Universality and RSW for inhomogeneous bond percolation Ioan - - PowerPoint PPT Presentation

universality and rsw for inhomogeneous bond percolation
SMART_READER_LITE
LIVE PREVIEW

Universality and RSW for inhomogeneous bond percolation Ioan - - PowerPoint PPT Presentation

Introduction and models Results The startriangle transformation Use of startriangle transformation Whats next Universality and RSW for inhomogeneous bond percolation Ioan Manolescu joint work with Geoffrey Grimmett Statistical


slide-1
SLIDE 1

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Universality and RSW for inhomogeneous bond percolation

Ioan Manolescu joint work with Geoffrey Grimmett

Statistical Laboratory Department of Pure Mathemetics and Mathematical Statistics University of Cambridge

22 August 2011

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-2
SLIDE 2

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Percolation

An edge e is

  • pen with probability pe

closed with probability 1 − pe

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-3
SLIDE 3

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Percolation

An edge e is

  • pen with probability pe

closed with probability 1 − pe

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-4
SLIDE 4

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Percolation

An edge e is

  • pen with probability pe

closed with probability 1 − pe

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-5
SLIDE 5

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Percolation

An edge e is

  • pen with probability pe

closed with probability 1 − pe

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-6
SLIDE 6

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Percolation

An edge e is

  • pen with probability pe

closed with probability 1 − pe

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-7
SLIDE 7

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Homogeneous Bond Percolation

p p p p p

Z2 T p < pc, a.s. no infinite component; p > pc, a.s. existence of an infinite component. Criticality: pc(Z2) = 1

2.

pc(T) = 2 sin π

18.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-8
SLIDE 8

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Homogeneous Bond Percolation

p p p p p

Z2 T p < pc, a.s. no infinite component; p > pc, a.s. existence of an infinite component. Criticality: pc(Z2) = 1

2.

pc(T) = 2 sin π

18.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-9
SLIDE 9

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Homogeneous Bond Percolation

p p p p p

Z2 T p < pc, a.s. no infinite component; p > pc, a.s. existence of an infinite component. Criticality: pc(Z2) = 1

2.

pc(T) = 2 sin π

18.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-10
SLIDE 10

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Inhomogeneous bond percolation

ph pv p2 p1 p0

Z2 with P

(ph,pv)

T with P△

p

Criticality for Z2: pv + ph = 1. Criticality for T : κ△(p) = p0 + p1 + p2 − p0p1p2 = 1, (p = (p0, p1, p2) ∈ [0, 1)3). Call M the above class of critical (inhomogeneous) models.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-11
SLIDE 11

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Inhomogeneous bond percolation

ph pv p2 p1 p0

Z2 with P

(ph,pv)

T with P△

p

Criticality for Z2: pv + ph = 1. Criticality for T : κ△(p) = p0 + p1 + p2 − p0p1p2 = 1, (p = (p0, p1, p2) ∈ [0, 1)3). Call M the above class of critical (inhomogeneous) models.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-12
SLIDE 12

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Inhomogeneous bond percolation

ph pv p2 p1 p0

Z2 with P

(ph,pv)

T with P△

p

Criticality for Z2: pv + ph = 1. Criticality for T : κ△(p) = p0 + p1 + p2 − p0p1p2 = 1, (p = (p0, p1, p2) ∈ [0, 1)3). Call M the above class of critical (inhomogeneous) models.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-13
SLIDE 13

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Criticality

For P critical we expect:

→ D(Ω, A, B, C, D), as δ → 0 Ω A B C D δ

P where D(Ω, A, B, C, D) is conformally invariant and does not depend on the underlying model. Only known for site percolation on the triangular lattice (Cardy’s formula, Smirnov 2001)

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-14
SLIDE 14

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Criticality

For P critical we expect:

→ D(Ω, A, B, C, D), as δ → 0 Ω A B C D δ

P where D(Ω, A, B, C, D) is conformally invariant and does not depend on the underlying model. Only known for site percolation on the triangular lattice (Cardy’s formula, Smirnov 2001)

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-15
SLIDE 15

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

The box-crossing property

A model satisfies the box-crossing property if for all α there exists c(α) > 0 s.t. for all N:

αN N ∈ [c(α), 1 − c(α)]

P

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-16
SLIDE 16

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

The box-crossing property

A model satisfies the box-crossing property if for all α there exists c(α) > 0 s.t. for all N:

αN N ∈ [c(α), 1 − c(α)]

P The homogeneous models in M satisfy the box-crossing property.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-17
SLIDE 17

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Main result I

Theorem All models in M satisfy the box-crossing property.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-18
SLIDE 18

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Exponents at criticality

O N n

A4(N, n) For a critical percolation measure Ppc, as n → ∞, we expect: volume exponent: Ppc(|C0| = n) ≈ n−1−1/δ, connectivity exponent: Ppc(0 ↔ x) ≈ |x|−η,

  • ne-arm exponent:

Ppc(rad(C0) = n) ≈ n−1−1/ρ, 2j-alternating-arms exponents: Ppc[A2j(N, n)] ≈ n−ρ2j,

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-19
SLIDE 19

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Exponents near ciritcality

Percolation probability: Ppc+ǫ(|C0| = ∞) ≈ ǫβ as ǫ ↓ 0, Correlation length: ξ(pc − ǫ) ≈ ǫ−ν as ǫ ↓ 0, where − 1

n log Ppc−ǫ(rad(C0) ≥ n) →n→∞ 1 ξ(pc−ǫ).

Mean cluster-size: Ppc+ǫ(|C0|; |C0| < ∞) ≈ |ǫ|−γ as ǫ → 0, Gap exponent: for k ≥ 1, as ǫ → 0, Ppc+ǫ(|C0|k+1; |C0| < ∞) Ppc+ǫ(|C0|k; |C0| < ∞) ≈ |ǫ|−∆.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-20
SLIDE 20

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Scaling relations

Kesten ’87. For models with the box-crossing property if ρ or η exist, then ηρ = 2 and 2ρ = δ + 1. Kesten ’87. For models with the box-crossing property rotation and translation invariance, β, ν, γ and δ may be expressed in terms of ρ and ρ4.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-21
SLIDE 21

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Main result II

Theorem If one of the arm exponents exists in one of the models in M, then it exists and is the same in all models in M.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-22
SLIDE 22

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Main result II

Theorem If one of the arm exponents exists in one of the models in M, then it exists and is the same in all models in M. Theorem If ρ or η exist in one of the models in M, then the exponents at criticality (δ, η and ρ) exist and are the same in all models in M.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-23
SLIDE 23

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next The box-crossing property Critical exponents

Main result II

Theorem If one of the arm exponents exists in one of the models in M, then it exists and is the same in all models in M. Theorem If ρ or η exist in one of the models in M, then the exponents at criticality (δ, η and ρ) exist and are the same in all models in M. Theorem If ρ and ρ4 exist in one of the models in M, then the exponents away form criticality exist and are the same in the critical homogeneous models on the square, triangular and hexagonal lattices.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-24
SLIDE 24

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Star–triangle transformation

p0 p1 p2 A B C

O

1−p0 1−p1 1−p2 A B C

Take ω, respectively ω′, according to the measure on the left, respectively right. The families of random variables

  • x

G,ω

← − → y : x, y = A, B, C

  • ,
  • x

G ′,ω′

← − − → y : x, y = A, B, C

  • ,

have the same joint law whenever κ△(p) = p0 + p1 + p2 − p0p1p2 = 1.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-25
SLIDE 25

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Coupling

and similarly for all pairs of edges

(1 − p0)p1p2 P p0p1p2 P p0(1 − p1)p2 P p0p1(1 − p2) P (1 − p0)p1p2 P p0p1p2 P p0(1 − p1)p2 P p0p1(1 − p2) P

and similarly for all single edges T T S S S T

where P = (1 − p0)(1 − p1)(1 − p2).

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-26
SLIDE 26

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Lattice transformation

p0 1 − p0 p1 p2

√ 3 1 Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-27
SLIDE 27

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Lattice transformation

1 − p0

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-28
SLIDE 28

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Lattice transformation

p0 1 − p0 1 − p1 1 − p2 1 − p0

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-29
SLIDE 29

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Lattice transformation

1 − p0

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-30
SLIDE 30

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Lattice transformation

p0 1 − p0 p1 p2 p0 1 − p0

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-31
SLIDE 31

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Lattice transformation

p0 1 − p0 p1 p2 p0 1 − p0

The measure is preserved.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-32
SLIDE 32

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-33
SLIDE 33

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-34
SLIDE 34

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-35
SLIDE 35

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-36
SLIDE 36

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-37
SLIDE 37

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-38
SLIDE 38

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-39
SLIDE 39

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-40
SLIDE 40

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transformation of paths

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-41
SLIDE 41

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transporting box crossings

Proposition For p = (p0, p1, p2) ∈ (0, 1)3 such that κ△(p) = 1, P

(p0,1−p0) satisfies the box-crossing property iff P△ p does.

Use of the proposition: P

1 2, 1 2 satisfies the box-crossing property,

hence so does P△

1 2 ,p0,p′ , when κ△

1

2, p0, p′

  • = 1,

hence so does P

(p0,1−p0), for p0 ∈

  • 0, 1

2

  • ,

hence so does P△

(p0,p1,p2), for κ△ (p0, p1, p2) = 1.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-42
SLIDE 42

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transporting box crossings

Proposition For p = (p0, p1, p2) ∈ (0, 1)3 such that κ△(p) = 1, P

(p0,1−p0) satisfies the box-crossing property iff P△ p does.

Use of the proposition: P

1 2, 1 2 satisfies the box-crossing property,

hence so does P△

1 2 ,p0,p′ , when κ△

1

2, p0, p′

  • = 1,

hence so does P

(p0,1−p0), for p0 ∈

  • 0, 1

2

  • ,

hence so does P△

(p0,p1,p2), for κ△ (p0, p1, p2) = 1.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-43
SLIDE 43

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transporting box crossings

Proposition For p = (p0, p1, p2) ∈ (0, 1)3 such that κ△(p) = 1, P

(p0,1−p0) satisfies the box-crossing property iff P△ p does.

Use of the proposition: P

1 2, 1 2 satisfies the box-crossing property,

hence so does P△

1 2 ,p0,p′ , when κ△

1

2, p0, p′

  • = 1,

hence so does P

(p0,1−p0), for p0 ∈

  • 0, 1

2

  • ,

hence so does P△

(p0,p1,p2), for κ△ (p0, p1, p2) = 1.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-44
SLIDE 44

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transporting box crossings

Proposition For p = (p0, p1, p2) ∈ (0, 1)3 such that κ△(p) = 1, P

(p0,1−p0) satisfies the box-crossing property iff P△ p does.

Use of the proposition: P

1 2, 1 2 satisfies the box-crossing property,

hence so does P△

1 2 ,p0,p′ , when κ△

1

2, p0, p′

  • = 1,

hence so does P

(p0,1−p0), for p0 ∈

  • 0, 1

2

  • ,

hence so does P△

(p0,p1,p2), for κ△ (p0, p1, p2) = 1.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-45
SLIDE 45

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transporting box crossings

Proposition For p = (p0, p1, p2) ∈ (0, 1)3 such that κ△(p) = 1, P

(p0,1−p0) satisfies the box-crossing property iff P△ p does.

Use of the proposition: P

1 2, 1 2 satisfies the box-crossing property,

hence so does P△

1 2 ,p0,p′ , when κ△

1

2, p0, p′

  • = 1,

hence so does P

(p0,1−p0), for p0 ∈

  • 0, 1

2

  • ,

hence so does P△

(p0,p1,p2), for κ△ (p0, p1, p2) = 1.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-46
SLIDE 46

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Transporting arm exponents

Proposition For any k ∈ {1, 2, 4, 6, . . .} and any self-dual triplet p ∈ [0, 1)3 with p0 > 0, there exist c0, c1, n0 > 0 such that, for all n ≥ n0, c0P△

p [Ak(n)] ≤ P (p0,1−p0)[Ak(n)] ≤ c1P△ p [Ak(n)].

Using the same procedure we transport arm exponents between models.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-47
SLIDE 47

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Isoradial graphs

e θe

Each face is inscribed in a circle of radius 1. pe 1 − pe = sin(π−θ(e)

3

) sin(θ(e)

3 )

.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-48
SLIDE 48

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Inhomogeneous models as isoradial graphs

1 2 1 2

pc(T)

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-49
SLIDE 49

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Inhomogeneous models as isoradial graphs

ph pv p0 p1 p2

pv + ph = 1, κ△(p) = p0 + p1 + p2 − p0p1p2 = 1

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-50
SLIDE 50

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Conjectures

Conjecture The class M may be extended to all isoradial graphs.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-51
SLIDE 51

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Conjectures

Conjecture The class M may be extended to all isoradial graphs. Conjecture The class M may be extended to periodic isoradial graphs.

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation

slide-52
SLIDE 52

Introduction and models Results The star–triangle transformation Use of star–triangle transformation What’s next

Thank you!

Ioan Manolescu joint work with Geoffrey Grimmett Universality and RSW for inhomogeneous bond percolation