Abstract

In this article we study the Atlas model, which constitutes of Brownian particles on $ \mathbb{R} $, independent except that the Atlas (i.e., lowest ranked) particle $ X_{(1)}(t) $ receive drift $ \gamma dt $, $ \gamma\in\mathbb{R} $. For any fixed shape parameter $ a>2\gamma_- $, we show that, up to a shift $ \frac{a}{2}t $, the entire particle system has an invariant distribution $ \nu_a $, written in terms an explicit Radon-Nikodym derivative with respect to the Poisson point process of density $ a e^{a\xi} d\xi $. We further show that $ \nu_a $ indeed has the product-of-exponential gap distribution $ \pi_a $ derived in Sarantsev and Tsai (2016). As a simple application, we establish a bound on the fluctuation of the Atlas particle $ X_{(1)}(t) $ uniformly in $ t $, with the gaps initiated from $ \pi_a $ and $ X_{(1)}(0)=0 $.

Highlights

  • In this article we study the Atlas model

  • Such a model consists of a semiinfinite collection of particles Xi(t), i = 1, 2, . . ., performing independent Brownian motions on R, except that the Atlas particle receives a drift of strength γ ∈ R

  • To rigorously define the model, we recall that x = (xi)∞ i=1 ∈ RN is rankable if there exists a ranking permutation p : N → N such that xp(i) ≤ xp(j), for all i < j ∈ N

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Summary

Introduction

In this article we study the (infinite) Atlas model. Such a model consists of a semiinfinite collection of particles Xi(t), i = 1, 2, . . ., performing independent Brownian motions on R, except that the Atlas (i.e., lowest ranked) particle receives a drift of strength γ ∈ R. Stationary distributions of the Atlas model and note that limi→∞ xi = ∞ necessarily implies that x is rankable. It is shown in [Sar17a, Theorem 3.2], for any fixed γ ∈ R and any given x ∈ U , the system (1.1). Parts of the motivation was to understand the effect of a drift exerted on a large (but finite) collection of Brownian particles [Ald, TT15] It was shown in [PP08] that, for γ > 0, the system (1.1) admits a stationary gap distribution of i.i.d. Exp(2γ), which indicates that the drift γdt is balanced by the push-back of a crowd of particles of density 2γ.

The distribution νa is a stationary distribution of
Using this we calculate
We then consider the following mollified system t
As is Lipschitz with

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