# Intrinsic area near the origin for self-similar growth-fragmentations   and related random surfaces

**Authors:** Fran\c{c}ois Gaston Ged

arXiv: 1908.03746 · 2019-08-13

## TL;DR

This paper investigates the asymptotic behavior of a natural measure on the leaves of genealogical trees in self-similar growth-fragmentation processes, revealing new insights into their measure distribution near the origin and applications to random surfaces.

## Contribution

It provides the almost sure and distributional asymptotics of the measure near the root for self-similar growth-fragmentations, extending results to random surfaces and stable disks.

## Key findings

- Almost sure behavior of the measure when the Eve cell starts positive
- Distributional convergence of rescaled measure in certain cases
- Bounds on the measure's behavior near the origin

## Abstract

We study the behaviour of a natural measure defined on the leaves of the genealogical tree of some branching processes, namely self-similar growth-fragmentation processes.   Each particle, or cell, is attributed a positive mass that evolves in continuous time according to a positive self-similar Markov process and gives birth to children at negative jumps events.   We are interested in the asymptotics of the mass of the ball centered at the root, as its radius decreases to $0$.   We obtain the almost sure behaviour of this mass when the Eve cell starts with a strictly positive size.   This differs from the situation where the Eve cell grows indefinitely from size 0.   In this case, we show that, when properly rescaled, the mass of the ball converges in distribution towards a non-degenerate random variable.   We then derive bounds describing the almost sure behaviour of the rescaled mass.   Those results are applied to certain random surfaces, exploiting the connection between growth-fragmentations and random planar maps obtained in Bertoin et al. [6].   This allows us to extend a result of Le Gall [24] on the volume of a free Brownian disk close to its boundary, to a larger family of stable disks.   The upper bound of the mass of a typical ball in the Brownian map is refined, and we obtain a lower bound as well.

## Full text

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## References

37 references — full list in the complete paper: https://tomesphere.com/paper/1908.03746/full.md

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Source: https://tomesphere.com/paper/1908.03746