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Spiky strings, light-like Wilson loops and a pp-wave anomaly M. Kruczenski Purdue University Based on: arXiv:0802.2039 A. Tseytlin, M.K. work in progress R. Ishizeki, A. Tirziu, M.K

Spiky strings, light-like Wilson loops and a pp-wave anomaly

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Spiky strings, light-like Wilson loops and a pp-wave anomaly. M. Kruczenski. Purdue University. Based on: arXiv:0802.2039 A. Tseytlin, M.K. work in progress R. Ishizeki, A. Tirziu, M.K. Summary. ● Introduction Twist two operators in gauge theories ( QCD ) - PowerPoint PPT Presentation

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Page 1: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Spiky strings, light-like Wilson loops and a pp-wave anomaly

M. Kruczenski

Purdue University

Based on: arXiv:0802.2039A. Tseytlin, M.K.work in progressR. Ishizeki, A. Tirziu, M.K.

Page 2: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Summary● Introduction

Twist two operators in gauge theories (QCD) String / gauge theory duality (AdS/CFT)

AdS/CFT and twist two operators ● Rotating strings ● Cusp anomaly

Higher twist operators: spiky stringsOther applications / results.

● Large spin limit of the spiky string Limiting shape and near boundary string

● Limit in the boundaryGauge theory in a pp-wave

Page 3: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

● PP-wave anomalyGauge theory in a pp-wave pp-wave anomaly

cusp anomaly/ anomalous dim. of twist two ops. ● Strong coupling String calculation: Wilson loop in pp-wave w/ AdS/CFT ● Small coupling Field theory calculation: Wilson loop in pp-wave (Class. source).

● Wilson loops in PP-wave

● Conformal mapping: Wilson loops in flat space

● Other Wilson loops: New ansatz for Wilson loops

● Conclusions

Page 4: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Twist two operators in gauge theories (QCD)

q2 ∞, =-2 p.q / q2 fixed

X

e

e

q

H, por q+ ∞, q-

fixedNear l.c. expansion

OPE: (z20, light-like, twist), (z20, euclidean, conf. dim.)

This (after including indices correctly) is plugged into:

Page 5: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

String/gauge theory duality: Large N limit (‘t Hooft)

QCD [ SU(3) ] Large N-limit [SU(N)]

Effective strings

Strong coupling

Lowest order: sum of planar diagrams (infinite number)

N g N fixedYM , 2More precisely: (‘t Hooft coupl.)

qq

Page 6: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

AdS/CFT correspondence (Maldacena)

Gives a precise example of the relation betweenstrings and gauge theory.

Gauge theory

N = 4 SYM SU(N) on R4

Aμ , Φi, Ψa

Operators w/ conf. dim.

String theory

IIB on AdS5xS5

radius RString states w/ E

R

g g R l g Ns YM s YM 2 2 1 4; / ( ) /

N g NYM , 2fixed

λ large → string th.λ small → field th.

Page 7: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Twist two operators from rotation in AdS5 (Gubser, Klebanov, Polyakov)Y Y Y Y Y Y R1

222

32

42

52

62 2

s in h ; [ ]2

3 cosh ;2 t

ds d t d d2 2 2 2 23

2 cosh sin h [ ]

E S S S

O Tr x z tS

ln , ( )

, θ = ω t

Page 8: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Twist two ops. from cusp anomaly (MK, Makeenko)

The anomalous dimensions of twist two operators can also be computed by using the cusp anomaly of light-like Wilson loops (Korchemsky and Marchesini).

In AdS/CFT Wilson loops can be computed using surfaces of minimal area in AdS5 (Maldacena, Rey, Yee)

z

The result agrees with the rotating string calculation.

Page 9: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Generalization to higher twist operators (MK)

O TrnS n S n S n S n

[ ]/ / / / O Tr S

[ ]2

x A n A n

y A n A n

co s[( ) ] ( ) co s [ ]

sin [( ) ] ( ) sin [ ]

1 1

1 1

In flat space such solutions are easily found in conf. gauge:

Page 10: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Spiky strings in AdS:

Ansatz:

Eq. of motion:

Action and momenta:

Page 11: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

E Sn

S S

O Tr S n S n S n S n

2

ln , ( )

/ / / /

S d t d tjj

j j

j

22 1

84

21 12 1

(cosh ) ln s in

Page 12: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Other applications / results for f()

● Gluon scattering amplitudes (Bern, Dixon, Smirnov …)

● Scattering amplitudes in AdS/CFT (Alday, Maldacena,…)

● Anomalous dimension f() at all loops (Beisert, Eden, Staudacher ,…)

For all couplings we are lead to define f() through:

E = S + (n/2) f() ln S (large S)

Page 13: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Large spin limit of the spiky string

The limit of large spin (E-S ~ ln S) corresponds to 1. In that limit the spikes touch the boundary andthe solution simplifies.

In embedding coordinates

The same f() should appear in all of them!

Page 14: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Near boundary limit

We can take 0∞ and get a solution close to the bdy.

AdS5

Near bdyregion

Define light-like coords.

Near bdy.rescaling.Zooms in the shaded region

Half spike

Page 15: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

In the limit 0 we get the metric:

So, the tiny string sees an AdS pp-wave in Poincarecoordinates. When z0, the boundary metric becomesa pp-wave in usual flat space:

N = 4 SYM SU(N) on R4 pp-wave dual to

IIB on AdS5 pp-wave x S5

This duality should contain all the information about f()

AdS!

According

to AdS/CFT

Page 16: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Limit in the boundary

S3

t

In the boundary (RxS3) the particle is moving along a light-like geodesics so it seesthe Penrose limit of the metric.

Therefore it suffices to study the gauge theory in a pp-wave:

Page 17: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

We just argued that to compute f() we need to study

N = 4 in a pp-wave or strings in an AdS pp-wave.

What should we compute? Before it was E-S = f() ln S for the folded string.

Following the change of coordinates we find that

Since E~S we can say that for a single charge moving along x+ we should have

with

Page 18: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

This leads us to define a PP wave anomaly

According to the previous calculations we need to compute P± in the presence of a charge (WL):

Equivalently: UVcut-off

PP-wave anomaly

Page 19: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

PP wave anomaly Strong coupling

We put a particle in a pp-wave backgroundand compute P± which amounts to computing a Wilson loop. We can use AdS/CFT since we knowThat the dual of the pp-wave is the AdS pp-wave.

The Wilson loop is x+=and the string solution is simply:

Giving:

or

OK

Page 20: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

PP wave anomaly Small coupling

Again we need to compute a Wilson loop in the pp-wave background. At lowest order it is a classicalsource in the linearized approximation. We need to solve Maxwell eqns. in the pp-wave witha source moving according to x+=

r2=x12+x2

2

Page 21: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

We can now compute the energy momentum tensor

Obtaining

Using

we get

Page 22: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Or

Giving OK

The symmetry if the pp-wave under

implies that P+ ~ ln P- and therefore that the anomalousdimension grows logarithmically with the spin.

Page 23: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Other Wilson loops in the pp-wave

ds2 = 2 dx+ dx- - 2 x2 dx+

2 + dx2 ,

● Light-like line: x=0, x- =0, x+=

x

t

xx t

2

Page 24: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

● Time-like line: x= x=0, t=

● Parallel lines in x+ direction: x=0 , x- =±a, x+=

x

t

x

t

Page 25: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

● Parallel lines in x+ direction: x2=a,b , x- =0, x+=

● Parallel line in time-like direction: x=±a, t=

t

x

x2

x

t

Page 26: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Conformal mapping

The metric:

ds2 = 2 dx+ dx- - 2 x2 dx+

2 + dx2 ,

is conformally flat! But this is a local equivalence.Equivalently the AdS pp-wave is (locally) AdS space in different coordinates. (Brecher, Chamblin, Reall)

We can map the Wilson loop solutions to Wilson loops in ordinary space.

xx t

2

Page 27: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Indeed, the mapping:

gives:

and

gives:

Page 28: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

This allows us to obtain new Wilson loop solutions in usual AdS in Poincare coordinates.

● Light-like line: x=0, x- =0, x+=

x

t

Page 29: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

● Time-like line: x= x=0, t=

The Wilson loop now changes shape. Particle decelerating and then accelerating.

x

t

Page 30: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

We can do the same with the other solutions.Generically we obtain surfaces in which z is a functionof two variables and therefore very difficult to finddirectly.

Physically these solution seem to represent Wilson loops in the presence of propagating gluons given byspikes coming out from the horizon.

Also, in general the energy is not conserved so itrequires certain power to move the quarks in these particular way.

Page 31: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Other Wilson loop solutions (new ansatz)

We use the ansatz

The equations of motion linearize. We get:

The boundary curve (WL) is:

Page 32: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

These solutions are BPS and therefore the areavanishes.

By a conformal transformation we can map them to WL given by closed curves.

Again, is arbitrary. Namely we can find the solution for any such function.

The area is

Page 33: Spiky strings, light-like Wilson loops  and a pp-wave anomaly

Conclusions: ● We define a pp-wave anomaly for a gauge theory living in a pp-wave as a (logarithmic) divergence of the energy momentum tensor in the presence of a particlemoving at the speed of light.

● We proposed that it is given by the cusp anomaly andverify it at lowest order in the strong (string) and weak(field theory) coupling expansion.

● Following these ideas new open string solutions can be found both, in the AdS pp-wave and, by conformal mapping in ordinary AdS

● We found other solutions using a new ansatz.