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Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo Galilei Institute, Florence, May 2013 [Aharony, GA, Yacoby 2011, 2012] [GA, Yacoby 2012] [Aharony, Giombi, GA, Maldacena, Yacoby 2012]

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Page 1: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Chern-Simons-Matter Theories, High-Spin Gravity,

and 3D Bosonization

Guy Gur-AriWeizmann Institute, Israel

The Galileo Galilei Institute, Florence, May 2013[Aharony, GA, Yacoby 2011, 2012] [GA, Yacoby 2012][Aharony, Giombi, GA, Maldacena, Yacoby 2012]

Page 2: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Vector Models in 3D

• Complex scalars

• Singlet sector of

• Single-trace primaries:

i = 1, . . . , N

s = 0, 1, 2, . . .Js = �†

i@ · · · @�i

U(N)

�s = s+ 1

L = @µ�†i@µ�

i +�6

N2(�†

i�i)3

Page 3: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

• Singlet sector of

• Single-trace primaries:

Vector Models in 3DL = i�

µ@µ i

J0 = Js = �@ · · · @ �0 = 2

�s = s+ 1

s = 1, 2, . . .

U(N)

Page 4: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Outline

• 3D vector models ↔ high-spin gravity

• Matter + Chern-Simons interactions

• 3D bosonization

Page 5: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Vasiliev’s Theory

• Defined on AdS4

• Scalar, photon, graviton, ...

• Consistent, classical interacting theory

dx

A+ A ⇤ A =

1

4+ ei✓0B ⇤K

�dz2 + c.c.

dx

B + A ⇤B �B ⇤ ⇡(A) = 0

Page 6: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Holographic Duality

[Sezgin, Sundell 2001]

GN ⇠ 1

NJ0, Js ! B, A ✓0 = 0

✓0 = ⇡/2

Boundary scalars:

Boundary fermions:

Page 7: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

• dimension:

• Currents not renormalized at large N

• Bulk: change of scalar boundary conditions

Critical Vector Model

Wilson-Fischer

[Klebanov, Polyakov 2002]

Free Scalars�L ⇠ (�†�)2

J0 �IR0 = d��0 = 2

Page 8: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Detailed Evidence

• Conformal theory in flat 3D space + high-spin symmetry ⇒ free theory[Maldacena, Zhiboedov 2011]

• All 3-point functions agree[Giombi, Yin 2010]

Page 9: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Motivation• Weak-weak duality

• Tensionless limit of string theory[Chang, Minwalla, Sharma, Yin 2012]

• Boundary scalars and fermions continuously connected

Page 10: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Bulk Suggests Bosonization

Boundary Scalars

BoundaryFermions

Boundary scalars / fermions are connected

0 ⇡/2

dx

A+ A ⇤ A =

1

4+ ei✓0B ⇤K

�dz2 + c.c.

(Parity)✓0

Page 11: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Bulk Suggests Bosonization

Free ScalarsJ0 = �†�

� = 1

Critical Scalars� = 2

Critical Fermions� = 1

J0 =

� = 2

Free Fermions

0 ⇡/2✓0 (/P)

✓0 (/P)

Page 12: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Matter +Chern-Simons

Interactions

Page 13: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Why Chern-Simons?

• symmetry already gauged

• No additional primary operators

Smatter +ik

4⇡

ZTr

✓A ^ dA+

2

3A3

� =N

kN, k ! 1

U(N)

Page 14: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

• Chern-Simons level k is quantized

• deformation marginal at large N

• Theory is conformal at large N

Conformal Symmetry

(�†�)3

[Giombi, Minwalla, Prakash, Trivedi, Wadia, Yin 2011][Aharony, GA, Yacoby 2011]

Smatter +ik

4⇡

ZTr

✓A ^ dA+

2

3A3

Page 15: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Fate of the High-Spin Symmetry

Currents not renormalizedat large N

@ · hJsJs0i = 0

Symmetry is broken, not renormalized

@ · hJsJs0Js00i 6= 0

�� s = 3

J0

@ · Js ⇠ 0 +1

NJs�2J0 + · · ·

Page 16: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

3D BosonizationFree Scalar

J0 = �†�

� = 1

Critical Scalar� = 2

Critical Fermion� = 1

J0 =

� = 2

Free Fermion

0 ⇡/2✓0 (/P)

✓0 (/P)

Page 17: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

• General theory, high-spin symmetry ‘slightly’ broken:

• Broken Ward identities constrain correlators

• 3-point functions of single-trace operators fixed by two parameters

CFT Perspective

[Maldacena, Zhiboedov 2012]

hJJJi�=1

= N

"1

1 + �2

h·ibos. +

�2

1 + �2

h·ifer. +

1 + �2

h·iodd

#N , �

?

@ · Js ⇠ Js�2J0/N + · · ·

N , � $ N,� = N/k

Page 18: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Computing Exact Correlators

hJ0J0i = J0 J0 + · · ·

hTT i , hJ0J0J0i , · · ·

[Aharony, GA, Yacoby 2012] [GA, Yacoby 2012]

h��†i

h��†��†i

Page 19: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Degrees of FreedomhTT i

hTT ifree=

sin(⇡�)

⇡�

0.0 0.2 0.4 0.6 0.8 1.0 1.2

0.0

0.2

0.4

0.6

0.8

1.0

l

(� = N/k)

[Aharony, GA, Yacoby 2012] [GA, Yacoby 2012]

Page 20: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Exact Correlators

✓0 =⇡�

2Bulk coupling:

hJJJi�=1

= N

"1

1 + �2

h·ibos. +

�2

1 + �2

h·ifer. +

1 + �2

h·iodd

#

=

2N sin(⇡�)

⇡�

"cos

2

✓⇡�

2

◆h·i

bos. + sin

2

✓⇡�

2

◆h·i

fer.

+

sin (⇡�)

2

h·iodd

#

[Aharony, GA, Yacoby 2012] [GA, Yacoby 2012]

[Chang, Minwalla, Sharma, Yin 2012]

hJ0J0J0i, . . .(� = N/k)

Page 21: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

• Comparing correlators gives relation

• Level-rank duality in terms of

Bosonization Duality

k0 = k � sign(k)N

Scalar + U(N)k0

Critical Fermion + U(k0)�N

(Scalars) (Fermions)N,� $ N,�

� = 0

� = 1 � = 0

� = 1

(� = N/k)

Page 22: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Thermal Free Energy• Thermal cycle can support non-trivial

holonomy

• Eigenvalues hold gauge-invariant info

[Aharony, Giombi, GA, Maldacena, Yacoby 2012]

IA 6= 0

NV T 2 � N2

Matter sectorAttractive potential

Pure Chern-Simons

F/T :

Page 23: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Non-Trivial Holonomy

[Aharony, Giombi, GA, Maldacena, Yacoby 2012]

T 2 ⇥ R

SCS ! k

2⇡

Zdt a b

Reduce on

b ⇠= b+ 2⇡ ) �a =2⇡

k

Eigenvalues are quantized & fermionic,Spread evenly: 2⇡

kN = 2⇡�

!

!" "!"# "#

⇡b =k

2⇡a

[Douglas, 94]

a, b =

I

⌃1,2

A =

✓. . .

1,2

Page 24: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Thermal Free Energy

• Free energy computed by summing planar diagrams

• Consistent with bosonization

[Aharony, Giombi, GA, Maldacena, Yacoby 2012]

Ff = �NV2T 3

2⇡2i�

µ2

3Li2

��e�µ+⇡i�

�+

Z 1

µdy y Li2

��e�y+⇡i�

�� c.c.

(1� �)µ =1

⇡i

⇥Li2(�e�µ�⇡i�)� c.c.

⇤Thermal mass

Page 25: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

Open Questions• Better understand bosonization

• 1/N

• Mapping of fundamental fields

• Better understand holographic duality

• Singlet sector implementation

• Pure Chern-Simons contributions[Banerjee, Hellerman, Maltz, Shenker 2012]

Page 26: Chern-Simons-Matter Theories, High-Spin Gravity, and 3D ... · Chern-Simons-Matter Theories, High-Spin Gravity, and 3D Bosonization Guy Gur-Ari Weizmann Institute, Israel The Galileo

• Vector models + Chern-Simons are dual to Vasiliev’s theory with broken parity

• 3D bosonization

• Single-trace 3-point functions, thermal free energy

Summary

Thank You

Scalar + U(N)k0

Critical Fermion + U(k0)�N

� = 0

� = 1 � = 0

� = 1