Probabilities of moderately atypical fluctuations of the size of a swarm of Brownian bees

Pavel Sasorov, Arkady Vilenkin, and Naftali R. Smith
Phys. Rev. E 107, 014140 – Published 30 January 2023

Abstract

The “Brownian bees” model describes an ensemble of N= const independent branching Brownian particles. The conservation of N is provided by a modified branching process. When a particle branches into two particles, the particle which is farthest from the origin is eliminated simultaneously. The spatial density of the particles is governed by the solution of a free boundary problem for a reaction-diffusion equation in the limit of N1. At long times, the particle density approaches a spherically symmetric steady-state solution with a compact support of radius ¯0. However, at finite N, the radius of this support, L, fluctuates. The variance of these fluctuations appears to exhibit a logarithmic anomaly [Siboni et al., Phys. Rev. E 104, 054131 (2021)]. It is proportional to N1lnN at N. We investigate here the tails of the probability density function (PDF), P(L), of the swarm radius, when the absolute value of the radius fluctuation ΔL=L¯0 is sufficiently larger than the typical fluctuations' scale determined by the variance. For negative deviations the PDF can be obtained in the framework of the optimal fluctuation method. This part of the PDF displays the scaling behavior lnPNΔL2ln1(ΔL2), demonstrating a logarithmic anomaly at small negative ΔL. For the opposite sign of the fluctuation, ΔL>0, the PDF can be obtained with an approximation of a single particle, running away. We find that lnPN1/2ΔL. We consider in this paper only the case when |ΔL| is much less than the typical radius of the swarm at N1.

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  • Received 15 September 2022
  • Accepted 17 January 2023

DOI:https://doi.org/10.1103/PhysRevE.107.014140

©2023 American Physical Society

Physics Subject Headings (PhySH)

Statistical Physics & Thermodynamics

Authors & Affiliations

Pavel Sasorov1,*, Arkady Vilenkin2,†, and Naftali R. Smith3,‡

  • 1Institute of Physics CAS, ELI Beamlines, 182 21 Prague, Czech Republic
  • 2Racah Institute of Physics, Hebrew University of Jerusalem, Jerusalem 91904, Israel
  • 3Department of Solar Energy and Environmental Physics, Blaustein Institutes for Desert Research, Ben-Gurion University of the Negev, Sede Boqer, 8499000, Israel

  • *pavel.sasorov@gmail.com
  • vilenkin@mail.huji.ac.il
  • naftalismith@gmail.com

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Issue

Vol. 107, Iss. 1 — January 2023

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