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Page 1: Why Quantum Gravity-An introductory survey.pdf

8/19/2019 Why Quantum Gravity-An introductory survey.pdf

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Quantum Gravity

An introductory survey

Hermann Nicolai 

Max-Planck-Institut f ¨ ur Gravitationsphysik 

(Albert–Einstein–Institut, Potsdam)

. – p.1/25

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Why Quantum Gravity?

. – p.2/25

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Why Quantum Gravity?

General Relativity and Quantum Theory: not only verydifferent domains of validity, but very different  theories:

. – p.2/25

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Why Quantum Gravity?

General Relativity and Quantum Theory: not only verydifferent domains of validity, but very different  theories:

General Relativity: smoothness and geometry

. – p.2/25

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Why Quantum Gravity?

General Relativity and Quantum Theory: not only verydifferent domains of validity, but very different  theories:

General Relativity: smoothness and geometryQuantum Mechanics: probability and uncertainty

. – p.2/25

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Why Quantum Gravity?

General Relativity and Quantum Theory: not only verydifferent domains of validity, but very different  theories:

General Relativity: smoothness and geometryQuantum Mechanics: probability and uncertainty

Einstein equations tie together matter and geometry :

Rµν  −  1

2gµν R

         classical?

=   κT µν 

    quantum?

→ mathematical and conceptual inconsistencies?

. – p.2/25

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Unsolved Questions

. – p.3/25

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Unsolved Questions

Singularities in General Relativity (GR) – Black holes: gravitational collapse generically unavoidable

 – Cosmological ("big bang") singularity: what ‘happened’ at t  = 0?

 – Singularity theorems: space and time ‘end’ at the singularity

. – p.3/25

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Unsolved Questions

Singularities in General Relativity (GR) – Black holes: gravitational collapse generically unavoidable

 – Cosmological ("big bang") singularity: what ‘happened’ at t  = 0?

 – Singularity theorems: space and time ‘end’ at the singularity

Singularities in Quantum Field Theory (QFT) – Perturbation theory: UV divergences in Feynman diagrams

 – Can be removed by infinite renormalizations order by order

 – But: Standard Model (or its extensions) unlikely to exist as rigorous QFTs

. – p.3/25

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Unsolved Questions

Singularities in General Relativity (GR) – Black holes: gravitational collapse generically unavoidable

 – Cosmological ("big bang") singularity: what ‘happened’ at t  = 0?

 – Singularity theorems: space and time ‘end’ at the singularity

Singularities in Quantum Field Theory (QFT) – Perturbation theory: UV divergences in Feynman diagrams

 – Can be removed by infinite renormalizations order by order

 – But: Standard Model (or its extensions) unlikely to exist as rigorous QFTs

Difficulties have similar origin: – Spacetime as a continuum  ( = differentiable manifold) in GR and QFT

 – Elementary particles as pointlike excitations  in GR and QFT

. – p.3/25

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Unsolved Questions

Singularities in General Relativity (GR) – Black holes: gravitational collapse generically unavoidable

 – Cosmological ("big bang") singularity: what ‘happened’ at t  = 0?

 – Singularity theorems: space and time ‘end’ at the singularity

Singularities in Quantum Field Theory (QFT) – Perturbation theory: UV divergences in Feynman diagrams

 – Can be removed by infinite renormalizations order by order

 – But: Standard Model (or its extensions) unlikely to exist as rigorous QFTs

Difficulties have similar origin: – Spacetime as a continuum  ( = differentiable manifold) in GR and QFT

 – Elementary particles as pointlike excitations  in GR and QFT

Structure of space-time at the smallest distances?‘Smallest distance’: Planck scales   P  ∼ 10−33cm   and   tP   = 10−43sec

[Planck mass:   M P   = 1019 GeV ∼ 10−5g ]

. – p.3/25

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Geometry and Matter

. – p.4/25

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Geometry and Matter

Einstein’s equations once more:

Rµν 

 − 1

2

gµν R         Marble?

=   κT µν     Timber?

. – p.4/25

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Geometry and Matter

Einstein’s equations once more:

Rµν 

 − 1

2

gµν R         Marble?

=   κT µν     Timber?

Question:  can we understand the r.h.s. geometrically?

. – p.4/25

G d M

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Geometry and Matter

Einstein’s equations once more:

Rµν 

 − 1

2

gµν R         Marble?

=   κT µν     Timber?

Question:  can we understand the r.h.s. geometrically?

Or:  what is the relation between gravitation and theother fundamental (strong and electroweak) forces?

. – p.4/25

G d M

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Geometry and Matter

Einstein’s equations once more:

Rµν 

 − 1

2

gµν R         Marble?

=   κT µν     Timber?

Question:  can we understand the r.h.s. geometrically?

Or:  what is the relation between gravitation and theother fundamental (strong and electroweak) forces?

And:  is the ‘geometrization’ of matter a necessary prerequi-

site for consistent quantization of gravity?

. – p.4/25

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A Basic Problem

Perturbative quantum gravity is non-renormalizable

Γ(2)div  =

 1

ε

209

2880

1

(16π2

)2    dV C µνρσC ρσλτ C λτ 

µν 

[Goroff, Sagnotti; van de Ven]

. – p.5/25

A B i P bl

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A Basic Problem

Perturbative quantum gravity is non-renormalizable

Γ(2)div  =

 1

ε

209

2880

1

(16π2

)2    dV C µνρσC ρσλτ C λτ 

µν 

[Goroff, Sagnotti; van de Ven]

Two possible conclusions:

. – p.5/25

A B i P bl

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A Basic Problem

Perturbative quantum gravity is non-renormalizable

Γ(2)div  =

 1

ε

209

2880

1

(16π2

)2    dV C µνρσC ρσλτ C λτ 

µν 

[Goroff, Sagnotti; van de Ven]

Two possible conclusions:

Consistent quantization of gravity requires inclusion of(supersymmetric) matter to cancel UV divergences; or

. – p.5/25

A B i P bl

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A Basic Problem

Perturbative quantum gravity is non-renormalizable

Γ(2)div  =

 1

ε

209

2880

1

(16π2

)2    dV C µνρσC ρσλτ C λτ 

µν 

[Goroff, Sagnotti; van de Ven]

Two possible conclusions:

Consistent quantization of gravity requires inclusion of(supersymmetric) matter to cancel UV divergences; or

UV divergences are artefacts of perturbative treatment⇒ disappear upon non-perturbative  quantization?

. – p.5/25

A B i P bl

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A Basic Problem

Perturbative quantum gravity is non-renormalizable

Γ(2)div  =

 1

ε

209

2880

1

(16π2

)2    dV C µνρσC ρσλτ C λτ 

µν 

[Goroff, Sagnotti; van de Ven]

Two possible conclusions:

Consistent quantization of gravity requires inclusion of(supersymmetric) matter to cancel UV divergences; or

UV divergences are artefacts of perturbative treatment⇒ disappear upon non-perturbative  quantization?

The real problem: infinite number of ambiguities!

(NB: This is also a problem for existing non-perturbative approaches)

. – p.5/25

Approaches to Quantum Gravity

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Approaches to Quantum Gravity

. – p.6/25

Approaches to Quantum Gravity

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Approaches to Quantum Gravity

Supergravity, Superstring and M Theory... preferred by particle theorists 

. – p.6/25

Approaches to Quantum Gravity

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Approaches to Quantum Gravity

Supergravity, Superstring and M Theory... preferred by particle theorists 

Canonical quantum gravity: geometrodynamics,loop and spin foam quantum gravity (LQG)... preferred by general relativists 

. – p.6/25

Approaches to Quantum Gravity

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Approaches to Quantum Gravity

Supergravity, Superstring and M Theory... preferred by particle theorists 

Canonical quantum gravity: geometrodynamics,loop and spin foam quantum gravity (LQG)... preferred by general relativists 

Other: – (Euclidean) Path integrals

 – Discrete quantum gravity: Regge calculus and dynamical triangulations

 – Non-commutative geometry and non-commutative space-time

 – Asymptotic safety and RG fixed points – Causal histories

 – Cellular automata

 –    . . . . . .

. – p.6/25

Canonical Quantization

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Canonical Quantization

. – p.7/25

Canonical Quantization

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Canonical Quantization

Non-perturbative  and background independent  approach:quantum metric fluctuations and quantum geometry

. – p.7/25

Canonical Quantization

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Canonical Quantization

Non-perturbative  and background independent  approach:quantum metric fluctuations and quantum geometry

Hamiltonian approach: manifest space-time covarianceis lost through split (‘foliation’) of space-time accordingto M = Σ× R with spatial manifold Σ and time  R

. – p.7/25

Canonical Quantization

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Canonical Quantization

Non-perturbative  and background independent  approach:quantum metric fluctuations and quantum geometry

Hamiltonian approach: manifest space-time covarianceis lost through split (‘foliation’) of space-time accordingto M = Σ× R with spatial manifold Σ and time  R

→ Space-time geometry as the evolution of spatial geometry in time  according to Einstein’s equations

. – p.7/25

Canonical Quantization

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Canonical Quantization

Non-perturbative  and background independent  approach:quantum metric fluctuations and quantum geometry

Hamiltonian approach: manifest space-time covarianceis lost through split (‘foliation’) of space-time accordingto M = Σ× R with spatial manifold Σ and time  R

→ Space-time geometry as the evolution of spatial geometry in time  according to Einstein’s equations

Textbook method: replace  { p, q } = 1   →   [ p, q ] = i 

. – p.7/25

Canonical Quantization

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Canonical Quantization

Non-perturbative  and background independent  approach:quantum metric fluctuations and quantum geometry

Hamiltonian approach: manifest space-time covarianceis lost through split (‘foliation’) of space-time accordingto M = Σ× R with spatial manifold Σ and time  R

→ Space-time geometry as the evolution of spatial geometry in time  according to Einstein’s equations

Textbook method: replace  { p, q } = 1   →   [ p, q ] = i 

Matter interactions are to be ignored in a first step:unification is not the primary goal of this approach!

. – p.7/25

Geometrodynamics(I)

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Geometrodynamics(I)

. – p.8/25

Geometrodynamics(I)

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Geometrodynamics(I)

= (formal) canonical quantization with metric variables 

. – p.8/25

Geometrodynamics(I)

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Geometrodynamics(I)

= (formal) canonical quantization with metric variables 

4-Metric gµν  decomposes into dynamical variables

gij   (spatial components of 4-metric)

. – p.8/25

Geometrodynamics(I)

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G y a ( )

= (formal) canonical quantization with metric variables 

4-Metric gµν  decomposes into dynamical variables

gij   (spatial components of 4-metric)

and Lagrange multipliers (→ constraints)

N  ∼ g00   (Lapse)   , N i ∼ g0i   (Shift)

. – p.8/25

Geometrodynamics(I)

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y ( )

= (formal) canonical quantization with metric variables 

4-Metric gµν  decomposes into dynamical variables

gij   (spatial components of 4-metric)

and Lagrange multipliers (→ constraints)

N  ∼ g00   (Lapse)   , N i ∼ g0i   (Shift)

thus: canonical dynamical  degrees of freedom

gij(t,x)   ,   Πij(t,x) = δ LEinsteinδ gij(t,x)

. – p.8/25

Geometrodynamics (II)

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y ( )

. – p.9/25

Geometrodynamics (II)

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y ( )

Quantization in Schrödinger picture

Πij(x)

−→

   

i

δ 

δgij(x

)

. – p.9/25

Geometrodynamics (II)

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y ( )

Quantization in Schrödinger picture

Πij(x)

−→

   

i

δ 

δgij(x

)

leads to Wheeler-DeWitt Equation (1962)

− 2Gijkl δ 2

Ψ[g]δgik(x)δg jl(x)

 −√ gR(3)(x)Ψ[g] = 0

for Wave Function(al) of the Universe  Ψ[g].

. – p.9/25

Geometrodynamics (II)

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y

Quantization in Schrödinger picture

Πij(x)

−→

   

i

δ 

δgij(x

)leads to Wheeler-DeWitt Equation (1962)

− 2Gijkl δ 2

Ψ[g]δgik(x)δg jl(x)

 −√ gR(3)(x)Ψ[g] = 0

for Wave Function(al) of the Universe  Ψ[g].

Schrödinger equation of quantum gravity!

‘Timeless’→

contains information ‘from beginning to end’ 

. – p.9/25

Numerous Questions...

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. – p.10/25

Numerous Questions...

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Conceptual and interpretational problems – Physical interpretation of ‘wave function of the universe’ Ψ[g]?

 – Quantum theory in the cosmological context: Copenhagen vs. many worlds?

 – Decoherence and the emergence of a classical (FRW or de Sitter) universe?

 – Origin of time and time arrow?

. – p.10/25

Numerous Questions...

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Conceptual and interpretational problems – Physical interpretation of ‘wave function of the universe’ Ψ[g]?

 – Quantum theory in the cosmological context: Copenhagen vs. many worlds?

 – Decoherence and the emergence of a classical (FRW or de Sitter) universe?

 – Origin of time and time arrow?

Mathematical Challenges – Singular functional differential equation

 – Just the old UV divergences in a new guise? – No Hilbert space of wave functionals?

. – p.10/25

Numerous Questions...

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Conceptual and interpretational problems – Physical interpretation of ‘wave function of the universe’ Ψ[g]?

 – Quantum theory in the cosmological context: Copenhagen vs. many worlds?

 – Decoherence and the emergence of a classical (FRW or de Sitter) universe?

 – Origin of time and time arrow?

Mathematical Challenges – Singular functional differential equation

 – Just the old UV divergences in a new guise? – No Hilbert space of wave functionals?

Very little progress in more than 40 years:

“... that damned equation!”   (Bryce DeWitt)

. – p.10/25

Numerous Questions...

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Conceptual and interpretational problems – Physical interpretation of ‘wave function of the universe’ Ψ[g]?

 – Quantum theory in the cosmological context: Copenhagen vs. many worlds?

 – Decoherence and the emergence of a classical (FRW or de Sitter) universe?

 – Origin of time and time arrow?

Mathematical Challenges – Singular functional differential equation

 – Just the old UV divergences in a new guise? – No Hilbert space of wave functionals?

Very little progress in more than 40 years:

“... that damned equation!”   (Bryce DeWitt)

Recent advances based on ‘change of variables’: – Replace metric variables gij  by (Ashtekar) connection Ai

a

 – Loop Quantum Gravity: holonomies and fluxes as basic variables

 – Space (and time) at the Planck scale: spin network or spin foam?

. – p.10/25

Spin networks and quantum geometry?

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The ‘Superworld’

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The ‘Superworld’

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Basic strategy: render gravity perturbatively consistent(i.e.  finite) via inclusion of suitable matter couplings

. – p.12/25

The ‘Superworld’

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Basic strategy: render gravity perturbatively consistent(i.e.  finite) via inclusion of suitable matter couplings

Supersymmetry: matter (fermions) ↔ forces (bosons)

→ cancellation of UV divergences in perturbation theory

. – p.12/25

The ‘Superworld’

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Basic strategy: render gravity perturbatively consistent(i.e.  finite) via inclusion of suitable matter couplings

Supersymmetry: matter (fermions) ↔ forces (bosons)

→ cancellation of UV divergences in perturbation theoryMaximally symmetric point field theories

D = 4, N  = 8 Supergravity

D = 11 Supergravity

. – p.12/25

The ‘Superworld’

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Basic strategy: render gravity perturbatively consistent(i.e.  finite) via inclusion of suitable matter couplings

Supersymmetry: matter (fermions) ↔ forces (bosons)

→ cancellation of UV divergences in perturbation theoryMaximally symmetric point field theories

D = 4, N  = 8 Supergravity

D = 11 Supergravity

Supersymmetric extended objects

IIA/IIB und heterotic superstrings (D = 10)

Supermembranes and M(atrix)-Theory (D = 11)

No point-like interactions→

no UV singularities?

. – p.12/25

Successes....

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No UV Divergences (so far...) – superstrings: up to and including two loops

 – N=8 supergravity: see below!

 – no results for supermembranes or M(atrix) theory

. – p.13/25

Successes....

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No UV Divergences (so far...) – superstrings: up to and including two loops

 – N=8 supergravity: see below!

 – no results for supermembranes or M(atrix) theory

Gravity is ‘predicted’ by string theory

. – p.13/25

Successes....

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No UV Divergences (so far...) – superstrings: up to and including two loops

 – N=8 supergravity: see below!

 – no results for supermembranes or M(atrix) theory

Gravity is ‘predicted’ by string theory

Semi-realistic spectrum of low energy physics?

. – p.13/25

Successes....

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No UV Divergences (so far...) – superstrings: up to and including two loops

 – N=8 supergravity: see below!

 – no results for supermembranes or M(atrix) theory

Gravity is ‘predicted’ by string theory

Semi-realistic spectrum of low energy physics?

Microscopic BH Entropy:  S  =  14A

. – p.13/25

Successes....

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No UV Divergences (so far...) – superstrings: up to and including two loops

 – N=8 supergravity: see below!

 – no results for supermembranes or M(atrix) theory

Gravity is ‘predicted’ by string theory

Semi-realistic spectrum of low energy physics?

Microscopic BH Entropy:  S  =  14A

New ideas for physics beyond the Standard Model: – Low energy supersymmetry and the MSSM

 – Large extra dimensions and brane worlds – Multi- (or mega-)verses and the ‘string landscape’

. – p.13/25

Successes....

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No UV Divergences (so far...) – superstrings: up to and including two loops

 – N=8 supergravity: see below!

 – no results for supermembranes or M(atrix) theory

Gravity is ‘predicted’ by string theory

Semi-realistic spectrum of low energy physics?

Microscopic BH Entropy:  S  =  14A

New ideas for physics beyond the Standard Model: – Low energy supersymmetry and the MSSM

 – Large extra dimensions and brane worlds – Multi- (or mega-)verses and the ‘string landscape’

If true, a new El Dorado  for experimentalists:new particles, new forces, new dimensions,...

. – p.13/25

An important development

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. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity

. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity... is super-finite  up to four  loops[Bern et al., hep-th/0905.2326]

. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity... is super-finite  up to four  loops[Bern et al., hep-th/0905.2326]

... and might thus be finite to all  orders for D = 4!

. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity... is super-finite  up to four  loops[Bern et al., hep-th/0905.2326]

... and might thus be finite to all  orders for D = 4!

String inspired techniques are crucial for derivation.

. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity... is super-finite  up to four  loops[Bern et al., hep-th/0905.2326]

... and might thus be finite to all  orders for D = 4!

String inspired techniques are crucial for derivation.

New feature: cancellations beyond supersymmetry .

. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity... is super-finite  up to four  loops[Bern et al., hep-th/0905.2326]

... and might thus be finite to all  orders for D = 4!

String inspired techniques are crucial for derivation.

New feature: cancellations beyond supersymmetry .

If true, this could change the picture completely:

. – p.14/25

An important development

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Very recent work has shown that N  = 8 supergravity... is super-finite  up to four  loops[Bern et al., hep-th/0905.2326]

... and might thus be finite to all  orders for D = 4!

String inspired techniques are crucial for derivation.

New feature: cancellations beyond supersymmetry .

If true, this could change the picture completely:

 – A uniquely distinguished UV finite field theory consistently incorporating Einstein gravity?

 – Superstring theory (partly) motivated by expectation that N   = 8 SUGRA is divergent  !

 –  N  = 8 SUGRA has ‘right’ number of fermions (48 = 3 × 16): is this just a curiosity?

. – p.14/25

The esoteric road?

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[with T. Damour, M. Henneaux, A. Kleinschmidt,...]

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The esoteric road?

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[with T. Damour, M. Henneaux, A. Kleinschmidt,...]

Symmetry: the most successful principle of physics

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The esoteric road?

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[with T. Damour, M. Henneaux, A. Kleinschmidt,...]

Symmetry: the most successful principle of physics

Thus: search for a fundamental symmetry of space,time and matter (and quantum gravity)

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The esoteric road?

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[with T. Damour, M. Henneaux, A. Kleinschmidt,...]

Symmetry: the most successful principle of physics

Thus: search for a fundamental symmetry of space,time and matter (and quantum gravity)

A uniquely distinguished symmetry:  E 10 → encodes allknown facts about maximally supersymmetric theories

 – different ‘slicings’ of E 10  yield D  = 11, mIIA, IIB, . . .   supermultiplets

 – field equations as ‘null geodesic motion’ on E 10/K (E 10)

 – expansion in spatial gradients = expansion in heights of E 10  roots

. – p.15/25

The esoteric road?

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[with T. Damour, M. Henneaux, A. Kleinschmidt,...]

Symmetry: the most successful principle of physics

Thus: search for a fundamental symmetry of space,time and matter (and quantum gravity)

A uniquely distinguished symmetry:  E 10 → encodes allknown facts about maximally supersymmetric theories

 – different ‘slicings’ of E 10  yield D  = 11, mIIA, IIB, . . .   supermultiplets

 – field equations as ‘null geodesic motion’ on E 10/K (E 10)

 – expansion in spatial gradients = expansion in heights of E 10  roots

A Lie algebraic mechanism for the ‘de-emergence’ ofspace(-time) at the cosmological singularity? Or: isthere physics ‘before’ (i.e.  ‘without’) space and time?

. – p.15/25

Quantum gravity and experiment?

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Quantum gravity and experiment?

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Any direct  check must contend with smallness ofPlanck scale  →   seems completely hopeless....

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Quantum gravity and experiment?

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Any direct  check must contend with smallness ofPlanck scale  →   seems completely hopeless....

But there may exist indirect checks : is it possible to

link known physics to Planck scale physics, e.g. via– Astrophysics and the early universe? 

– Elementary particle physics? 

. – p.16/25

Quantum gravity and experiment?

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Any direct  check must contend with smallness ofPlanck scale  →   seems completely hopeless....

But there may exist indirect checks : is it possible to

link known physics to Planck scale physics, e.g. via– Astrophysics and the early universe? 

– Elementary particle physics? 

Or do there exist cumulative effects, such as e.g.– Modifi ed dispersion laws for cosmic rays? 

– Unexplained noise in GEO600 detector? 

. – p.16/25

Quantum gravity and experiment?

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Any direct  check must contend with smallness ofPlanck scale  →   seems completely hopeless....

But there may exist indirect checks : is it possible to

link known physics to Planck scale physics, e.g. via– Astrophysics and the early universe? 

– Elementary particle physics? 

Or do there exist cumulative effects, such as e.g.– Modifi ed dispersion laws for cosmic rays? 

– Unexplained noise in GEO600 detector? 

However: without a tight theoretical framework thereare almost unlimited possibilities for such ‘predictions’,and they will not have much discriminatory power.

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Hints from the sky?

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Hints from the sky?

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Or from accelerator experiments?

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Or from accelerator experiments?

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What LHC can tell us

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What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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g g /... and (most probably) not a mini-black-hole factory either!

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What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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... and (most probably) not a mini-black-hole factory either!

Coupling gravity to matter: how mass is generated

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What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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... and (most probably) not a mini-black-hole factory either!

Coupling gravity to matter: how mass is generated

If Higgs is found and mH  measured, many ‘beyondthe standard model’ scenarios will be ruled out! – Example: MSSM type models require mH   < O(130 GeV)

. – p.19/25

What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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... and (most probably) not a mini-black-hole factory either!

Coupling gravity to matter: how mass is generated

If Higgs is found and mH  measured, many ‘beyondthe standard model’ scenarios will be ruled out! – Example: MSSM type models require mH   < O(130 GeV)

Low energy supersymmetry — to be or not to be?

. – p.19/25

What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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... and (most probably) not a mini-black-hole factory either!

Coupling gravity to matter: how mass is generated

If Higgs is found and mH  measured, many ‘beyondthe standard model’ scenarios will be ruled out! – Example: MSSM type models require mH   < O(130 GeV)

Low energy supersymmetry — to be or not to be?

Crucial question: are there new scales between theweak scale and the Planck scale associated with..., substructure (e.g. technicolor), GUTs, supersymmetry, brane worlds,...?

. – p.19/25

What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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... and (most probably) not a mini-black-hole factory either!

Coupling gravity to matter: how mass is generated

If Higgs is found and mH 

 measured, many ‘beyondthe standard model’ scenarios will be ruled out!

 – Example: MSSM type models require mH   < O(130 GeV)

Low energy supersymmetry — to be or not to be?

Crucial question: are there new scales between theweak scale and the Planck scale associated with..., substructure (e.g. technicolor), GUTs, supersymmetry, brane worlds,...?

Or is there a ‘grand desert’: can the standard modelsurvive all the way up to the Planck scale?

. – p.19/25

What LHC can tell us

Not a "big bang machine":  E LHC/M P   = 10−15 !

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... and (most probably) not a mini-black-hole factory either!

Coupling gravity to matter: how mass is generated

If Higgs is found and mH 

 measured, many ‘beyondthe standard model’ scenarios will be ruled out!

 – Example: MSSM type models require mH   < O(130 GeV)

Low energy supersymmetry — to be or not to be?

Crucial question: are there new scales between theweak scale and the Planck scale associated with..., substructure (e.g. technicolor), GUTs, supersymmetry, brane worlds,...?

Or is there a ‘grand desert’: can the standard modelsurvive all the way up to the Planck scale?

→an unobstructed view of Planck scale physics?

. – p.19/25

Prospects (I)

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. – p.20/25

Prospects (I)

E i ti h t diff t t

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Existing approaches stress different aspects:

. – p.20/25

Prospects (I)

E i ti h t diff t t

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Existing approaches stress different aspects:

Background independence and quantum geometry

. – p.20/25

Prospects (I)

Existing approaches stress different aspects

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Existing approaches stress different aspects:

Background independence and quantum geometry

UV finiteness and perturbative consistency

. – p.20/25

Prospects (I)

Existing approaches stress different aspects:

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Existing approaches stress different aspects:

Background independence and quantum geometry

UV finiteness and perturbative consistencyUnification of matter and gravitation

. – p.20/25

Prospects (I)

Existing approaches stress different aspects:

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Existing approaches stress different aspects:

Background independence and quantum geometry

UV finiteness and perturbative consistencyUnification of matter and gravitation

However ...

. – p.20/25

Prospects (I)

Existing approaches stress different aspects:

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Existing approaches stress different aspects:

Background independence and quantum geometry

UV finiteness and perturbative consistencyUnification of matter and gravitation

However ...The hypotheses underlying the different approachesmay not be mutually compatible

 →

. – p.20/25

Prospects (I)

Existing approaches stress different aspects:

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Existing approaches stress different aspects:

Background independence and quantum geometry

UV finiteness and perturbative consistencyUnification of matter and gravitation

However ...The hypotheses underlying the different approachesmay not be mutually compatible

 →‘Grand synthesis’ appears unlikely (at least for now)

. – p.20/25

Prospects (I)

Existing approaches stress different aspects:

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Existing approaches stress different aspects:

Background independence and quantum geometry

UV finiteness and perturbative consistencyUnification of matter and gravitation

However ...The hypotheses underlying the different approachesmay not be mutually compatible

 →‘Grand synthesis’ appears unlikely (at least for now)

To discriminate between numerous different ansätzeand ideas, need to rely more on Occam’s razor!

. – p.20/25

Prospects (II)

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Prospects (II)

Theoretical search has generated many ideas

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Theoretical search has generated many ideas...

. – p.21/25

Prospects (II)

Theoretical search has generated many ideas

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Theoretical search has generated many ideas...... but to arrive at testable predictions and to ‘beat’ thesmallness of the Planck scale we must pin down the

correct theory more or less uniquely −→

. – p.21/25

Prospects (II)

Theoretical search has generated many ideas...

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Theoretical search has generated many ideas...... but to arrive at testable predictions and to ‘beat’ thesmallness of the Planck scale we must pin down the

correct theory more or less uniquely −→The search for the ‘right’ theory is still far from finished!

. – p.21/25

Prospects (II)

Theoretical search has generated many ideas...

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Theoretical search has generated many ideas...... but to arrive at testable predictions and to ‘beat’ thesmallness of the Planck scale we must pin down the

correct theory more or less uniquely −→The search for the ‘right’ theory is still far from finished!

Outside Views:

D. Overbye, String theory, at 20, explains it all (or not)   (New York Times, 7 Dec. 2004);

H. Nicolai, K. Peeters and M. Zamaklar, Class. Quant. Grav.   22 (2005) R193;

M. Rauner, Aus!    (DIE ZEIT, 26 Januar 2006);Tied up with string?    (NATURE, November 2006)

. – p.21/25

Prospects (II)

Theoretical search has generated many ideas...

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eo et ca sea c as ge e ated a y deas... but to arrive at testable predictions and to ‘beat’ thesmallness of the Planck scale we must pin down thecorrect theory more or less uniquely 

−→The search for the ‘right’ theory is still far from finished!

Outside Views:

D. Overbye, String theory, at 20, explains it all (or not)   (New York Times, 7 Dec. 2004);

H. Nicolai, K. Peeters and M. Zamaklar, Class. Quant. Grav.   22 (2005) R193;

M. Rauner, Aus!    (DIE ZEIT, 26 Januar 2006);Tied up with string?    (NATURE, November 2006)

Thank you for your attention

. – p.21/25

... and open problems

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... and open problems

Semi-classical limit and smooth space-time?

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p

ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?

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p

ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?

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p

ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

Quantum space-time covariance?

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?

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ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

Quantum space-time covariance?

Where is the 2-loop divergence?

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?

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ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

Quantum space-time covariance?

Where is the 2-loop divergence?Matter couplings: anything goes?No divergences, no anomalies,...?

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?

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ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

Quantum space-time covariance?

Where is the 2-loop divergence?Matter couplings: anything goes?No divergences, no anomalies,...?

Degeneracy:  > 10500 consistent Hamiltonians?

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?δ δ

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ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

Quantum space-time covariance?

Where is the 2-loop divergence?Matter couplings: anything goes?No divergences, no anomalies,...?

Degeneracy:  > 10500 consistent Hamiltonians?

Idem for spin foam models

. – p.22/25

... and open problems

Semi-classical limit and smooth space-time?δ δ

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ggij(x) ∝   δ 

δAia(x)

 ·   δ 

δA ja(x)

Status of Wheeler-DeWitt equation?

Quantum space-time covariance?

Where is the 2-loop divergence?Matter couplings: anything goes?No divergences, no anomalies,...?

Degeneracy:  > 10500 consistent Hamiltonians?

Idem for spin foam models

Is LQG falsifiable?

. – p.22/25

Simplifications

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. – p.23/25

Simplifications

Semi-classical limit  

→ 0:i

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Ψ[g] ∼ exp

i

 S cl[g]

(1 + O( ))

. – p.23/25

Simplifications

Semi-classical limit  

→ 0:i

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Ψ[g] ∼ exp

i

 S cl[g]

(1 + O( ))

‘Mini-superspace’: only finitely many  d.o.f.’s

gij(t,x

)dx

i

dx

 j

→   a

2

(t)   dr2

1− kr2  + r

2

2

+ r

2

sin

2

θdφ

2⇒ Functional differential equation becomes an‘ordinary’ PDE, that is :   Ψ[g]

 →  ψ(a)

. – p.23/25

New Variables — New Perspectives?

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. – p.24/25

New Variables — New Perspectives?

Replace metric gij

 by connection   [Ashtekar (1986)]

1

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Ama = −1

2abcωmbc + γK m

a

Conjugate variable E am ∝ inverse dreibein (triad)

. – p.24/25

New Variables — New Perspectives?

Replace metric gij

 by connection   [Ashtekar (1986)]

1

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Ama = −1

2abcωmbc + γK m

a

Conjugate variable E am ∝ inverse dreibein (triad)

New canonical brackets

{Ama

(x), Anb

(y)} = {E am

(x), E an

(y)} = 0   ,   {Ama

(x), E bn

(y)} = γδnmδ

ab δ

(3)

(x,y)

. – p.24/25

New Variables — New Perspectives?

Replace metric gij

 by connection   [Ashtekar (1986)]

1 b

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Ama = −1

2abcωmbc + γK m

a

Conjugate variable E am ∝ inverse dreibein (triad)

New canonical brackets

{Ama

(x), Anb

(y)} = {E am

(x), E an

(y)} = 0   ,   {Ama

(x), E bn

(y)} = γδnmδ

ab δ

(3)

(x,y)

γ  = ±i   ⇒ equations become polynomial :

E amF mna(A) ≈ 0   , abcE a

mE bnF mnc(A) ≈ 0

with SU (2) (Yang-Mills) field strength

F mna(A) := ∂ mAna − ∂ nAma + abcAm

b

An

c

. – p.24/25

Loop Quantum Gravity (LQG)

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. – p.25/25

Loop Quantum Gravity (LQG)

New canonical variables: holonomy (along link e)

he[A] = P exp

 A

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he[A] P exp

e

A

. – p.25/25

Loop Quantum Gravity (LQG)

New canonical variables: holonomy (along link e)

he[A] = P exp

 A

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he[A] P exp

e

A

Conjugate variable = flux through area element S 

F aS [E ] :=

 S 

dF a =

 S 

mnpE amdxn ∧ dx p

. – p.25/25

Loop Quantum Gravity (LQG)

New canonical variables: holonomy (along link e)

he[A] = P exp

 A

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e[ ] p

e

Conjugate variable = flux through area element S 

F aS [E ] :=

 S 

dF a =

 S 

mnpE amdxn ∧ dx p

Operators act on cylindrical wave functionals 

Ψ{Γ,C }[A] = f C he1 [A], . . . , hen [A]which ‘probe’ connection not on all of Σ, but on spin network  Γ (= graph consisting of links and vertices).

. – p.25/25