Title: Noise Sensitivity
1Noise 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.)
3Plan 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
4Planar 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.
5Noise 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.
6Noise 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.
7High 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.
8Critical Percolation
9Critical Percolation problems and progress
- The critical probability
- Limit conjectures and Conformal invariance
- SLE and scaling limits
- Noise sensitivity and spectral description
10Kesten 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)
11Limit 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.
12Cardy, 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.) -
13Limits Conjectures and conformal Invariance
14Schramm 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.
15SLE and PercolationGrey/white Interface
16Smirnov 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.)
17Putting 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.)
18Noise 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
19Noise 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.
20Percolation 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.
21Percolation 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!
22Fourier-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.
23Noise 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.
24The 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)
25An 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.
26Dynamic Percolation
27Fourier 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.
28Diversion 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.)
29Noise 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.
30Tsirelson 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.)
31Other 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...
32Questions 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.
33Questions 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
34Are 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.
35Required 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.
37I. 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.
38II...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.)
39III. 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).
40III. 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.
41III. 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.
42Other 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?? ?)
43Conclusion
- 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.
44THANK YOU FOR HAVING ME!????
45Comments 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.
46HU-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.
47HU-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.
48HU-hep seminar participants Comments (continued)
- Ido Ben-Dayan mentioned a work by Malomed and
coauthors on sensitivity to noise of a classic
two beams experiment. - 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.
49HU-hep seminar participants Comments (continued)
- 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.)
50HU-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 !