Population size of critical Galton-Watson processes under small deviations and infinite variance
Vladimir Vatutin, Elena Dyakonova
TL;DR
This work analyzes a critical Galton-Watson process with infinite offspring-variance, characterized by $f(s)=s+(1-s)^{1+\alpha}L(1-s)$ for $\alpha\in(0,1]$, and studies the distribution of the population size $Z(m)$ under the rare event that the distant-time population is small, encoded by the conditioning $\mathcal{H}(n,\varphi(n))$. By leveraging Yaglom-type limits, a reduced process $Z(m,n)$, and auxiliary asymptotics for $\mathcal{H}(n,\varphi(n))$, the authors derive explicit asymptotic Laplace transforms of $Z(m)$ across five regimes relating $m$ and $n$. The results reveal a rich set of conditional limit laws: a universal $(1+\lambda^{\alpha})^{-(1/\alpha+1)}$ form in the $m=o(n)$ regime; a theta-dependent family in the $m\sim \theta n$ regime; a near-terminal universal $(1+\lambda)^{-(\alpha+1)}$ form for $m=n-\psi(n)$; a convolutional series in the $n-m\sim y\varphi(n)$ case; and a beta-like $\alpha\int_0^1 x^{\alpha-1} e^{ -\lambda x } dx$ limit when the gap is $n-\chi(n)$. These findings extend Yaglom-type results to infinite-variance offspring laws and provide precise characterizations of how a small distant-time population emerges under various observational gaps, with implications for MRCA-distance scaling and conditional branching behavior.
Abstract
We study the evolution of the population size distribution of a critical Galton-Watson process with infinite variance of the offspring size of particles assuming that the population size is unusually small at the distant moment $n$ of observation.
