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BRANE SOLUTIONS AND RG FLOW. FRANCISCO A. BRITO. UNIVERSIDADE FEDERAL DE CAMPINA GRANDE. September 2006. BRANE SOLUTIONS AND RG FLOW. INTRODUCTION. Compactification - Factorizable - Non-factorizable ( phenomenology d=4 ) - PowerPoint PPT Presentation

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BRANE SOLUTIONS AND RG FLOW

UNIVERSIDADE FEDERAL DE CAMPINA GRANDE

September 2006

FRANCISCO A. BRITO

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

INTRODUCTION

i) Compactification

- Factorizable

- Non-factorizable

(phenomenology d=4)

* Other interests (BTZ black holes, gravity in 2d string theory, and sugra 10 and 11 to lower dimensions > 4)

ii) Dualidade gauge/gravity (e.g. AdS/CFT)

- gravity duals (brane solutions): D - dimensions

- RG flow of a dual field theory: (D-1) - dimensions

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

BOSONIC STRINGSBOSONIC STRINGS

SUPERSTRINGSSUPERSTRINGS

COMPACTIFICATIONS OF COMPACTIFICATIONS OF SIX DIMSIX DIM

D = 26

D = 10

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

BOSONIC STRINGSBOSONIC STRINGS

SUPERSTRINGSSUPERSTRINGS

COMPACTIFICATIONS OF SIX DIMCOMPACTIFICATIONS OF SIX DIM

D = 26

D = 10

M10 = M4 X K6“factorizable geometry”

Compact 6-manifold

Our four dim universe

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

OUR UNIVERSE ON A 3-BRANE

Randall & Sundrum, (1999)

AN ALTERNATIVE TO COMPACTIFICATION

3-BRANEr

NON-COMPACT DIMENSION

M4 ½ AdS5

NON-FACTORIZABLE

“WARPED GEOMETRY”

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

AdS5 METRIC

, = 0, 1, 2, 3(brane world-volume indices)

e 2A(r) ≡ warp factor

ds52= e2A(r) dx dx + dr2

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

THE Randall-Sundrum SCENARIO

r

A (r)

r

e 2A (r)

SOLUTION:|5| = 12 k2 = σ2 / 12

A = - k |r|

branebulk

xdrRgxdS 55

5 )(

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRAVITY FLUCTUATIONS

h

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRAVITY FLUCTUATIONS

h

)()()]([ 22 rmrrVr

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRAVITY FLUCTUATIONS

H (r) = m2 (r) H = Q+ Q

Q = r + 3 r A(r)_2

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRAVITY FLUCTUATIONS

SOLUTION:

Zero Mode: m = 0

H (r) = m2 (r) H = Q+ Q

Q = r + 3 z A(r)_2

H o = 0 ) Q o = 0 ) o e 3/2 A(r)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRAVITY FLUCTUATIONS

SOLUTION:

Zero Mode: m = 0

H (r) = m2 (r) H = Q+ Q

Q = r + 3 r A(r)_2

H o = 0 ) Q o = 0 ) o e 3/2 A(r)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

r

o e -3/2 k |r|

Localization of Gravity!

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRAVITY FLUCTUATIONS

SOLUTION:

r

Zero Mode: m = 0

Localization of gravity!

H (r) = m2 (r) H = Q+ Q

Q = r + 3 r A(r)_2

H o = 0 ) Q o = 0 ) o e 3/2 A(r)

o e -3/2 k |r|

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

z

V(z)

Massive modes

z

V(z)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

Massive modes

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

z

V(z)KK modes

Massive modes

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

z

V(z)

Massive modes

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

Massive modes

Correction of Newtonian Potential!

3521

40

52144 )(

|)0(|kRG

Rmm

GedmRG

Rmm

GU mmR

D

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRS SCENARIO

Massive gravity: metastable gravity

Gregory, Rubakov & Sibiryakov (2000)

222 )( drdxdxrads

crk

crk

rrae

rrera

c

0)(

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRS SCENARIO

Massive gravity: metastable gravity

Gregory, Rubakov & Sibiryakov (2000)

222 )( drdxdxrads

crk

crk

rrae

rrera

c

0)(

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GRS SCENARIO Flat brane embeded into 5d Minkowski

bulk: infinite volume!

No zero modes

rc rcσ < 0 σ < 0σ > 0

0

A

r

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

ASYMMETRIC BRANESBrito & Gomes (work in progress)

2||2222/)3|(|2 )( dredxdxedteds rkiirkrrk

Finite volume massive modes

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

U (R) ~ 1 / R L

L

log R

1

2

R >> RcR << Rc

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

LOCALLY LOCALIZED GRAVITY Karch & Randall (2001)

ds2= eA(r) gdx dx + dr2-ds2= eA(r) gdx dx + dr2-

Λ > 0-

Λ = 0-

Λ < 0-

dS4

M4

AdS4

Λ → four dimensional-

cosmological constant

gR

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

LOCALLY LOCALIZED GRAVITY

r

A (r)

AdS4 (Local localization)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

A = -k |r|

M4

LOCALLY LOCALIZED GRAVITY

r

A (r)

AdS4 (Local localization)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

LOCALLY LOCALIZED GRAVITY

r

A (r)

A = -k |r|

M4

dS4

“No global issues !”

e. g. infinite volume

AdS4 (Local localization)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SCHROEDINGER POTENTIAL

z

V (z) AdS4

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SCHROEDINGER POTENTIAL

z

V (z)

M4

AdS4

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SCHROEDINGER POTENTIAL

z

V (z)

M4

AdS4

dS4

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SCHROEDINGER POTENTIAL

z

V (z) AdS4

Quase-zeromode emerges M4

dS4

(Massive) GRAVITY LOCALIZATION : A LOCAL EFFECT !!

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

GEOMETRIC TRANSITIONS & LOCALLY LOCALIZED GRAVITY

Brito, Bazeia & Gomes (2004)Λ = L-2 [ σ (T)2 – σ* ]-Λ = L-2 [ σ (T)2 – σ* ]-

4 dim cosmological constant

Brane tension depending on temperature

T

σ

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

dS4M4AdS4

Susy Breaking

Λ = 0-

Λ < 0- Λ > 0

-

0T*∞ critical temperature

T

GEOMETRIC TRANSITIONS & LOCALLY LOCALIZED GRAVITY

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SUPERGRAVITY ACTION

5 dim cosmological constant

→ critical points

W - superpotential

5*2 0)()( WV

; *

FermionsVgRexdS NmMN )(5

22

* )( WWV

0*

W

Cvetic et al (2000)Brito & Cvetic (2001)Bazeia, Brito & Nascimento (2003)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SUPERGRAVITY ACTION

CONTENTS TURNED ON

Supergravity multiplet: (eam, i

m)

Scalar super multiplet:( , i

m)S = 0

im ea

m ;;;

UNDER SUSY TRANSFORMATIONS!!!!UNDER SUSY TRANSFORMATIONS!!!!

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

THE SUSY FLOW EQUATIONS

= 0

n = 0

ds2= a2 (r) dx dx + dr2

KILLING EQUATIONS

))

(i)’ = ± 3 g i j j W

g i j - metric definied on moduli space

energy scale (AdS/CFT))(22 )( rAera

WrA )(' or Waa

'

Skenderis & Townsend (1999)Freedman et al (1999)Kallosh & Linde (2000)Cvetic & Behrndt (2000)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

THE SUSY FLOW EQUATIONS

CRITICAL POINTS

i (r →∞) = i * ) (i)’ = 0

) j W (i* ) = 0

) kWaa

'

krera )(

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

THE SUSY FLOW EQUATIONS

CRITICAL POINTS

i (r →∞) = i * ) (i)’ = 0

) j W (i* ) = 0

W

*

*Flow

) kWaa

'

krera )(

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

RG EQUATION

Wg jiji 3)( '

X ara

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

RG EQUATION

where

Wg jiji 3)( '

Warag

ara j

iji

3'

)(3 ijiji

WW

ga

a

0)( * i

a – energy scalei - couplings

RG EQUATION ON THE FIELD THEORY SIDE

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

RG EQUATION

where

Wg jiji 3)( '

Warag

ara j

iji

3'

)(3 ijiji

WW

ga

a

0)( * i

iii * ...)()( **

i

jjj

i

)()( **

i

jjj

i

aa

j

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

RG EQUATION

where

Wg jiji 3)( '

Warag

ara j

iji

3'

)(3 ijiji

WW

ga

a

0)( * i

iii *...)()( **

i

jjj

i

)()( **

i

jjj

i

aa

** 3)(

WW

g jiiji

j

Restrictions on W?

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SPECIAL GEOMETRIES

Thus we find

Assuming perturbation as

)(32)( ** WgW ijji

iji

j

2)( *

)2(...)( ij

ji

jji

i

aa

ac ii ; ci = constant

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SPECIAL GEOMETRIES

STABLE CRITICAL POINT

i) SUGRA D = 5

Not good for Not good for localizing gravity!localizing gravity!

) UV FIXED POINT (QFT)

QFT on AdS boundary

r

e 2 A ( r)

IR UV AdS5 solution: a (r) = e k r

UNSTABLE IR

> 0 r →∞

a →∞ i → 0 ;0

i

j

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SPECIAL GEOMETRIES ii) GRAVITY LOCALIZATION < 0

AdS5 solution:

a (r) = e -k r

i = ci a ||:

“IR FIXED POINT”STABLE CRITICAL POINT r →∞

a → 0 i → 0 ;

0

i

j

r

e 2 A ( r)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

SPECIAL GEOMETRIES

STABLE CRITICAL POINT r →∞

a → 0 i → 0 ;

INTRODUCING A BRANE: a (r) = e –k |r|

zero modeo e-k|r|

Two copies of AdS5 pasted

together

LOCALIZATION OF GRAVITY!!(Massless)

r

e 2 A ( r)

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM AND “BENT” BRANES: Freedman et al. (2004)Bazeia et al. (2006)Brito, Bazeia, Losano (work in progress)

NEW DEVELOPMENTSNEW DEVELOPMENTS

),...,(

21...

21

41|| 111

4NNN VRgdrxdS

““fake sugra”fake sugra”

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM AND “BENT” BRANES: Freedman et al. (2004)Bazeia et al. (2006)Brito, Bazeia, Losano (work in progress)

NEW DEVELOPMENTSNEW DEVELOPMENTS

),...,(

21...

21

41|| 111

4NNN VRgdrxdS

“BENT” BRANE GEOMETRIES

2)(225 drdxdxgeds rA

3,2,1,0,

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM AND “BENT” BRANES: Freedman et al. (2004)Bazeia et al. (2006)Brito, Bazeia, Losano (work in progress)

NEW DEVELOPMENTSNEW DEVELOPMENTS

),...,(

21...

21

41|| 111

4NNN VRgdrxdS

“BENT” BRANE GEOMETRIES

3,2,1,0, 2)(225 drdxdxgeds rA

gR

0;)(

0;

0;)(

23

22

21

22

23

22

21

2

23

22

21

22

3 dxdxdxdte

dxdxdxdt

dxdxdxedt

dxdxgx

t

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM AND “BENT” BRANES:

NEW DEVELOPMENTSNEW DEVELOPMENTS

EQUATIONS OF MOTION

NNN

VA

VA

''''

1

'1

'''1 4,...,4

)...(32 2'2'

12''

NAeA

),...,(31)...(

61

12'2'

122'

NNA VeA

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM

i) MINKOWSKI BRANES: 0

22

11 3

181),...,( WWV

N

i iN

FIRST ORDER EQUATIONS

Wii 21' NiWW

ii ,...,2,1,

WA31'

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM

FIRST ORDER EQUATIONS

ii) “BENT” BRANES: 0

2

11 )(

31)3()(

81),...,( ZWZWZWV

N

iiiiiiiN

NiZW iii ,...,2,1;)(21

ZWA 31'

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM

FIRST ORDER EQUATIONS

ii) “BENT” BRANES: 0

2

11 )(

31)3()(

81),...,( ZWZWZWV

N

iiiiiiiN

034

)(2...

ZZWZZW iiiiiii

CONSTRAINTSCONSTRAINTS

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM

FIRST ORDER EQUATIONS

ii) “BENT” BRANES: 0

2

11 )(

31)3()(

81),...,( ZWZWZWV

N

iiiiiiiN

034

)(2...

ZZWZZW iiiiiii

NiZW iii ,...,2,1;)(21

ZWA 31'

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

FIRST ORDER FORMALISM

iii) BETA FUNCTION

ZW

ZWa

a iii

i

)(

23

)(

*

2*'

)()()()(

23)(

ZW

ZWZWZW

ZW iiiiiii

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

EXAMPLES

r

A

r

32

32 babW

)(tanh1 2 rbab

0i) 0* W

)(tanh91)(secln

94 22

22

2 rabb

rabhb

A )(tanh91)(secln

94 22

22

2 rabb

rabhb

A 0)( * i

029)(

2*'

bi

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

EXAMPLES

r

A

r

32

32 babW

)(tanh1 2 rbab

)(tanh91)(secln

94 22

22

2 rabb

rabhb

A

0* W0i)

0)( * i 029)(

2*'

bi

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

r

EXAMPLESii) Z;0

)sinh(baW

A

r

rbabababh

b2222

41tanarctan2

)(cos26ln21

2222412

2222

rbababab

baA

0)( * i

023*)(

2'

bi

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

ii) EXAMPLES

r Z;0

)sinh(baW

A

r

rbabababh

b2222

41tanarctan2

)(cos26ln21

2222412

2222

rbababab

baA

0)( * i 023*)(

2'

bi

BRANE SOLUTIONS AND RG FLOWBRANE SOLUTIONS AND RG FLOW

CONCLUSIONSi) D=4 is phenomenologically motivated

ii) Infinite volume implies no zero modes

iii) Warp factor regarded as energy scale on dual theory

iv) Bent branes may give a dual gravitational description of RG flows in susy field theories in a curved spacetime

v) Theories in AdS spaces exhibit improved infrared behavior

Th e Th e E n d E n d

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