Monday, May 22 |
07:30 - 09:00 |
Breakfast (Restaurant Hotel Hacienda Los Laureles) |
08:45 - 09:00 |
Introduction and Welcome (Conference Room San Felipe) |
09:00 - 09:30 |
Rodrigo Bañuelos: A Doob h-process and singular integrals on lattice Z^d ↓ In 1979 R. F. Gundy and N. Th. Varopoulos published a beautiful 3-page paper titled "Les
transformations de Riesz et les integrales stochastiques" in which they gave a representation
for the classical Riesz transforms on Rd as conditional expectations of stochastic integrals.
During the last 40+ years, in combination with sharp martingale inequalities, this simple and
elegant representation has had a phenomenal success in obtaining optimal, or near optimal,
Lp bounds for Riesz transforms and more general singular integrals and Fourier multipliers
in a variety of geometric and analytic settings. An important feature of these bounds is their
independence on the geometry of the ambient space.
In this talk the speaker will discuss a modi cation of this construction which leads to sharp
estimates for discrete singular integrals on the lattice Zd,d≥1, and in particular to the
identification of the ℓpEnormofthediscreteHilberttransformontheintegersZ$. The latter had
been a long-standing conjecture initiated in part by an erroneous proof of E. C. Titchmarsh
in 1926.
Based on work with Mateusz Kwasnicki ofWroc law University, Poland (2019), and Daesung
Kim, Georgia Tech & Mateusz Kwasnicki (2022). (Hotel Hacienda Los Laureles) |
09:35 - 10:05 |
Davar Khoshnevisan: On the valleys of the stochastic heat equation ↓ We consider a generalization of the parabolic Anderson model driven by space-time white noise, also called the stochastic
heat equation, on the real line. High peaks of solutions have been extensively studied under the name of intermittency, but less is known
about spatial regions between peaks, which may loosely refer to as valleys. We present two results about the valleys of the solution.
Our first theorem provides information about the size of valleys and the supremum of the solution over a valley. More precisely, we show
that the supremum of the solution over a valley vanishes as the time variable tends to infiniry, and we establish an upper bound of
exp(-const. t^{1/3}) for the rate of decay. We demonstrate also that the length of a valley grows at least as exp(+const. t^{1/3}) as t gets large.
Our second theorem asserts that the length of the valleys are eventually infinite when the initial data has subgaussian tails.
This is based on joint work with Kunwoo Kim (POSTECH) and Carl Mueller (Rochester). (Online) |
10:05 - 11:00 |
Coffee Break (Conference Room San Felipe) |
11:00 - 11:30 |
Céline Lacaux: Fractional Gaussian and Stable randoms fields on fractals ↓ In this talk, we adopt the viewpoint about fractional fields which is given in Lodhia and al. Fractional Gaussian fields: a survey,
Probab. Surv., 2016. As example, we focus on random fields defined on the Sierpiński gasket but random fields defined on
fractional metric spaces can also be considered. Hence, for s≥0, we consider the random measure X=(−Δ)−sW
where Δ is a Laplacian on the Sierpiński gasket K equipped with its Hausdorff measure μ and where W is a
Gaussian random measure with intensity μ. For a range of values of the parameter s, the random measure X admits a Gaussian
random field (X(x))x∈K as density with respect to μ. Moreover, using entropy method, an upper bound of the
modulus of continuity of (X(x))x∈K is obtained, which leads to the existence of a modification with Hölder sample paths.
In addition, the fractional Gaussian random field X is invariant by the symmetries of the gasket.
If time allows, some extension to α-stable random fields will also be presented.
This is a joint work with Fabrice Baudoin (University of Connecticut). (Hotel Hacienda Los Laureles) |
11:35 - 12:05 |
William Salkeld (Hotel Hacienda Los Laureles) |
12:05 - 13:20 |
Lunch (Hotel Hacienda Los Laureles) |
13:20 - 13:30 |
Group Photo (Hotel Hacienda Los Laureles) |
13:30 - 14:00 |
Break (Hotel Hacienda Los Laureles) |
14:00 - 14:30 |
Carl Mueller: The radius of star polymers in low dimensions and for small time ↓ Joint with Eyal Neuman. Studying the end-to-end distance of a self-avoiding or weakly self-avoiding
random walk in two dimensions is a well known hard problem in probability and
statistical physics. The conjecture is that the average end-to-end distance
up to time n should be about n3/4.
It would seem that studying more complicated models would be even harder,
but we are able to make progress in one such model. A star polymer is a
collection of N weakly mutually-avoiding Brownian motions taking values in
Rd and starting at the origin. We study the two and three
dimensional cases, and our sharpest results are for d=2. Instead of the
end-to-end distance, we define a radius RT which measures the spread of
the entire configuration up to time T. There are two phases: a crowded
phase for small values for T, and a sparser phase for large T where
paths do not interfere much. Our main result states for $T (Online) |
14:35 - 15:05 |
Raluca Balan: Hyperbolic Anderson model with time-independent rough noise: Gaussian fluctuations ↓ In this talk, we introduce the hyperbolic Anderson model in dimension 1, driven by a time-independent rough noise, i.e. the noise associated with the fractional Brownian motion of Hurst index H∈(1/4,1/2). The goal of the talk will be to show that, with appropriate normalization and centering, the spatial integral of the solution converges in distribution to the standard normal distribution, and to estimate the speed of this convergence in the total variation distance. For this, we use some recent developments related to the Stein-Malliavin method. More precisely, we use a version of the second-order Gaussian Poincar\'e inequality developed by Nualart, Xia, Zheng (2022) for the similar problem for the parabolic Anderson model with rough noise in space (colored in time). To apply this method, we need to derive first some moment estimates for the increments of the first and second Malliavin derivatives of the solution. These are obtained using a connection with the wave equation with delta initial velocity, a method which is different than the one used in the parabolic case.
This talk is based on joint work with Wangjun Yuan (University of Luxembourg). (Hotel Hacienda Los Laureles) |
15:05 - 15:30 |
Coffee Break (Conference Room San Felipe) |
15:30 - 16:00 |
Eulalia Nualart: Everywhere and instantaneous blowup of parabolic SPDEs ↓ We consider the non-linear stochastic heat equation defined on the whole line driven by a space time white noise. We will first recall some known results on the almost sure blow up for this type of equations. We then give sufficient conditions for the solution to blow up everywhere and instantaneously almost surely. The main ingredient of the proof is the study of the spatial growth of stochastic convolutions using techniques from Malliavin calculus and Poincare inequalities .
This is a joint work with Davar Khoshnevisan and Mohammud Foondun. (Hotel Hacienda Los Laureles) |
16:05 - 16:35 |
Hakima Bessaih: Synchronization of stochastic models with applications. ↓ In the first part of the talk, we consider a system of two coupled stochastic lattice equations driven by additive white noise processes. Our objective is to investigate its longtime behavior. A system synchronizes if all elements eventually exhibit the same behavior. We show a synchronization for this system. To describe this phenomenon, we prove the upper semi continuity of the family of attractors with respect to the attractor of a specific limiting stochastic system.
In the second part of the talk, we investigate a complex network consisting of finitely many nodes that are coupled in a deterministic and stochastic way. The behavior of each node is described by an evolution equation that includes a reaction diffusion equation driven by a multiplicative noise. We prove that the system synchronizes towards a deterministic equation. Furthermore, we describe various concepts of synchronization (Online) |
16:40 - 17:10 |
Frederi Viens: Yule’s nonsense correlation: Wiener chaos analysis towards asymptotics and testing ↓ The empirical correlation ρn, defined for two related sequences of data of
length n, is defined classically via Pearson’s correlation statistic. When the data is
i.i.d. with two moments, it is known to converge to the correlation coefficient of the pair of random variables behind the two data series, with normal fluctuations, as n tends to infinity. This property remains if the two sequences of data have some level of sequential correlation and are stationary. However, it fails under stronger memory conditions, and when the sequences are sufficiently non-stationary. Famously, the statistic is asymptotically diffuse, over the entire interval (−1,1), when the data are random walks. The statistics is known as Yule's "nonsense correlation" in honor of the statistician G. Udny Yule who first described the phenomenon in 1926. Many decades later, there still exist vexing instances of applied scientists who draw incorrect attribution conclusions based on invalid inference about correlations of time series, in ignorance of Yule’s observation. We will described the mathematical question of what happens exactly with ρn as n gets large. We will present an explicit expression for ρn’s second moment, in the case of a pair of discrete-time random walks with Gaussian increments, and we will explain why this moment converges to 0 at the rate 1/n2. This result appeared in a paper with Philip Ernst and Dongzhou Huang, in SPA in April 2023. The result motivates the further study of ρn’s asymptotics, in order to build statistical test of independence of paths of Gaussian stochastic processes. We will discuss this open issue briefly, which involves Gaussian and non-Gaussian convergence in Wiener chaos (Online) |
19:00 - 21:00 |
Dinner (Restaurant Hotel Hacienda Los Laureles) |