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ESI Higher spin Holography 2019 Chaos in 3D HS Gravity Jung gi Yoon Korea Institute for Advanced Study ( K IHS )

ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

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Page 1: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

ESI Higher spin Holography 2019

Chaos

in 3D HS Gravity

Junggi Yoon

Korea Institute for Advanced Study( K IHS )

Page 2: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

Chaos in 3D Higher spin Gravity

Based on 1903 .

08761 Prithvi Narayan , TY

( 1903 . 09086 Viktor Jahnke,Keun - Young Kim ,JY)

↳ rotating BTZ Black hole .

I.

Introduction.

* Butterfly effect.

* .

" "

• Classical.

fuel% ,

next .

• Quantum ( [ VCA ,Wco )? My

,n e

*

• out - of - time - ordered correlate.

⇒ ( Vce ) Wco ) Vce ) WCO ) ) n l - E e't

'

B

* Bound on chaos.

:

XL € 2¥Malda cena ,Shenker , Stanford .

Page 3: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

* Black hole :

maximally chaotic .

thyEoe .si#asai:er.ing

of

exchangeofgraviton .

⇒ t.

: saturate !r e

spin - s field exchange?

)f ⇒ e⇒cs - he

D= ⇒ Cst ) ;violate chaos bound

for s > 2.

HS gravity .

i ) HS symmetry is broken.

Ti ) HSsymmetry is not broken

. .infinite cower of Its field

.

@ Too > - It e¥tte tt - - .

= ÷¥ - A- O. .

.

iii ) Finite cower of Hs field.

3D SLU ) CSgravity .

5=2.3 .- - -

- N.

: semi - classical limit of ↳ EAI HS gravity .

( x → - N ) ⇒ truncation

non -

unitary . Causality in Ape function ??

E.Perlmutter : W vacuum block

.

Page 4: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

Motivation :

How to calculate spin - s field contributionto Ape function in SLCN.ci ) CS

)spi§gravity ?

Cf ) JT gravity / Schwarzman theory / STK model.

S = Jdt . Sch team -4¥ ) , Ef f : boundary graviton( pseudo Goldstone boson

=fde Sch # es , Eft 2¥ If-

SSBIESB of

reparameeri Eat ion

Coddjoint orbit action.

DiffLcs ) .

o O

Schutt . -4.

-

- fEff÷5

o

D Quadratic level : foes = t t Eee )

& mode expansion : = et E En e-"t

-

S" '

= n-

Cn-

- I ) E- n En

.

'

. vanishes at n -- O , I I

③ Gct , its ) -- LOGGED > ~

so

[email protected]_Gcei.t .it Efface . .es

-feet -- Et Eine htt

.. .

Page 5: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

-

i③ / LEN E- n > Senga 't " Se. .Gets . eat

,

-

Questions.

I.

What is W - generalizationof Schwarz ian action ?

Ooguri . Bershadsky ( 1.989) & Wei Li . Theisen 420157

Grum i ler etc . ( 2018 )

D How to get the on - shell action ?

( in CS gravity )

- Boundary term , Boundary condition.

② finite temperature Schwarz ion ?

( smoothgauge

transfers Large gauge transf )

Sch [ feel . - it ⇒ Solitaire " . tff : R → R fee ) :S

'

→ s'

Page 6: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

TI.

( boundary - to - boundary ) two point function.

① What kind of ewo point function .

pure CS : no matter

topological : difficult to

couple to matter .

② Ws - transformation of two - point function

③ Why do we calculate

< En E - n > SEUG FENG ?

Page 7: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

I.

W - generalized Schwarz ian :

* Quick derivation :

A = bib ( d tacet ) bar) : CS connection

r Lob = e

..

⇒ Az = g¥BzfG ) & Gauss Decomposition g- LDU

=L:{ EtD SLCN.cl ) CS gravity

A. Tt

.

Los = fTr( ADA -15A ' ) -

.

--

. .

I "

SIG n f Tr( ASA ) r .e.Ezra

= for , Tr( Az SAE - A -zfAz )

Az = O .

. good variational principle .

Spin -3 charged black hole : X( chemical potential .

)

Page 8: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

A = b-' ( dta # b b -

-emo .

Asympeic Ads condition '

[ Ln .hn?--@-m)Ln-im .

A - Aids ~ OU )Wn .

→ a # = Le - 2 dell - it Wiz ) KI - z

r

Jan de Boer , Juan Jotter. 1302.0816 .

\ Solid torus .

I✓

£ ~ ZTZTL N ETI, ,

In variation,consider St : periodicity can be changed

w ~ Wtt ~ w t2TLi..

dwrdut = #td÷⇐, . .

d5= dzdE=

Upshot :

• keep volume dando =

4TdE_Tenth ) i

④ Add boundary term

⇒ Variational principle .

Page 9: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

Az -

- O,

82=0.

⇒ Ion- shell = iL÷ff÷⇒Tr[ Eat - EEE )

=i fE÷a

, @ Ice - Esea )(a. c:¥¥⇒

* No spin - 3 chemical potential .

⇒ No NCE ) in action : future work.

* fo : const . csolution ⇒ BTF..

( Lo > O )→ ABIE = Li - fol - l

AE hI£Ao¥ Iz ) htt ) .

h : smooth residualgauge

transf !↳ does not chang hdonomy ( can be connected

* Holonomy alongEuclidean eine direst identity .

Hol CA ) =b-lh-ie-whbcju-raceiblecyde.ca#nmge )

smoothness condition

W = Caz f- I Az ~ Zai Lo.

Euclidean BH .

⇒ e - if2TCLo a

Page 10: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

Change holonomy → change e.

fluctuation→ See =o implies So : fixed ( around fixed

② finite temperature Schwarzman ? background .

* Difficult to parametrize large & smoothgauge

transfseparately .

⇒ Give. up the finite transf

.

he large h- or

do -_Je LEO

( smooch fluctuation aroundLIFO

stationary background )* Consider fixed fo → infinitesimal residual gauge→

( stationary background) transf- y

'

. g-uant.ee smooth residualgauge

transf.

→ h= I teh "t 's E

' "D 't * ' I.

3×3K "

.I ' ' : traceless # aerix

8 d. of 8. d. of

Geqs .

2 parameter .

1st order :

gauge fixing condition ⇒ N, §

2nd order e. . → n

'

. 5475 .

begs .

fat,87

2 parameter .

Page 11: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

Ion- Ey Io t C- I "

t EI" '

± . -- .

-

toed derivative

-Vanishes at a- 0.tl

,

&vanish at n' -0 , It ,I2

.

graviton spin 3 field.

It.

Vasiliev equation ( SL CN ) ).

DC TAC - CF -

- O.

* For seaeionarybackground

Ccr ,E. Z ) = BID e- AKZZCoe-aem-Eb-l.gg

* For non - constant A.

shr '

e- t.ee- fi :#

⇐ e-si :*

he - so Genii classical )Q

Icr , zrzizsz ' )

= ercot-erflim.me - IIe. e-

SEE )r.s.ae

'

.

Wilson line.

Trc )s

-

.

↳ °o°.

"

highest weight"

Page 12: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

* OI CEE . . E. E.) = finesse" "

Ecr . Ez , ⇒ E. )

: boundary - to -

boundary propagator.

-⇒ geodesic distance .

* For Non - constant background ⑦⇒ gravitationally dressed

Wilson line Cmaseer field )

by boundary graviton( soft )

* Soft mode expansionh= I t NCH t . - - -

⇒ §dressed

=

↳ Mn& anode expansion )

⇐ i. ⇒ Boca . . Ht znnfn.

@dressed

, . .

,

I

↳ ( Zi , Zz )

: two - point function

in constant background

( Ezdressedcz . .z . ) &dressed

⇒ S

= GG.4Gcs.ci ) t cnn.n-nyfmEU.nfnfks.ci/

= + e . .

Page 13: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

* Soft mode eigenfunction [email protected] ,-

= Er Cir )

=

& #dressed

#

GUY

X -

- lzczitza ) , G- Iz CF - Zz )

quantumfluctuate -

②. @

dressed=

'

+ qfnngfdres.ie .-

n

µ ,@dressed

y ~ fun @dressed - - -

Ward ideneiey

* Ws - transf of two point function ?

At least , a special operator .

Observation : null relation in Way minimal modelin Large C .

( II :O ) ( dual to scalar field )

[email protected]= -

- . .

La → Iz,

Page 14: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

(( z → e-"# for finite temperature .

u

§ 197 = Gain fan ( x , o )

* Conjecture .

for null relations.

HE '0 n CL-it "¢

gthen

,we can fix coefficient

.

→ Sgs , L 7 = Hypergeometric functions.

appears in STK model

as basis in limit q→N , n → 1,

They are solution of

Page 15: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

* Recursion relation.

We know

[email protected]

tfrom 04 > transf ← from coyfoz.mg/eransf .

- f. ( X ,= Zz fun ( XO )

1h

* Can we conserve fan ( XD ) out of fssn ?

51=1 , 2,

- - -

,S - C

.

fan I >

e-" " Xgs.ncoystffs.n.fssn.ws :& ,

transl ihy of center of coordinates( ska ) talk ) )

* We found that- 5lgsmCo )Gses , a

= I Gain ( O ) t45-1

Then, we have .

Js , n (G) = O for n = O , II. 12 ,

- -

; Est .

( fan ,fs

, a > ~ Sss ' fan '

=) Solution for recursion relations.

Page 16: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

* Four point functions.

¥¥dresed!④

in Gaa )

one spin - s fieldexchange .

es, es ,dressed

dressed

{ 5ns - n > 898 SEE.

I A

AnalyticFaction 070C ~1e¥GtH .

C -

Lyapunov exponent : ⇒ Cst )

: violate -the bound on chaos ( for s > 2)

⇒ Semi - classical limit : non - unitary .

Page 17: ESI Chaos - TU Wienquark.itp.tuwien.ac.at/~grumil/ESI2019/talks/yoon.pdf · Chaos in 3D Higher spin Gravity Based on 1903 08761 Prithvi Narayan TY (1903. 09086 Viktor Jahnke Keun-Young

I corrections .

( E correction toLyeayygnon)

Interesting to study⇐ 3. a > SEELE

( 5=2 ) £÷→t Ise . - -. ) t - - -

loop correction.

+ f t + ..

E

Gis - n > Tsm .su#nSnEf.nS.nEl Ee - c- - E .

E E t - - -

t t + . . .

Es - c - Ia Ia - C - I ,

5555788 ESE.