![Schematic illustration of the non-spatial Hash Chemistry model (from [16], with modification). - -[q-bio.PE]](https://i0.wp.com/astrobiology.com/wp-content/uploads/2026/08/Hash-Chemistry.png?fit=1200%2C676&ssl=1)
[q-bio.PE] Hash Chemistry is a family of minimalistic evolutionary models in which a deterministic hash function assigns a scalar score to entities of arbitrary size, opening a combinatorially vast possibility space (a “cardinality leap). Since its introduction, the idea has been realized in several settings, from the original spatial formulation to a fast non-spatial variant and then to structural cellular models.
Here we review the Hash Chemistry family as a coherent modeling framework and use it to explore how minimal systems can demonstrate the mechanisms behind multiscale open-ended evolutionary dynamics. The most recent model, Structural Cellular Hash Chemistry (SCHC), successfully demonstrated multiscale ecological interaction/adaptation and complexity growth of replicators in a computationally efficient manner. In this study, we first extend SCHC to incorporate spatial locality and dyadicity of competitive interactions among replicating structures.
We show this extension substantially enhances SCHC’s evolutionary dynamics. Furthermore, we explore SCHC in a significantly larger spatial domain using a GPU-accelerated implementation.
We show that the size of the space acts as a control parameter for a stochastic, nucleation-like transition between a compact-replicator regime and a runaway size-dominance regime, and we separate the responsible mechanism into a non-spatial, size-biased sampling feedback and a finite-size spatial effect. Altogether, these results illustrate the rich potential of Hash Chemistry as a minimal, mechanistically transparent testbed for studying open-ended evolution across scales.
Ilya Horiguchi, Hiroki Sayama
Comments: 26 pages, 9 figures, 4 tables
Subjects: Populations and Evolution (q-bio.PE); Neural and Evolutionary Computing (cs.NE); Cellular Automata and Lattice Gases (nlin.CG)
Cite as: arXiv:2607.28219 [q-bio.PE] (or arXiv:2607.28219v1 [q-bio.PE] for this version)
https://doi.org/10.48550/arXiv.2607.28219
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Submission history
From: Hiroki Sayama
[v1] Thu, 30 Jul 2026 13:54:23 UTC (1,097 KB)
https://arxiv.org/abs/2607.28219
Astrobiology,
