Invasion with size-dependent dispersion range

The coalescing colony model provides a minimal framework for biological invasions with long-range dispersion.

In its standard formulation, the dispersion range is assumed independent of the size of the invading population.

Here, we relax this assumption and consider size-dependent dispersal: a main colony of linear size $r$ emits secondary colonies at distance $r^\mu$, with $0 \leq \mu \leq 1$.

We derive the generalized dynamical equations for this extended model and map out the growth phase diagram for the leading order contribution.

Depending on $\mu$, the main colony exhibits distinct regimes: linear expansion, power-law growth, exponential regime and finite-time blow-up.

We confront these theoretical predictions with a spatially explicit physical model.

While the coalescing colony approach correctly captures the scaling of the perimeter, it fails to predict the scaling of the volume.

We trace this discrepancy to an effective breakdown of circular symmetry in the morphology of the main colony.

Finally, we quantify temporal evolution of the population fraction residing outside of the main colony.

The coalescing colony model predicts its decay to~$0$ like a power-law when~$\mu<1$, and a macroscopic amount of the population remains in the secondary colonies at~$\mu=1$.

Simulations of the physical model reveal a persistent satellite population not captured by the theory at~$\mu>\mu^*\approx 0.7$.

Broadly, our findings highlight how coupling dispersal range to population size fundamentally alters invasion dynamics, with implications for biological invasions, metastatic growth, and urban expansion.