Gravity and the cosmological constant as superconducting phenomena - - PowerPoint PPT Presentation

gravity and the cosmological constant as superconducting
SMART_READER_LITE
LIVE PREVIEW

Gravity and the cosmological constant as superconducting phenomena - - PowerPoint PPT Presentation

Gravity and the cosmological constant as superconducting phenomena Gianluca Calcagni August 28th, 2008 Based on S. Alexander, G.C., Superconducting loop quantum gravity 1 and the cosmological constant [ 0806.4382 ]. S. Alexander, G.C., Quantum


slide-1
SLIDE 1

Gravity and the cosmological constant as superconducting phenomena

Gianluca Calcagni August 28th, 2008

slide-2
SLIDE 2

Based on

1

  • S. Alexander, G.C., Superconducting loop quantum gravity

and the cosmological constant [0806.4382].

2

  • S. Alexander, G.C., Quantum gravity as a Fermi liquid

[0807.0225].

slide-3
SLIDE 3

Aims of the talk

slide-4
SLIDE 4

Aims of the talk

To throw a rock.

slide-5
SLIDE 5

Aims of the talk

To throw a rock. Not to hide the hand.

slide-6
SLIDE 6

The rock

slide-7
SLIDE 7

The rock

Setup: Loop quantum gravity with Λ, no matter, and the Chern–Simons state as ground state.

slide-8
SLIDE 8

The rock

Setup: Loop quantum gravity with Λ, no matter, and the Chern–Simons state as ground state. Assumption: Deform the topological sector (then Λ becomes dynamical).

slide-9
SLIDE 9

The rock

Setup: Loop quantum gravity with Λ, no matter, and the Chern–Simons state as ground state. Assumption: Deform the topological sector (then Λ becomes dynamical). Result 1: spacetime degenerate (1 + 1 dimensions), Hamiltonian modified by a quantum counterterm.

slide-10
SLIDE 10

The rock

Setup: Loop quantum gravity with Λ, no matter, and the Chern–Simons state as ground state. Assumption: Deform the topological sector (then Λ becomes dynamical). Result 1: spacetime degenerate (1 + 1 dimensions), Hamiltonian modified by a quantum counterterm. Result 2: Gravity behaves as a Fermi liquid, in particular BCS.

slide-11
SLIDE 11

BCS theory

slide-12
SLIDE 12

BCS theory

Bardeen, Cooper, and Schrieffer, Phys. Rev. 108, 1175 (1957).

slide-13
SLIDE 13

BCS theory

Bardeen, Cooper, and Schrieffer, Phys. Rev. 108, 1175 (1957). Nobel Prize in 1972 (Bardeen’s second!).

slide-14
SLIDE 14

BCS theory

Bardeen, Cooper, and Schrieffer, Phys. Rev. 108, 1175 (1957). Nobel Prize in 1972 (Bardeen’s second!).

Nonperturbative vacuum CONDENSATION FERMI SURFACE Fermi−Dirac statistics Bose−Einstein statistics Occupation Number n(k) 1 Fermionic Momentum k Perturbative vacuum

slide-15
SLIDE 15

BCS theory

Bardeen, Cooper, and Schrieffer, Phys. Rev. 108, 1175 (1957). Nobel Prize in 1972 (Bardeen’s second!).

Nonperturbative vacuum CONDENSATION FERMI SURFACE Fermi−Dirac statistics Bose−Einstein statistics Occupation Number n(k) 1 Fermionic Momentum k Perturbative vacuum

1958-1971: 1 Nobel Prize for studies on condensed matter (Landau).

slide-16
SLIDE 16

BCS theory

Bardeen, Cooper, and Schrieffer, Phys. Rev. 108, 1175 (1957). Nobel Prize in 1972 (Bardeen’s second!).

Nonperturbative vacuum CONDENSATION FERMI SURFACE Fermi−Dirac statistics Bose−Einstein statistics Occupation Number n(k) 1 Fermionic Momentum k Perturbative vacuum

1958-1971: 1 Nobel Prize for studies on condensed matter (Landau). 1973-2007: 10 Prizes awarded in this field.

slide-17
SLIDE 17

The ripples (to be explored)

slide-18
SLIDE 18

The ripples (to be explored)

1

Λ is exponentially suppressed, nonperturbative phenomenon; at small scales gravity is perturbative, like in QCD confinement.

slide-19
SLIDE 19

The ripples (to be explored)

1

Λ is exponentially suppressed, nonperturbative phenomenon; at small scales gravity is perturbative, like in QCD confinement.

2

Geometrical measurements amount to counting Cooper pairs.

slide-20
SLIDE 20

The ripples (to be explored)

1

Λ is exponentially suppressed, nonperturbative phenomenon; at small scales gravity is perturbative, like in QCD confinement.

2

Geometrical measurements amount to counting Cooper pairs.

3

Classically, Cooper pairs are microscopic nonlocal d.o.f. living on the dS boundary (wormholes).

slide-21
SLIDE 21

The ripples (to be explored)

1

Λ is exponentially suppressed, nonperturbative phenomenon; at small scales gravity is perturbative, like in QCD confinement.

2

Geometrical measurements amount to counting Cooper pairs.

3

Classically, Cooper pairs are microscopic nonlocal d.o.f. living on the dS boundary (wormholes).

4

Four dimensions recovered by the spin network defined by the superfluid theory.

slide-22
SLIDE 22

The ripples (to be explored)

1

Λ is exponentially suppressed, nonperturbative phenomenon; at small scales gravity is perturbative, like in QCD confinement.

2

Geometrical measurements amount to counting Cooper pairs.

3

Classically, Cooper pairs are microscopic nonlocal d.o.f. living on the dS boundary (wormholes).

4

Four dimensions recovered by the spin network defined by the superfluid theory.

5

Matter is ‘hidden’ in gravity?

slide-23
SLIDE 23

Nonlocal degrees of freedom on dS horizons

slide-24
SLIDE 24

The hand: 1. Loop quantum gravity

slide-25
SLIDE 25

The hand: 1. Loop quantum gravity

Ashtekar variables: connection C-field A ≡ Ai

ατidxα and

real triad Ei

α.

slide-26
SLIDE 26

The hand: 1. Loop quantum gravity

Ashtekar variables: connection C-field A ≡ Ai

ατidxα and

real triad Ei

α.

Scalar, vector, and Gauss constraints: H = ǫijkEi · Ej ×

  • Bk + Λ

3 Ek

  • = 0,

Vα = (Ei × Bi)α = 0 , Gi = DαEα

i = 0.

slide-27
SLIDE 27

The hand: 1. Loop quantum gravity

Ashtekar variables: connection C-field A ≡ Ai

ατidxα and

real triad Ei

α.

Scalar, vector, and Gauss constraints: H = ǫijkEi · Ej ×

  • Bk + Λ

3 Ek

  • = 0,

Vα = (Ei × Bi)α = 0 , Gi = DαEα

i = 0.

Quantum theory: E → ˆ Eα

i = −δ/δAi α, ˆ

Ai

α multiplicative.

slide-28
SLIDE 28

The hand: 1. Loop quantum gravity

Ashtekar variables: connection C-field A ≡ Ai

ατidxα and

real triad Ei

α.

Scalar, vector, and Gauss constraints: H = ǫijkEi · Ej ×

  • Bk + Λ

3 Ek

  • = 0,

Vα = (Ei × Bi)α = 0 , Gi = DαEα

i = 0.

Quantum theory: E → ˆ Eα

i = −δ/δAi α, ˆ

Ai

α multiplicative.

Constraints annihilated by the Chern–Simons state ΨCS = exp iθ 8π2

  • S3 tr(A ∧ dA + 2

3A ∧ A ∧ A)

  • ,

θ ≡ 6π2 iΛ ,

slide-29
SLIDE 29

The hand: 1. Loop quantum gravity

Ashtekar variables: connection C-field A ≡ Ai

ατidxα and

real triad Ei

α.

Scalar, vector, and Gauss constraints: H = ǫijkEi · Ej ×

  • Bk + Λ

3 Ek

  • = 0,

Vα = (Ei × Bi)α = 0 , Gi = DαEα

i = 0.

Quantum theory: E → ˆ Eα

i = −δ/δAi α, ˆ

Ai

α multiplicative.

Constraints annihilated by the Chern–Simons state ΨCS = exp iθ 8π2

  • S3 tr(A ∧ dA + 2

3A ∧ A ∧ A)

  • ,

θ ≡ 6π2 iΛ , Different sectors of Euclidean gravity (θ → iθ) connected by large gauge transformations.

slide-30
SLIDE 30

The hand: 2. Deformation of θ

slide-31
SLIDE 31

The hand: 2. Deformation of θ

We deform the topological sector as θ → θ(A),

slide-32
SLIDE 32

The hand: 2. Deformation of θ

We deform the topological sector as θ → θ(A), thus breaking large-gauge U(1) invariance (analogy with Peccei–Quinn invariance in QCD).

slide-33
SLIDE 33

The hand: 2. Deformation of θ

We deform the topological sector as θ → θ(A), thus breaking large-gauge U(1) invariance (analogy with Peccei–Quinn invariance in QCD). Λ is promoted to an evolving functional Λ(A).

slide-34
SLIDE 34

The hand: 2. Deformation of θ

We deform the topological sector as θ → θ(A), thus breaking large-gauge U(1) invariance (analogy with Peccei–Quinn invariance in QCD). Λ is promoted to an evolving functional Λ(A). No matter introduced by hand!

slide-35
SLIDE 35

The hand: 2. Deformation of θ

We deform the topological sector as θ → θ(A), thus breaking large-gauge U(1) invariance (analogy with Peccei–Quinn invariance in QCD). Λ is promoted to an evolving functional Λ(A). No matter introduced by hand! The only sectors compatible with this step and the Gauss constraint are degenerate: det E = 0, no metric!

slide-36
SLIDE 36

The hand: 3. Jacobson sector (rk E = 1)

slide-37
SLIDE 37

The hand: 3. Jacobson sector (rk E = 1)

E.o.m. for A can be written as the (1 + 1)-dimensional Dirac equation γ0 ˙ ψ + γz∂zψ = 0

slide-38
SLIDE 38

The hand: 3. Jacobson sector (rk E = 1)

E.o.m. for A can be written as the (1 + 1)-dimensional Dirac equation γ0 ˙ ψ + γz∂zψ = 0, where ψ ≡     iA1

1

A1

2

A2

1

iA2

2

    .

slide-39
SLIDE 39

The hand: 3. Jacobson sector (rk E = 1)

E.o.m. for A can be written as the (1 + 1)-dimensional Dirac equation γ0 ˙ ψ + γz∂zψ = 0, where ψ ≡     iA1

1

A1

2

A2

1

iA2

2

    .

E V E E

slide-40
SLIDE 40

The hand: 3. Jacobson sector (rk E = 1)

E.o.m. for A can be written as the (1 + 1)-dimensional Dirac equation γ0 ˙ ψ + γz∂zψ = 0, where ψ ≡     iA1

1

A1

2

A2

1

iA2

2

    .

E V E E

A model for V interactions and physical interpretation naturally emerge at quantum level.

slide-41
SLIDE 41

The hand: 4. Suppression of Λ

slide-42
SLIDE 42

The hand: 4. Suppression of Λ

A quantum counterterm in H modifies the e.o.m. for A as γ0 ˙ ψ + γz∂zψ + imψ = 0.

slide-43
SLIDE 43

The hand: 4. Suppression of Λ

A quantum counterterm in H modifies the e.o.m. for A as γ0 ˙ ψ + γz∂zψ + imψ = 0. Mass term m = −2i ¯ ψγ5∂zψ.

slide-44
SLIDE 44

The hand: 4. Suppression of Λ

A quantum counterterm in H modifies the e.o.m. for A as γ0 ˙ ψ + γz∂zψ + imψ = 0. Mass term m = −2i ¯ ψγ5∂zψ. The simplest nonperturbative solution requires Λ = Λ0 exp(− ¯ ψγ5γzψ)

slide-45
SLIDE 45

The hand: 4. Suppression of Λ

A quantum counterterm in H modifies the e.o.m. for A as γ0 ˙ ψ + γz∂zψ + imψ = 0. Mass term m = −2i ¯ ψγ5∂zψ. The simplest nonperturbative solution requires Λ = Λ0 exp(− ¯ ψγ5γzψ) j5α associated with a chiral transformation of the fermion ψ and not conserved in the presence of m.

slide-46
SLIDE 46

The hand: 4. Suppression of Λ

A quantum counterterm in H modifies the e.o.m. for A as γ0 ˙ ψ + γz∂zψ + imψ = 0. Mass term m = −2i ¯ ψγ5∂zψ. The simplest nonperturbative solution requires Λ = Λ0 exp(− ¯ ψγ5γzψ) j5α associated with a chiral transformation of the fermion ψ and not conserved in the presence of m. P symmetry is broken.

slide-47
SLIDE 47
  • 5. The hand opens
slide-48
SLIDE 48
  • 5. The hand opens

Perturbative regime

slide-49
SLIDE 49
  • 5. The hand opens

Perturbative regime (small values of the connection)

slide-50
SLIDE 50
  • 5. The hand opens

Perturbative regime (small values of the connection): |j5z| ≪ 1, Λ ≈ Λ0(1 − j5z) = O(1).

slide-51
SLIDE 51
  • 5. The hand opens

Perturbative regime (small values of the connection): |j5z| ≪ 1, Λ ≈ Λ0(1 − j5z) = O(1). Nonperturbative regime

slide-52
SLIDE 52
  • 5. The hand opens

Perturbative regime (small values of the connection): |j5z| ≪ 1, Λ ≈ Λ0(1 − j5z) = O(1). Nonperturbative regime (large connection values)

slide-53
SLIDE 53
  • 5. The hand opens

Perturbative regime (small values of the connection): |j5z| ≪ 1, Λ ≈ Λ0(1 − j5z) = O(1). Nonperturbative regime (large connection values): Condensate with v.e.v. j5z ∼ O(102).

slide-54
SLIDE 54
  • 5. The hand opens

Perturbative regime (small values of the connection): |j5z| ≪ 1, Λ ≈ Λ0(1 − j5z) = O(1). Nonperturbative regime (large connection values): Condensate with v.e.v. j5z ∼ O(102). Smallness of Λ regarded as a large-scale nonperturbative quantum mechanism similar to quark confinement.

slide-55
SLIDE 55
  • 5. The hand opens

Perturbative regime (small values of the connection): |j5z| ≪ 1, Λ ≈ Λ0(1 − j5z) = O(1). Nonperturbative regime (large connection values): Condensate with v.e.v. j5z ∼ O(102). Smallness of Λ regarded as a large-scale nonperturbative quantum mechanism similar to quark confinement. Quantizing ψ as a Majorana fermion, H ∝ HBCS =

  • k,σ

Ekc†

kσckσ −

  • k,k′

Vkk′c†

k+c† k−ck′−ck′+.

Correspondence made rigorous using a deformed CFT (WZW model at critical level).