More than fifty years have elapsed since the publication of ‘A statistical theory of spatial distribution models’. In a paper with Britton Harris in 1978, new foundations were laid for dynamic modelling – later seen as adding space to Lotka-Volterra concepts to the Boltzmann core, and hence for these models to be labelled as BLV models.
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This work deepens our understanding of the fundamental laws governing the universe, from subatomic particles to cosmic structures.
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