The large N limit of Field Theories and Gravity

Transcript Of The large N limit of Field Theories and Gravity
QCD, Strings and Black holes
The large N limit of Field Theories and
Gravity
Juan Maldacena
Field Theory
=
Gravity theory
Gauge Theories QCD
Plan
QCD, Strings, the large N limit Supersymmetric QCD
N large
Gravitational theory in 10 dimensions
Calculations Correlation functions Quark-antiquark potential
Black holes
Quantum Gravity String theory
Strings and Strong Interactions
Before 60s Æ proton, neutron Æ elementary During 60s Æ many new strongly interacting particles Many had higher spins s = 2, 3, 4 …. All these particles Æ different oscillation modes of a string.
This model explained “Regge trajectories”
Rotating String model
m2 ~ TJmax + const
From E. Klempt hep-ex/0101031
Strong Interactions from Quantum ChromoDynamics
Experiments at higher energies revealed quarks and gluons
3 colors (charges) They interact exchanging gluons
Electrodynamics
photon
g
g
electron
Gauge group
U(1)
Chromodynamics (QCD)
g
g gluon
SU(3)
3 x 3 matrices
Gluons carry color charge, so they interact among themselves
Coupling constant decreases at high energy
Gross, Politzer, Wilczek
g
0
at high energies
QCD is easier to study at high energies
Hard to study at low energies Indeed, at low energies we expect to see confinement
q
q
Flux tubes of color field = glue
V = T L
At low energies we have something that looks like a string
Can we have an effective theory in terms of strings ?
Large N limit
Take N colors instead of 3, SU(N)
t’ Hooft ‘74
Large N and strings
Gluon: color and anti-color
Open strings Æ mesons Closed strings Æ glueballs Looks like a string theory, but…
1. Simplest action = Area
Not consistent in D=4 ( D=26 ? )
generate
At least one more dimension (thickness)
Polyakov
2. Strings theories always contain a state with m=0, spin =2: a Graviton.
For this reason strings are commonly used to study quantum gravity
Scherk-Schwarz Yoneya
We combine these two problems into a solution. We will look for a 5 dimensional theory that contains gravity. We have to find an appropriate 5 dimensional curved spacetime.
Most supersymmetric QCD
Supersymmetry Bosons
Fermions
Ramond Wess, Zumino
Gluon
Gluino
Many supersymmetries
B1
F1
B2
F2
Maximum 4 supersymmetries, N = 4 Super Yang Mills
Aμ Vector boson Ψα 4 fermions (gluinos) ΦI 6 scalars
All NxN matrices
spin = 1 spin = 1/2 spin = 0
SO(6) symmetry
Susy might be present in the real world but spontaneously broken at low energies.
We study this case because it is simpler.
Similar in spirit to QCD
Difference: most SUSY QCD is scale invariant Classical electromagnetism is scale invariant V = 1/r QCD is scale invariant classically but not quantum mechanically, g(E)
Most susy QCD is scale invariant even quantum mechanically
Symmetry group Lorentz + translations + scale transformations + other
The string should move in a space of the form
ds2 = R2 w2 (z) ( dx23+1 + dz2 )
redshift factor = warp factor ~ gravitational potential
Demanding that the metric is symmetric under scale transformations x Æ λ x , we find that w(z) = 1/z
ds2 = R2 (dx23+1 + dz2) z2
R4
Boundary
AdS5
z
z = 0
z = infinity
This metric is called anti-de-sitter space. It has constant negative curvature, with a radius of curvature given by R.
w(z)
Gravitational potential
z
The large N limit of Field Theories and
Gravity
Juan Maldacena
Field Theory
=
Gravity theory
Gauge Theories QCD
Plan
QCD, Strings, the large N limit Supersymmetric QCD
N large
Gravitational theory in 10 dimensions
Calculations Correlation functions Quark-antiquark potential
Black holes
Quantum Gravity String theory
Strings and Strong Interactions
Before 60s Æ proton, neutron Æ elementary During 60s Æ many new strongly interacting particles Many had higher spins s = 2, 3, 4 …. All these particles Æ different oscillation modes of a string.
This model explained “Regge trajectories”
Rotating String model
m2 ~ TJmax + const
From E. Klempt hep-ex/0101031
Strong Interactions from Quantum ChromoDynamics
Experiments at higher energies revealed quarks and gluons
3 colors (charges) They interact exchanging gluons
Electrodynamics
photon
g
g
electron
Gauge group
U(1)
Chromodynamics (QCD)
g
g gluon
SU(3)
3 x 3 matrices
Gluons carry color charge, so they interact among themselves
Coupling constant decreases at high energy
Gross, Politzer, Wilczek
g
0
at high energies
QCD is easier to study at high energies
Hard to study at low energies Indeed, at low energies we expect to see confinement
q
q
Flux tubes of color field = glue
V = T L
At low energies we have something that looks like a string
Can we have an effective theory in terms of strings ?
Large N limit
Take N colors instead of 3, SU(N)
t’ Hooft ‘74
Large N and strings
Gluon: color and anti-color
Open strings Æ mesons Closed strings Æ glueballs Looks like a string theory, but…
1. Simplest action = Area
Not consistent in D=4 ( D=26 ? )
generate
At least one more dimension (thickness)
Polyakov
2. Strings theories always contain a state with m=0, spin =2: a Graviton.
For this reason strings are commonly used to study quantum gravity
Scherk-Schwarz Yoneya
We combine these two problems into a solution. We will look for a 5 dimensional theory that contains gravity. We have to find an appropriate 5 dimensional curved spacetime.
Most supersymmetric QCD
Supersymmetry Bosons
Fermions
Ramond Wess, Zumino
Gluon
Gluino
Many supersymmetries
B1
F1
B2
F2
Maximum 4 supersymmetries, N = 4 Super Yang Mills
Aμ Vector boson Ψα 4 fermions (gluinos) ΦI 6 scalars
All NxN matrices
spin = 1 spin = 1/2 spin = 0
SO(6) symmetry
Susy might be present in the real world but spontaneously broken at low energies.
We study this case because it is simpler.
Similar in spirit to QCD
Difference: most SUSY QCD is scale invariant Classical electromagnetism is scale invariant V = 1/r QCD is scale invariant classically but not quantum mechanically, g(E)
Most susy QCD is scale invariant even quantum mechanically
Symmetry group Lorentz + translations + scale transformations + other
The string should move in a space of the form
ds2 = R2 w2 (z) ( dx23+1 + dz2 )
redshift factor = warp factor ~ gravitational potential
Demanding that the metric is symmetric under scale transformations x Æ λ x , we find that w(z) = 1/z
ds2 = R2 (dx23+1 + dz2) z2
R4
Boundary
AdS5
z
z = 0
z = infinity
This metric is called anti-de-sitter space. It has constant negative curvature, with a radius of curvature given by R.
w(z)
Gravitational potential
z