Skip to main content
Log in

Self-Attracting Poisson Clouds in an Expanding Universe

  • Published:
Communications in Mathematical Physics Aims and scope Submit manuscript

Abstract:

 We consider the following elementary model for clustering by ballistic aggregation in an expanding universe. At the initial time, there is a doubly infinite sequence of particles lying in a one-dimensional universe that is expanding at constant rate. We suppose that each particle p attracts points at a certain rate a(p)/2 depending only on p, and when two particles, say p and q, collide by the effect of attraction, they merge as a single particle p*q. The main purpose of this work is to point at the following remarkable property of Poisson clouds in these dynamics. Under certain technical conditions, if at the initial time the system is distributed according to a spatially stationary Poisson cloud with intensity μ 0 , then at any time t > 0, the system will again have a Poissonian distribution, now with intensity μ t , where the family solves a generalization of Smoluchowski's coagulation equation.

This is a preview of subscription content, log in via an institution to check access.

Access this article

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Similar content being viewed by others

Author information

Authors and Affiliations

Authors

Additional information

Received: 15 February 2002 / Accepted: 8 July 2002 Published online: 7 November 2002

Rights and permissions

Reprints and permissions

About this article

Cite this article

Bertoin, J. Self-Attracting Poisson Clouds in an Expanding Universe. Commun. Math. Phys. 232, 59–81 (2002). https://doi.org/10.1007/s00220-002-0740-1

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1007/s00220-002-0740-1

Keywords

Navigation