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Noise Sensitivity

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Title: Noise Sensitivity


1
Noise Sensitivity The case of Percolation
  • Gil Kalai
  • Institute of Mathematics
  • Hebrew University
  • HU HEP seminar, 25 April 2007

2
  • (We start with a one-slide summary of the
    lecture followed by a 4 slides very informal
    summary of its three main ingredients.)

3
Plan of the talk
  • Two dimensional percolation
  • Noise sensitivity The primal description
  • Noise sensitivity - The Fourier description
  • How the spectrum looks like
  • - Scaling limit existence and description
  • Other models with noise sensitivity
  • Questions and thoughts regarding models from
    high-energy physics

4
Planar Percolation
  • The infinite model we have an infinite lattice
    grid
  • in the plane. Every edge (bond) is open with
  • probability p. All these probabilities are
    statistically independent.
  • Basic questions
  • What is the probability of an infinite open
    cluster?
  • What is the probability of an infinite open
    cluster containing the origin?
  • Critical properties of percolation.

5
Noise sensitivity
  • Primal description - Functions (random
    variables) that are extremely sensitive to small
    random changes (which respect the overall
    underlying distribution.) Such functions cannot
    be measured by (even slightly) noisy
    measurements.
  • Dual description Spectrum concentrated on
    large sets
  • Examples Critical percolation, and many others
  • Basic insight Noise sensitivity is common and
    forced in various general situations.

6
Noise stability/Noise sensitivity Dichotomy
  • Familiar stochastic processes are noise stable.
  • Their sensitivity to small amount of noise is
    small.
  • Their spectrum is concentrated on small sets.
  • The notions of noise stability and noise
    sensitivity were introduced by Benjamini, Kalai
    and Schramm. Closely related notions (black
    noise non-Fock models) were introduced by
    Tsirelson and Vershik.

7
High energy physics
  • Are the basic models of high energy physics noise
    stable?
  • If this is indeed the case, does it reflect some
    law of physics or (more likely), will noise
    sensitivity allow additional modeling power.

8
Critical Percolation
9
Critical Percolation problems and progress
  • The critical probability
  • Limit conjectures and Conformal invariance
  • SLE and scaling limits
  • Noise sensitivity and spectral description

10
Kesten Critical probability 1/2
  • Kestens Theorem (1980) The critical probability
    for percolation in the plane is ½.
  • If the probability p for a bond to be open (or
    for a hexagon to be grey) is below ½ the
    probability for an infinite cluster is 0. If the
    probability for a bond to be open is gt ½ then the
    probability for an infinite cluster is 1.
  • (Q And when p is precisely ½?)
  • (A The probability for an infinite cluster is
    0)

11
Limit conjectures
  • Conjecture The probability for the crossing
    event for an n by m rectangular grid tends to a
    limit if the ratio m/n tends to a real number a,
    agt0, as n tends to infinity.
  • (Sounds almost obvious, yet very difficult to
    prove)
  • Note we have moved from infinite models to
    finite ones.

12
Cardy, Aizenman, Langlands Conformal invariance
conjectures
  • Conjecture Crossing events in percolation are
    conformally invariant!!
  • Sounds very surprising. (But there is no case of
    a planar percolation model where the limit
    conjectures are proven and conformal invariance
    is not.)

13
Limits Conjectures and conformal Invariance
14
Schramm SLE
  • Oded Schramm defined a one parameter planar
    stochastic models SLE(?). Lawler, Schramm and
    Werner extensively studied the SLE processes,
    found relations to several planar processes, and
    computed various critical exponents. SLE(6)
    describes the scaling limit of percolation.

15
SLE and PercolationGrey/white Interface
16
Smirnov Conformal Invariance
  • Smirnov proved that for the model of site
    percolation on the triangular grid, equivalently
  • For the white/grey hexagonal model (simply
    HEX), the conformal invariance conjecture is
    correct!
  • (An incredibly simple form of Cardys formulas
    in this case found by Carleson was of
    importance.)

17
Putting things together
  • Combining Smirnov results with the work of Lawler
    Schramm and Werner all critical exponents for
    percolation predicted by physicists and quite a
    few more were computed. (rigorously)
  • (For the model of bond percolation with square
    grid this is yet to be done.)

18
Noise Sensitivity The Primal description
  • We consider a BOOLEAN FUNCTION
  • f -1,1n ? -1,1
  • f(x1 ,x2,...,xn)
  • (For percolation, every hexagon corresponds to a
    variable. xi -1 if the hexagon is white and xi
    1 if it is grey. f1 if there is a left to right
    grey crossing.)
  • Given x1 ,x2,...,xn we define y1 ,y2,...,yn as
    follows
  • xi yi with probability 1-t
  • xi -yi with probability t

19
Noise Sensitivity The Primal description (cont.)
  • Let C(ft) be the correlation between
  • f(x1 , x2,...,xn) and f(y1,y2,...,yn)
  • A sequence of Boolean function (fn ) is
    (completely) noise-sensitive if for every tgt0,
    C(fn,t) tends to zero with n.

20
Percolation is Noise sensitive
  • Theorem BKS The crossing event for critical
    planar percolation model is noise- sensitive
  • Basic argument 1) Fourier description of noise
    sensitivity 2) hypercontractivity
  • This argument applies to very general cases.

21
Percolation is Noise sensitive
  • Imagine two separate pictures of n by n
    hexagonal models for percolation. A hexagon is
    grey with probability ½.
  • If the grey and white hexagons are independent in
    the two pictures the probability for crossing in
    both is ¼.
  • If for each hexagon the correlation between its
    colors in the two pictures is 0.99, still the
    probability for crossing in both pictures is very
    close to ¼ as n grows! If you put one drawing on
    top of the other you will hardly notice a
    difference!

22
Fourier-Walsh expansion
  • Given a Boolean function f -1,1n ? -1,1, we
    write f(x) as a sum of multilinear (square free)
    monomials.
  • f(x) Sfˆ(S)W(S), where W(S) ?xs s ? S.
  • f(S) is the Fourier-Walsh coefficient
    corresponding to S.
  • Used by Kahn, Kalai and Linial (1988) to settle a
    conjecture by Ben-Or and Linial on influences.

23
Noise sensitivity the dual Description
  • The spectral distribution of f is a probability
    distribution assigning to a subset S the
    probability (f(S))2
  • For a sequence of Boolean function
  • fn -1,1n ? -1,1
  • (fn) is (completely) noise sensitive if for every
    k the overall spectral probability for non empty
    sets of size at most k tends to 0 as n tends to
    0.

24
The motivations
  • This was an attempt towards limits and
    conformal invariance conjectures. (Second attempt
    for Oded and Itai.)
  • Understanding the spectrum of percolation
    looked interesting One critical exponent
    (correlation length) has a simple description.
  • (Late) Percolation on certain random planar
    graphs arise here naturally. (KPZ)

25
An application Dynamic percolation
  • Dynamic percolation was introduced and first
    studied by Häggström, Peres and Steif (1997).
    The model was introduced independently by Itai
    Benjamini. Häggström, Peres and Steif proved that
    above the critical probability we have infinite
    clusters at all times, and below the critical
    probability there are infinite clusters at no
    times.
  • Schramm and Steif proved that for dynamic
    percolation on the HEX model there are
    exceptional times. The proof is based on their
    strong versions of noise sensitivity for planar
    percolation.

26
Dynamic Percolation
27
Fourier Description of Crossing events of
Percolation
  • Benjamini, Kalai, and Schramm Most Fourier
    Coefficients are above log n
  • Schramm and Steif Most Fourier coefficients are
    above nb (bgt0)
  • Schramm and Smirnov Scaling limit for spectral
    distribution for Percolation exists ()
  • Garban, Pete and Schramm (yet unwritten)
    Spectral distributions concentrated on sets of
    size n3/4(1o(1)). ()
  • () proved only for models where Smirnovs
    result apply.
  • In summary Scaling limit for the spectral
    distribution of percolation is described by
    Cantor sets of dimension ¾.

28
Diversion Simulating and computing the spectrum
for percolation
  • Can we sample according (approximately) to the
    spectral distribution of the crossing event of
    percolation?
  • This is unknown and it might be hard on digital
    computers.
  • But... it is known to be easy for... quantum
    computers. For every Boolean function where f is
    computable in polynomial time. (Quantum computers
    are hypothetical devices based on QM which allow
    superior computational power.)

29
Noise sensitivity, and non-classical stochastic
processes black noise
  • Closly related notions to noise sensitivity
    were studied by Tsirelson and Vershik . In their
    terminology noise sensitivity translates to
    non Fock processes, black noise, and
    non-classical stochastic processes. Their
    motivation is closer to mathematical quantum
    physics.

30
Tsirelson and Vershik Non Fock spaces black
noise non classical stochastic processes (cont)
  • The terminology is confusing but here is the
    dictionary
  • Noise stable White noise classical stochastic
    process Fock model
  • Noise sensitive Black noise non classical
    stochastic process non-Fock model.
  • Tsirelson and Vershik pointed out a connection
    between noise sensitivity and non-linearity.
    (Well within the realm of QM.)

31
Other cases of noise sensitivity
  • First Passage Percolation (Benjamini, Kalai,
    Schramm)
  • A recursive example by Ben-Or and Linial
  • Eigenvalues of random Gaussian matrices
    (Essentially follows from the work of
    Tracy-Widom) Here, we leave the Boolean setting.
  • Examples related to random walks (required
    replacing the discrete cube by trees) and more...

32
Questions about HEP models
  • Are current HEP models noise stable?
  • Or perhaps there is some internal inconsistency
    about their noise stability
  • The naive idea is this Hep models describe a
    (quantum) stochastic state. Is this state
    necessarily noise stable?
  • (Less naively, according to Tsirelson) Noise
    sensitivity means that the very idea of the
    field operator at a point' (on the level of
    operator-valued Schwartz distributions (or
    something like that)) will fail.

33
Questions about HEP models
  • Tsireslon constructed a toy non-Fock model in
    hep-th/9912031
  • My thoughts on the matter can be found in
  • hep-th/0703092

34
Are basic models from High energy physics noise
stable?
  • Remark In order to properly ask the question we
    need to extend the notion of noise sensitivity
  • Quantum probabilities
  • Symmetries are not Z/2Z but other fixed groups
    like U(1), SU(2) and SU(3).
  • Noise sensitivity assumes a representation via
    independent random variables.

35
Required extensions for Noise sensitivity
  • Quantum probabilities This appears not to pose
    difficulties. Was studied by Tsirelson.
  • 2) Symmetries are not Z/2Z but other fixed groups
    like U(1), SU(2) and SU(3). The notions of noise
    sensitivity extends. Interesting new phenomena
    occurred even when moving from Z/2Z to to Z/3Z
    and more are expected in the non-Abelian case.
  • 3) Noise sensitivity assumes a representation via
    independent random variables. This is the most
    serious and interesting concern.

36
  • The next few slides consider some critical
    comments concerning the relevance and novelty of
    noise-sensitive models.

37
I. Does noise sensitivity just reflects wrong
scaling?
  • Perhaps, in some cases. (And if it does it may
    give an interesting mathematical setting for such
    scaling problems/renormalization.) It is known
    that for Boolean functions at the wrong scale
    noise sensitivity is forced.
  • However, in some cases, like the case of
    percolation, noise sensitivity occurs at all
    scales.

38
II...But Percolation is a model arising in CFT
  • The percolation model is a very basic example in
    CFT (conformal field theory). Since noise
    sensitivity occurs in a rather special case of a
    very familiar physics model, isnt it just an
    artifact of the way we look here at
    percolation?
  • Maybe. But it does not seem to be the case.
  • (Perhaps the non-rigorous physics theories treat
    noise sensitive processes as being noise stable.)

39
III. Do strings already capture the idea of noise
sensitivity?
  • (and also QCD(N) and other familiar models...)
  • The conjecture that Hep-model are describing
    noise stable processes is also based on the
    description of point particles and their (mainly)
    pair-wise interactions. We think about particles
    as living in the spectrum world.
  • Isnt noise sensitivity just a very primitive
    version of ideas that come to play in various
    current models from physics (which are really
    relevant to physics).

40
III. Is the spectral distribution for percolation
something like strings? (cont.)
  • (and also QCD(N) and other familiar models...)
  • Isnt noise sensitivity a very primitive version
    of ideas that come to play in various current
    models from physics (which are really relevant to
    physics)? Do strings already capture the idea of
    noise-sensitivity?
  • Well, if indeed the scaling limit for the
    spectrum of percolation is a rigorous
    mathematical model of something like strings
    this can be of interest.

41
III. Do strings capture the idea of noise
sensitivity (cont.) ?
  • Yes, maybe, but there are things that look quite
    different
  • A) The geometry of the scaling limit object for
    percolation is not that of a string the scaling
    limits are Cantor sets.
  • (It is an interesting problem to find a case of a
    noise sensitive process (black noise) with
    connected spectral scaling limit.)
  • B) For the case of percolation the spectral
    objects themselves appear to represent
    non-classical stochastic objects. (unlike strings
    which themselves looks as classical stochastic
    objects)
  • C) The mathematical framework for strings still
    looks (in part) as assuming some sort of
    noise-stability.

42
Other physics speculations
  • Black Noise/Noise sensitivity occurred at the
    Big Bang (Tsirelson and Vershik) this was a
    motivating idea behind their paper but it is
    not mentioned there.
  • Dark Energy is a black noise (noise-sensitive
    process).
  • Noise sensitivity models may allow string or
    string-like models in D31.
  • (And what about black holes?? ?)

43
Conclusion
  • If noise sensitivity is an option, noise
    sensitive models may allow modeling power beyond
    those of existing models.
  • If noise stability is a law of physics this is
    also interesting.
  • Noise sensitivity (and our notions of pixelwise
    Fourier expansions) may be relevant to
    mathematical foundations of current successful
    models from high energy physics (QED, QCD).
  • Noise sensitive (black) perturbations of other
    PDE from physics and related notions of
    generalized solutions, can also be of interest.

44
THANK YOU FOR HAVING ME!????
45
Comments by HU-HEP seminar participants
  • 1. (Major, rather justified critique.) Jumping
    from the model of percolation to hep-ph models
    was not justified. I was not specific about what
    is it precisely that I suspect to be noise
    sensitive. Also the analogy made in the lecture
    between the Z/2Z symmetry in the percolation
    model and symmetries in hep models may be by
    name only.

46
HU-hep seminar participants Comments (continued)
  • 2. Shmuel Elitzur asked if we can do something
    similar for the Ising model. In sort of defense
    against the previous critique he pointed out
    that, in some sense, general field theories can
    be built up from copies of the Ising model.

47
HU-hep seminar participants Comments (continued)
  • 3. There was a long discussion if (and how) noise
    sensitivity can be tested experimentally. (Not
    just by simulations.) Initially I thought the
    answer is negative but was convinced by the
    others otherwise.

48
HU-hep seminar participants Comments (continued)
  1. Ido Ben-Dayan mentioned a work by Malomed and
    coauthors on sensitivity to noise of a classic
    two beams experiment.
  2. Merav Stern commented that these notions are more
    suitable to condensed matter physics and
    speculated/suggested to think about
    noise-sensitive models in connection with high
    temperature superconductivity.

49
HU-hep seminar participants Comments (continued)
  1. Matteo Cardella asked about noise sensitivity of
    the actual paths exhibiting the crossing events
    in percolation. So, in the two pictures with 0.99
    correlation is it true that even if there is
    crossing in both pictures, the paths exhibiting
    the crossing are in some sense uncorrelated.
    (Oded Schramm pointed out that indeed this is the
    case.)

50
HU-hep seminar participants Comments (continued)
  • 7. Shmuel Elitzur summarized the lectures
    massage in a very sweet way In addition to
    classical part which is described by current
    HEP models the lecture proposes that there is
    another component which represents a different
    kind of stochastic behavior.

51
  • More remarks are welcomed !
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