 /

58 Double Trace Flow From the boundary point of view, we have deformations due to S B. Naturally, the deformed theory should be defined at ɛ, and the source should be A µ (ɛ) and the current should comes from J µ ɛ δs B δa µ,ɛ (54) July 7, 2011 ICTS-USTC,Hefei 26 /

59 Double Trace Flow From the boundary point of view, we have deformations due to S B. Naturally, the deformed theory should be defined at ɛ, and the source should be A µ (ɛ) and the current should comes from J µ ɛ δs B δa µ,ɛ (54) The Green function in linear level can be defined as G µµ ɛ = Jµ ɛ A µ,ɛ. (55) July 7, 2011 ICTS-USTC,Hefei 26 /

60 Double Trace Flow From the boundary point of view, we have deformations due to S B. Naturally, the deformed theory should be defined at ɛ, and the source should be A µ (ɛ) and the current should comes from J µ ɛ δs B δa µ,ɛ (54) The Green function in linear level can be defined as G µµ ɛ = Jµ ɛ A µ,ɛ. (55) The field theory effective action can be derived from which is given by S eff = d d x µ δs eff = 1 G κ δj J = 1 G ɛ µµ δj µ ɛ J µ ɛ. (56) [ 1 2 (Jµ ) 2 1 ] J µ (A µ,0 + µ ϕ) f µ. (57) July 7, 2011 ICTS-USTC,Hefei 26 /

61 Double Trace Flow ang Zhou From the boundary point of view, we have deformations due to S B. Naturally, the deformed theory should be defined at ɛ, and the source should be A µ (ɛ) and the current should comes from J µ ɛ δs B δa µ,ɛ (54) The Green function in linear level can be defined as G µµ ɛ = Jµ ɛ A µ,ɛ. (55) The field theory effective action can be derived from which is given by S eff = d d x µ δs eff = 1 G κ δj J = 1 G ɛ µµ δj µ ɛ J µ ɛ. (56) [ 1 2 (Jµ ) 2 1 ] J µ (A µ,0 + µ ϕ) f µ This is nothing but the Legendre transformation of S B!. (57) July 7, 2011 ICTS-USTC,Hefei 26 /

62 Double Trace Flow Double Trace Coupling flow Compare with Witten description: S B contains double trace deformation! For 4d AdS black hole 1 f i = 1 2 ɛ2, 1 = 1 ( ) 1 + ɛ 2 f 0 4 ln 1 ɛ 2 (58) July 7, 2011 ICTS-USTC,Hefei 27 /

63 Double Trace Flow Double Trace Coupling flow Compare with Witten description: S B contains double trace deformation! For 4d AdS black hole 1 f i = 1 2 ɛ2, 1 = 1 ( ) 1 + ɛ 2 f 0 4 ln 1 ɛ 2 (58) Double trace deformed Green function in linear level: J µ ɛ = G µµ ɛ A µ,ɛ, where ϕ(x µ, z) = z z 0 A z dz. 1 G µµ ɛ 1 G µµ z 0 = 1 f µ + µϕ J µ. (59) July 7, 2011 ICTS-USTC,Hefei 27 /

64 Double Trace Flow Double Trace Coupling flow Compare with Witten description: S B contains double trace deformation! For 4d AdS black hole 1 f i = 1 2 ɛ2, 1 = 1 ( ) 1 + ɛ 2 f 0 4 ln 1 ɛ 2 (58) Double trace deformed Green function in linear level: J µ ɛ = G µµ ɛ A µ,ɛ, where ϕ(x µ, z) = z z 0 A z dz. when ɛ 0, G ɛ G 0. 1 G µµ ɛ 1 G µµ z 0 = 1 f µ + µϕ J µ. (59) ang Zhou July 7, 2011 ICTS-USTC,Hefei 27 /

65 Double Trace Flow Conclusions and Future Questions HWRG and Sliding membrane flow are equivalent. July 7, 2011 ICTS-USTC,Hefei 28 /

66 Double Trace Flow Conclusions and Future Questions HWRG and Sliding membrane flow are equivalent. Double trace flow comes from integrating out UV bulk geometry. July 7, 2011 ICTS-USTC,Hefei 28 /

67 Double Trace Flow Conclusions and Future Questions HWRG and Sliding membrane flow are equivalent. Double trace flow comes from integrating out UV bulk geometry. Our Green function flow from Membrane is equivalent to Legendre transformation of S B in (I.heemskerk and J.Polchinski) July 7, 2011 ICTS-USTC,Hefei 28 /

68 Double Trace Flow Conclusions and Future Questions HWRG and Sliding membrane flow are equivalent. Double trace flow comes from integrating out UV bulk geometry. Our Green function flow from Membrane is equivalent to Legendre transformation of S B in (I.heemskerk and J.Polchinski) Open Question: what about the possible flow for non-local operator? Is it possible to establish the precise map between H-J flow and exact Wilson RG in field theory? July 7, 2011 ICTS-USTC,Hefei 28 /

69 Double Trace Flow Conclusions and Future Questions HWRG and Sliding membrane flow are equivalent. Double trace flow comes from integrating out UV bulk geometry. Our Green function flow from Membrane is equivalent to Legendre transformation of S B in (I.heemskerk and J.Polchinski) Open Question: what about the possible flow for non-local operator? Is it possible to establish the precise map between H-J flow and exact Wilson RG in field theory? Quick Question: Does this double trace flow mean anything in AdS/Nuclear or AdS/CMT? Running of everything we obtained before? Dispersion relation? Transport Coefficients? July 7, 2011 ICTS-USTC,Hefei 28 /

Holographic Wilsonian Renormalization Group

Holographic Wilsonian Renormalization Group Holographic Wilsonian Renormalization Group JiYoung Kim May 0, 207 Abstract Strongly coupled systems are difficult to study because the perturbation of the systems does not work with strong couplings.

More information

Inverse square potential, scale anomaly, and complex extension

Inverse square potential, scale anomaly, and complex extension Inverse square potential, scale anomaly, and complex extension Sergej Moroz Seattle, February 2010 Work in collaboration with Richard Schmidt ITP, Heidelberg Outline Introduction and motivation Functional

More information

Black hole thermodynamics under the microscope

Black hole thermodynamics under the microscope DELTA 2013 January 11, 2013 Outline Introduction Main Ideas 1 : Understanding black hole (BH) thermodynamics as arising from an averaging of degrees of freedom via the renormalisation group. Go beyond

More information

Holography on the Horizon and at Infinity

Holography on the Horizon and at Infinity Holography on the Horizon and at Infinity Suvankar Dutta H. R. I. Allahabad Indian String Meeting, PURI 2006 Reference: Phys.Rev.D74:044007,2006. (with Rajesh Gopakumar) Work in progress (with D. Astefanesei

More information

Holography and (Lorentzian) black holes

Holography and (Lorentzian) black holes Holography and (Lorentzian) black holes Simon Ross Centre for Particle Theory The State of the Universe, Cambridge, January 2012 Simon Ross (Durham) Holography and black holes Cambridge 7 January 2012

More information

TASI lectures: Holography for strongly coupled media

TASI lectures: Holography for strongly coupled media TASI lectures: Holography for strongly coupled media Dam T. Son Below is only the skeleton of the lectures, containing the most important formulas. I. INTRODUCTION One of the main themes of this school

More information

arxiv: v2 [hep-th] 17 Dec 2008

arxiv: v2 [hep-th] 17 Dec 2008 MIT-CTP 3983 Universality of the hydrodynamic limit in AdS/CFT and the membrane paradigm Nabil Iqbal and Hong Liu Center for Theoretical Physics, Massachusetts Institute of Technology, Cambridge, MA 039

More information

Holographic vortex pair annihilation in superfluid turbulence

Holographic vortex pair annihilation in superfluid turbulence Holographic vortex pair annihilation in superfluid turbulence Vrije Universiteit Brussel and International Solvay Institutes Based mainly on arxiv:1412.8417 with: Yiqiang Du and Yu Tian(UCAS,CAS) Chao

More information

Applications of AdS/CFT correspondence to cold atom physics

Applications of AdS/CFT correspondence to cold atom physics Applications of AdS/CFT correspondence to cold atom physics Sergej Moroz in collaboration with Carlos Fuertes ITP, Heidelberg Outline Basics of AdS/CFT correspondence Schrödinger group and correlation

More information

!onformali" Los# J.-W. Lee D. T. Son M. Stephanov D.B.K. arxiv: Phys.Rev.D80:125005,2009

!onformali Los# J.-W. Lee D. T. Son M. Stephanov D.B.K. arxiv: Phys.Rev.D80:125005,2009 !onformali" Los# J.-W. Lee D. T. Son M. Stephanov D.B.K arxiv:0905.4752 Phys.Rev.D80:125005,2009 Motivation: QCD at LARGE N c and N f Colors Flavors Motivation: QCD at LARGE N c and N f Colors Flavors

More information

Black hole entropy of gauge fields

Black hole entropy of gauge fields Black hole entropy of gauge fields William Donnelly (University of Waterloo) with Aron Wall (UC Santa Barbara) September 29 th, 2012 William Donnelly (UW) Black hole entropy of gauge fields September 29

More information

A sky without qualities

A sky without qualities A sky without qualities New boundaries for SL(2)xSL(2) Chern-Simons theory Bo Sundborg, work with Luis Apolo Stockholm university, Department of Physics and the Oskar Klein Centre August 27, 2015 B Sundborg

More information

BPS Black holes in AdS and a magnetically induced quantum critical point. A. Gnecchi

BPS Black holes in AdS and a magnetically induced quantum critical point. A. Gnecchi BPS Black holes in AdS and a magnetically induced quantum critical point A. Gnecchi June 20, 2017 ERICE ISSP Outline Motivations Supersymmetric Black Holes Thermodynamics and Phase Transition Conclusions

More information

QCD and a Holographic Model of Hadrons

QCD and a Holographic Model of Hadrons QCD and a Holographic Model of Hadrons M. Stephanov U. of Illinois at Chicago AdS/QCD p.1/18 Motivation and plan Large N c : planar diagrams dominate resonances are infinitely narrow Effective theory in

More information

Themodynamics at strong coupling from Holographic QCD

Themodynamics at strong coupling from Holographic QCD Themodynamics at strong coupling from Holographic QCD p. 1 Themodynamics at strong coupling from Holographic QCD Francesco Nitti APC, U. Paris VII Excited QCD Les Houches, February 23 2011 Work with E.

More information

On two dimensional black holes. and matrix models

On two dimensional black holes. and matrix models On two dimensional black holes and matrix models Based on: On Black Hole Thermodynamics of 2-D Type 0A, JHEP 0403 (04) 007, hep-th/0402152 with J. L. Davis and D. Vaman Madison April, 2004 Motivation:

More information

Beyond the unitarity bound in AdS/CFT

Beyond the unitarity bound in AdS/CFT Beyond the unitarity bound in AdS/CFT Tomás Andrade in collaboration with T. Faulkner, J. Jottar, R. Leigh, D. Marolf, C. Uhlemann October 5th, 2011 Introduction 1 AdS/CFT relates the dynamics of fields

More information

8.821 String Theory Fall 2008

8.821 String Theory Fall 2008 MIT OpenCourseWare http://ocw.mit.edu 8.821 String Theory Fall 2008 For information about citing these materials or our Terms of Use, visit: http://ocw.mit.edu/terms. 8.821 F2008 Lecture 03: The decoupling

More information

Symmetries, Horizons, and Black Hole Entropy. Steve Carlip U.C. Davis

Symmetries, Horizons, and Black Hole Entropy. Steve Carlip U.C. Davis Symmetries, Horizons, and Black Hole Entropy Steve Carlip U.C. Davis UC Davis June 2007 Black holes behave as thermodynamic objects T = κ 2πc S BH = A 4 G Quantum ( ) and gravitational (G) Does this thermodynamic

More information

Lectures on gauge-gravity duality

Lectures on gauge-gravity duality Lectures on gauge-gravity duality Annamaria Sinkovics Department of Applied Mathematics and Theoretical Physics Cambridge University Tihany, 25 August 2009 1. Review of AdS/CFT i. D-branes: open and closed

More information

Cosmological singularities, AdS/CFT and de Sitter deformations

Cosmological singularities, AdS/CFT and de Sitter deformations Cosmological singularities, AdS/CFT and de Sitter deformations K. Narayan Chennai Mathematical Institute (CMI), Chennai [ work in progress with Sumit Das; and arxiv:0807.1517, Adel Awad, Sumit Das, Suresh

More information

Holography for non-relativistic CFTs

Holography for non-relativistic CFTs Holography for non-relativistic CFTs Herzog, Rangamani & SFR, 0807.1099, Rangamani, Son, Thompson & SFR, 0811.2049, SFR & Saremi, 0907.1846 Simon Ross Centre for Particle Theory, Durham University Liverpool

More information

Insight into strong coupling

Insight into strong coupling Insight into strong coupling Many faces of holography: Top-down studies (string/m-theory based) focused on probing features of quantum gravity Bottom-up approaches pheno applications to QCD-like and condensed

More information

Black hole thermodynamics

Black hole thermodynamics Black hole thermodynamics Daniel Grumiller Institute for Theoretical Physics Vienna University of Technology Spring workshop/kosmologietag, Bielefeld, May 2014 with R. McNees and J. Salzer: 1402.5127 Main

More information

Holographic matter at finite chemical potential

Holographic matter at finite chemical potential Holographic matter at finite chemical potential Talk at NumHol 2016 Santiago de Compostela, Spain Aristomenis Donos Durham University Base on work with: J. P. Gauntlett, E. Banks, T. Griffin, L. Melgar,

More information

Renormalization of microscopic Hamiltonians. Renormalization Group without Field Theory

Renormalization of microscopic Hamiltonians. Renormalization Group without Field Theory Renormalization of microscopic Hamiltonians Renormalization Group without Field Theory Alberto Parola Università dell Insubria (Como - Italy) Renormalization Group Universality Only dimensionality and

More information

Fluid/Gravity Correspondence for general non-rotating black holes

Fluid/Gravity Correspondence for general non-rotating black holes Fluid/Gravity Correspondence for general non-rotating black holes Xiaoning Wu Institute of Mathematics, AMSS, CAS 2013. 7. 30, @Max Planck Institute for Physics, Munich Joint work with Y. Ling, Y. Tian,

More information

Boost-invariant dynamics near and far from equilibrium physics and AdS/CFT.

Boost-invariant dynamics near and far from equilibrium physics and AdS/CFT. Boost-invariant dynamics near and far from equilibrium physics and AdS/CFT. Micha l P. Heller michal.heller@uj.edu.pl Department of Theory of Complex Systems Institute of Physics, Jagiellonian University

More information

Holography with Shape Dynamics

Holography with Shape Dynamics . 1/ 11 Holography with Henrique Gomes Physics, University of California, Davis July 6, 2012 In collaboration with Tim Koslowski Outline 1 Holographic dulaities 2 . 2/ 11 Holographic dulaities Ideas behind

More information

Holographic entropy production

Holographic entropy production 1 1 School of Physics, University of Chinese Academy of Sciences ( 中国科学院大学物理学院 ) (Based on the joint work [arxiv:1204.2029] with Xiaoning Wu and Hongbao Zhang, which received an honorable mention in the

More information

AdS/CFT and condensed matter physics

AdS/CFT and condensed matter physics AdS/CFT and condensed matter physics Simon Ross Centre for Particle Theory, Durham University Padova 28 October 2009 Simon Ross (Durham) AdS/CMT 28 October 2009 1 / 23 Outline Review AdS/CFT Application

More information

Critical Region of the QCD Phase Transition

Critical Region of the QCD Phase Transition Critical Region of the QCD Phase Transition Mean field vs. Renormalization group B.-J. Schaefer 1 and J. Wambach 1,2 1 Institut für Kernphysik TU Darmstadt 2 GSI Darmstadt 18th August 25 Uni. Graz B.-J.

More information

Dynamics, phase transitions and holography

Dynamics, phase transitions and holography Dynamics, phase transitions and holography Jakub Jankowski with R. A. Janik, H. Soltanpanahi Phys. Rev. Lett. 119, no. 26, 261601 (2017) Faculty of Physics, University of Warsaw Phase structure at strong

More information

ACOUSTIC BLACK HOLES. MASSIMILIANO RINALDI Université de Genève

ACOUSTIC BLACK HOLES. MASSIMILIANO RINALDI Université de Genève ACOUSTIC BLACK HOLES MASSIMILIANO RINALDI Université de Genève OUTLINE Prelude: GR vs QM Hawking Radiation: a primer Acoustic Black Holes Hawking Radiation in Acoustic Black Holes Acoustic Black Holes

More information

How to build a holographic liquid crystal? Piotr Surówka Vrije Universiteit Brussel

How to build a holographic liquid crystal? Piotr Surówka Vrije Universiteit Brussel How to build a holographic liquid crystal? Piotr Surówka Vrije Universiteit Brussel Euler Symposium On Theoretical And Mathematical Physics, St. Petersburg 17.07.2013 Motivation Hydrodynamics is an effective

More information

Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis

Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis Black Hole Entropy: An ADM Approach Steve Carlip U.C. Davis ADM-50 College Station, Texas November 2009 Black holes behave as thermodynamic objects T = κ 2πc S BH = A 4 G Quantum ( ) and gravitational

More information

Spacetime emergence via holographic RG flow from incompressible Navier-Stokes at the horizon. based on

Spacetime emergence via holographic RG flow from incompressible Navier-Stokes at the horizon. based on Prifysgol Abertawe? Strong Fields, Strings and Holography Spacetime emergence via holographic RG flow from incompressible Navier-Stokes at the horizon based on arxiv:1105.4530 ; arxiv:arxiv:1307.1367 with

More information

Holographic Entanglement Entropy for Surface Operators and Defects

Holographic Entanglement Entropy for Surface Operators and Defects Holographic Entanglement Entropy for Surface Operators and Defects Michael Gutperle UCLA) UCSB, January 14th 016 Based on arxiv:1407.569, 1506.0005, 151.04953 with Simon Gentle and Chrysostomos Marasinou

More information

Status of Hořava Gravity

Status of Hořava Gravity Status of Institut d Astrophysique de Paris based on DV & T. P. Sotiriou, PRD 85, 064003 (2012) [arxiv:1112.3385 [hep-th]] DV & T. P. Sotiriou, JPCS 453, 012022 (2013) [arxiv:1212.4402 [hep-th]] DV, arxiv:1502.06607

More information

The Quantum Theory of Finite-Temperature Fields: An Introduction. Florian Divotgey. Johann Wolfgang Goethe Universität Frankfurt am Main

The Quantum Theory of Finite-Temperature Fields: An Introduction. Florian Divotgey. Johann Wolfgang Goethe Universität Frankfurt am Main he Quantum heory of Finite-emperature Fields: An Introduction Florian Divotgey Johann Wolfgang Goethe Universität Franfurt am Main Fachbereich Physi Institut für heoretische Physi 1..16 Outline 1 he Free

More information

Hydrodynamic Modes of Incoherent Black Holes

Hydrodynamic Modes of Incoherent Black Holes Hydrodynamic Modes of Incoherent Black Holes Vaios Ziogas Durham University Based on work in collaboration with A. Donos, J. Gauntlett [arxiv: 1707.xxxxx, 170x.xxxxx] 9th Crete Regional Meeting on String

More information

Zero Temperature Dissipation & Holography

Zero Temperature Dissipation & Holography Zero Temperature Dissipation & Holography Pinaki Banerjee National Strings Meeting - 2015 PB & B. Sathiapalan (on going) Outline 1 Introduction 2 Langevin Dynamics From Holography 3 Dissipation 4 Conclusions

More information

Virasoro hair on locally AdS 3 geometries

Virasoro hair on locally AdS 3 geometries Virasoro hair on locally AdS 3 geometries Kavli Institute for Theoretical Physics China Institute of Theoretical Physics ICTS (USTC) arxiv: 1603.05272, M. M. Sheikh-Jabbari and H. Y Motivation Introduction

More information

V Finite T, probe branes, quarks, other extensions

V Finite T, probe branes, quarks, other extensions Introduction to the AdS/CFT correspondence Outline I CFT review II AdS/CFT correspondence III Large N review IV D3 branes and AdS 5 S 5 V Finite T, probe branes, quarks, other extensions 1 0 References

More information

GENERAL RELATIVITY: THE FIELD THEORY APPROACH

GENERAL RELATIVITY: THE FIELD THEORY APPROACH CHAPTER 9 GENERAL RELATIVITY: THE FIELD THEORY APPROACH We move now to the modern approach to General Relativity: field theory. The chief advantage of this formulation is that it is simple and easy; the

More information

Strings and Black Holes

Strings and Black Holes Strings and Black Holes Erik Verlinde Institute for Theoretical Physics University of Amsterdam General Relativity R Rg GT µν µν = 8π µν Gravity = geometry Einstein: geometry => physics Strings: physics

More information

Non-relativistic AdS/CFT

Non-relativistic AdS/CFT Non-relativistic AdS/CFT Christopher Herzog Princeton October 2008 References D. T. Son, Toward an AdS/cold atoms correspondence: a geometric realization of the Schroedinger symmetry, Phys. Rev. D 78,

More information

Bulk versus boundary quantum states

Bulk versus boundary quantum states Bulk versus boundary quantum states Henrique Boschi-Filho and Nelson R. F. Braga Instituto de Física, Universidade Federal do Rio de Janeiro Caixa Postal 68528, 21945-970 Rio de Janeiro, RJ, Brazil Abstract

More information

Quantum Fields in Curved Spacetime

Quantum Fields in Curved Spacetime Quantum Fields in Curved Spacetime Lecture 3 Finn Larsen Michigan Center for Theoretical Physics Yerevan, August 22, 2016. Recap AdS 3 is an instructive application of quantum fields in curved space. The

More information

Cosmological constant is a conserved charge

Cosmological constant is a conserved charge Cosmological constant is a conserved Kamal Hajian Institute for Research in Fundamental Sciences (IPM) In collaboration with Dmitry Chernyavsky (Tomsk Polytechnic U.) arxiv:1710.07904, to appear in Classical

More information

HIGHER SPIN CORRECTIONS TO ENTANGLEMENT ENTROPY

HIGHER SPIN CORRECTIONS TO ENTANGLEMENT ENTROPY HIGHER SPIN CORRECTIONS TO ENTANGLEMENT ENTROPY JHEP 1406 (2014) 096, Phys.Rev. D90 (2014) 4, 041903 with Shouvik Datta ( IISc), Michael Ferlaino, S. Prem Kumar (Swansea U. ) JHEP 1504 (2015) 041 with

More information

Towards new relativistic hydrodynamcis from AdS/CFT

Towards new relativistic hydrodynamcis from AdS/CFT Towards new relativistic hydrodynamcis from AdS/CFT Michael Lublinsky Stony Brook with Edward Shuryak QGP is Deconfined QGP is strongly coupled (sqgp) behaves almost like a perfect liquid (Navier-Stokes

More information

Black Holes: Energetics and Thermodynamics

Black Holes: Energetics and Thermodynamics Black Holes: Energetics and Thermodynamics Thibault Damour Institut des Hautes Études Scientifiques ICRANet, Nice, 4-9 June 2012 Thibault Damour (IHES) Black Holes: Energetics and Thermodynamics 7/06/2012

More information

STOCHASTIC QUANTIZATION AND HOLOGRAPHY

STOCHASTIC QUANTIZATION AND HOLOGRAPHY STOCHASTIC QUANTIZATION AND HOLOGRAPHY WORK WITH D.MANSI & A. MAURI: TO APPEAR TASSOS PETKOU UNIVERSITY OF CRETE OUTLINE CONFORMAL HOLOGRAPHY STOCHASTIC QUANTIZATION STOCHASTIC QUANTIZATION VS HOLOGRAPHY

More information

Emergent Quantum Criticality

Emergent Quantum Criticality (Non-)Fermi Liquids and Emergent Quantum Criticality from gravity Hong Liu Massachusetts setts Institute te of Technology HL, John McGreevy, David Vegh, 0903.2477 Tom Faulkner, HL, JM, DV, to appear Sung-Sik

More information

Introduction to AdS/CFT

Introduction to AdS/CFT Introduction to AdS/CFT Who? From? Where? When? Nina Miekley University of Würzburg Young Scientists Workshop 2017 July 17, 2017 (Figure by Stan Brodsky) Intuitive motivation What is meant by holography?

More information

Talk based on: arxiv: arxiv: arxiv: arxiv: arxiv:1106.xxxx. In collaboration with:

Talk based on: arxiv: arxiv: arxiv: arxiv: arxiv:1106.xxxx. In collaboration with: Talk based on: arxiv:0812.3572 arxiv:0903.3244 arxiv:0910.5159 arxiv:1007.2963 arxiv:1106.xxxx In collaboration with: A. Buchel (Perimeter Institute) J. Liu, K. Hanaki, P. Szepietowski (Michigan) The behavior

More information

Smooth Wilson Loops and Yangian Symmetry in Planar N = 4 SYM

Smooth Wilson Loops and Yangian Symmetry in Planar N = 4 SYM Smooth Wilson Loops and Yangian Symmetry in Planar N = 4 SYM ITP, Niklas Beisert Workshop on Hidden symmetries and integrability methods in super Yang Mills theories and their dual string theories Centre

More information

Building a holographic liquid crystal

Building a holographic liquid crystal Building a holographic liquid crystal Piotr Surówka Vrije Universiteit Brussel Ongoing work with R. Rahman and G. Compère Gauge/Gravity Duality, Munich, 01.08.2013 Motivation Hydrodynamics is an effective

More information

Scale and Conformal Invariance in d = 4

Scale and Conformal Invariance in d = 4 Scale and Conformal Invariance in d = 4 Joseph Polchinski work with Markus Luty & Riccardo Rattazzi arxiv:1204xxxx N = 4 Super Yang-Mills Theory, 35 Years After Caltech, March 31, 2102 Overview: Scale

More information

Holographic construction of CFT excited states. Kostas Skenderis

Holographic construction of CFT excited states. Kostas Skenderis Holographic construction of CFT excited states STAG CH RESEARCH ER C TE CENTER Aspects of Conformal Field Theories Thessaloniki, Greece 24 September 2015 Introduction According to holography, gravity in

More information

Yangian Symmetry of Planar N = 4 SYM

Yangian Symmetry of Planar N = 4 SYM Yangian Symmetry of Planar N = 4 SYM ITP, Niklas Beisert New formulations for scattering amplitudes Ludwig Maximilians Universität, München 9 September 2016 work with J. Plefka, D. Müller, C. Vergu (1509.05403);

More information

Non-Perturbative Thermal QCD from AdS/QCD

Non-Perturbative Thermal QCD from AdS/QCD Issues Non-Perturbative Thermal QCD from AdS/QCD * Collaborators: B. Galow, M. Ilgenfritz, J. Nian, H.J. Pirner, K. Veshgini Research Fellow of the Alexander von Humboldt Foundation Institute for Theoretical

More information

Holographic phase space and black holes as renormalization group flows

Holographic phase space and black holes as renormalization group flows and black holes as renormalization group flows Laboratoire de Physique Théorique et Hautes Energies, Université Pierre et Marie Curie Based on arxiv: 1101.5993 DAMTP, University of Cambridge, 12/05/2011

More information

Lecture 8: 1-loop closed string vacuum amplitude

Lecture 8: 1-loop closed string vacuum amplitude Lecture 8: 1-loop closed string vacuum amplitude José D. Edelstein University of Santiago de Compostela STRING THEORY Santiago de Compostela, March 5, 2013 José D. Edelstein (USC) Lecture 8: 1-loop vacuum

More information

Holographic Entanglement and Interaction

Holographic Entanglement and Interaction Holographic Entanglement and Interaction Shigenori Seki RINS, Hanyang University and Institut des Hautes Études Scientifiques Intrication holographique et interaction à l IHES le 30 janvier 2014 1 Contents

More information

Trapped ghost wormholes and regular black holes. The stability problem

Trapped ghost wormholes and regular black holes. The stability problem Trapped ghost wormholes and regular black holes. The stability problem Kirill Bronnikov in collab. with Sergei Bolokhov, Arislan Makhmudov, Milena Skvortsova (VNIIMS, Moscow; RUDN University, Moscow; MEPhI,

More information

Universal features of Lifshitz Green's functions from holography

Universal features of Lifshitz Green's functions from holography Universal features of Lifshitz Green's functions from holography Gino Knodel University of Michigan October 19, 2015 C. Keeler, G.K., J.T. Liu, and K. Sun; arxiv:1505.07830. C. Keeler, G.K., and J.T. Liu;

More information

Large N fermionic tensor models in d = 2

Large N fermionic tensor models in d = 2 Large N fermionic tensor models in d = 2 Sylvain Carrozza Quantum spacetime and the Renormalization roup 2018 Bad Honnef Sylvain Carrozza Large N fermionic tensor models Bad Honnef 20/6/2018 1 / 17 Context

More information

Entanglement entropy and the F theorem

Entanglement entropy and the F theorem Entanglement entropy and the F theorem Mathematical Sciences and research centre, Southampton June 9, 2016 H RESEARH ENT Introduction This talk will be about: 1. Entanglement entropy 2. The F theorem for

More information

Absorption cross section of RN black hole

Absorption cross section of RN black hole 3 Absorption cross section of RN black hole 3.1 Introduction Even though the Kerr solution is the most relevant one from an astrophysical point of view, the solution of the coupled Einstein-Maxwell equation

More information

Geometry and Physics. Amer Iqbal. March 4, 2010

Geometry and Physics. Amer Iqbal. March 4, 2010 March 4, 2010 Many uses of Mathematics in Physics The language of the physical world is mathematics. Quantitative understanding of the world around us requires the precise language of mathematics. Symmetries

More information

PAPER 311 BLACK HOLES

PAPER 311 BLACK HOLES MATHEMATICAL TRIPOS Part III Friday, 8 June, 018 9:00 am to 1:00 pm PAPER 311 BLACK HOLES Attempt no more than THREE questions. There are FOUR questions in total. The questions carry equal weight. STATIONERY

More information

Insight into strong coupling

Insight into strong coupling Thank you 2012 Insight into strong coupling Many faces of holography: Top-down studies (string/m-theory based) Bottom-up approaches pheno applications to QCD-like and condensed matter systems (e.g. Umut

More information

Übungen zur Elektrodynamik (T3)

Übungen zur Elektrodynamik (T3) Arnold Sommerfeld Center Ludwig Maximilians Universität München Prof. Dr. Ivo Sachs SoSe 08 Übungen zur Elektrodynamik (T3) Lösungen zum Übungsblatt 7 Lorentz Force Calculate dx µ and ds explicitly in

More information

arxiv:hep-th/ v3 24 Apr 2007

arxiv:hep-th/ v3 24 Apr 2007 Anti-de Sitter boundary in Poincaré coordinates C. A. Ballón Bayona and Nelson R. F. Braga Instituto de Física, Universidade Federal do Rio de Janeiro, Caixa Postal 68528, RJ 21941-972 Brazil Abstract

More information

AdS/CFT Correspondence and Entanglement Entropy

AdS/CFT Correspondence and Entanglement Entropy AdS/CFT Correspondence and Entanglement Entropy Tadashi Takayanagi (Kyoto U.) Based on hep-th/0603001 [Phys.Rev.Lett.96(2006)181602] hep-th/0605073 [JHEP 0608(2006)045] with Shinsei Ryu (KITP) hep-th/0608213

More information

Emergent gravity. Diana Vaman. Physics Dept, U. Virginia. September 24, U Virginia, Charlottesville, VA

Emergent gravity. Diana Vaman. Physics Dept, U. Virginia. September 24, U Virginia, Charlottesville, VA Emergent gravity Diana Vaman Physics Dept, U. Virginia September 24, U Virginia, Charlottesville, VA What is gravity? Newton, 1686: Universal gravitational attraction law F = G M 1 M 2 R 2 12 Einstein,

More information

Emergent Causality in Holography

Emergent Causality in Holography Emergent Causality in Holography Netta Engelhardt Princeton University 20.6.18 Based mostly on: NE, Horowitz 16; NE 16; NE, Fischetti 17 Spacetime Emergence Holography: the equivalence of a higher-dim

More information

Time Evolution of Holographic Complexity

Time Evolution of Holographic Complexity Time Evolution of Holographic Complexity Sotaro Sugishita (Osaka Univ.) based on arxiv:1709.10184 [JHEP 1711, 188 (2017)] with Dean Carmi, Shira Chapman, Hugo Marrochio, Robert Myers RIKEN-Osaka-OIST Joint

More information

Glueballs at finite temperature from AdS/QCD

Glueballs at finite temperature from AdS/QCD Light-Cone 2009: Relativistic Hadronic and Particle Physics Instituto de Física Universidade Federal do Rio de Janeiro Glueballs at finite temperature from AdS/QCD Alex S. Miranda Work done in collaboration

More information

Black Hole Entropy and Gauge/Gravity Duality

Black Hole Entropy and Gauge/Gravity Duality Tatsuma Nishioka (Kyoto,IPMU) based on PRD 77:064005,2008 with T. Azeyanagi and T. Takayanagi JHEP 0904:019,2009 with T. Hartman, K. Murata and A. Strominger JHEP 0905:077,2009 with G. Compere and K. Murata

More information

κ = f (r 0 ) k µ µ k ν = κk ν (5)

κ = f (r 0 ) k µ µ k ν = κk ν (5) 1. Horizon regularity and surface gravity Consider a static, spherically symmetric metric of the form where f(r) vanishes at r = r 0 linearly, and g(r 0 ) 0. Show that near r = r 0 the metric is approximately

More information

Non-Equilibrium Steady States Beyond Integrability

Non-Equilibrium Steady States Beyond Integrability Non-Equilibrium Steady States Beyond Integrability Joe Bhaseen TSCM Group King s College London Beyond Integrability: The Mathematics and Physics of Integrability and its Breaking in Low-Dimensional Strongly

More information

Lecture 20: Effective field theory for the Bose- Hubbard model

Lecture 20: Effective field theory for the Bose- Hubbard model Lecture 20: Effective field theory for the Bose- Hubbard model In the previous lecture, we have sketched the expected phase diagram of the Bose-Hubbard model, and introduced a mean-field treatment that

More information

Analytic continuation of functional renormalization group equations

Analytic continuation of functional renormalization group equations Analytic continuation of functional renormalization group equations Stefan Flörchinger (CERN) Aachen, 07.03.2012 Short outline Quantum effective action and its analytic continuation Functional renormalization

More information

Cosmological solutions of Double field theory

Cosmological solutions of Double field theory Cosmological solutions of Double field theory Haitang Yang Center for Theoretical Physics Sichuan University USTC, Oct. 2013 1 / 28 Outlines 1 Quick review of double field theory 2 Duality Symmetries in

More information

Towards a holographic formulation of cosmology

Towards a holographic formulation of cosmology Towards a holographic formulation of cosmology Gonzalo Torroba Stanford University Topics in holography, supersymmetry and higher derivatives Mitchell Institute, Texas A&M, April 2013 During the last century,

More information

21 July 2011, USTC-ICTS. Chiang-Mei Chen 陳江梅 Department of Physics, National Central University

21 July 2011, USTC-ICTS. Chiang-Mei Chen 陳江梅 Department of Physics, National Central University 21 July 2011, Seminar @ USTC-ICTS Chiang-Mei Chen 陳江梅 Department of Physics, National Central University Outline Black Hole Holographic Principle Kerr/CFT Correspondence Reissner-Nordstrom /CFT Correspondence

More information

Nonlocal Effects in Quantum Gravity

Nonlocal Effects in Quantum Gravity Nonlocal Effects in Quantum Gravity Suvrat Raju International Centre for Theoretical Sciences 29th Meeting of the IAGRG IIT Guwahati 20 May 2017 Collaborators Based on work with 1 Kyriakos Papadodimas

More information

The Trailing String in Confining Holographic Theories

The Trailing String in Confining Holographic Theories The Trailing String in Confining Holographic Theories p. 1 The Trailing String in Confining Holographic Theories Francesco Nitti APC, U. Paris VII Twelfth Workshop on Non-Perturbative Quantum Chromodynamics

More information

Aspects of Renormalized Entanglement Entropy

Aspects of Renormalized Entanglement Entropy Aspects of Renormalized Entanglement Entropy Tatsuma Nishioka (U. Tokyo) based on 1207.3360 with Klebanov, Pufu and Safdi 1401.6764 1508.00979 with Banerjee and Nakaguchi T. Nishioka (Tokyo) Oct 15, 2015

More information

Seminar presented at the Workshop on Strongly Coupled QCD: The Confinement Problem Rio de Janeiro UERJ November 2011

Seminar presented at the Workshop on Strongly Coupled QCD: The Confinement Problem Rio de Janeiro UERJ November 2011 and and Seminar presented at the Workshop on Strongly Coupled QCD: The Problem Rio de Janeiro UERJ 28-30 November 2011 Work done in collaboration with: N.R.F. Braga, H. L. Carrion, C. N. Ferreira, C. A.

More information

Lecture 9: RR-sector and D-branes

Lecture 9: RR-sector and D-branes Lecture 9: RR-sector and D-branes José D. Edelstein University of Santiago de Compostela STRING THEORY Santiago de Compostela, March 6, 2013 José D. Edelstein (USC) Lecture 9: RR-sector and D-branes 6-mar-2013

More information

Holographic transport with random-field disorder. Andrew Lucas

Holographic transport with random-field disorder. Andrew Lucas Holographic transport with random-field disorder Andrew Lucas Harvard Physics Quantum Field Theory, String Theory and Condensed Matter Physics: Orthodox Academy of Crete September 1, 2014 Collaborators

More information

Black Holes in Nuclear and Particle Physics

Black Holes in Nuclear and Particle Physics Black Holes in Nuclear and Particle Physics Daniel Grumiller Center for Theoretical Physics Massachusetts Institute of Technology and Institute for Theoretical Physics Vienna University of Technology Annual

More information

A Brief Introduction to AdS/CFT Correspondence

A Brief Introduction to AdS/CFT Correspondence Department of Physics Universidad de los Andes Bogota, Colombia 2011 Outline of the Talk Outline of the Talk Introduction Outline of the Talk Introduction Motivation Outline of the Talk Introduction Motivation

More information

Scale without conformal invariance

Scale without conformal invariance Scale without conformal invariance Andy Stergiou Department of Physics, UCSD based on arxiv:1106.2540, 1107.3840, 1110.1634, 1202.4757 with Jean-François Fortin and Benjamín Grinstein Outline The physics:

More information

An Introduction to AdS/CFT Correspondence

An Introduction to AdS/CFT Correspondence An Introduction to AdS/CFT Correspondence Dam Thanh Son Institute for Nuclear Theory, University of Washington An Introduction to AdS/CFT Correspondence p.1/32 Plan of of this talk AdS/CFT correspondence

More information

Superconductivity, Superfluidity and holography

Superconductivity, Superfluidity and holography Outline Department of Theoretical Physics and Institute of Theoretical Physics, Autònoma University of Madrid, Spain and Scuola Normale Superiore di Pisa, Italy 12 November 2012, Laboratori Nazionali del

More information