# Game changing mutation

**Authors:** Omer Edhan, Ziv Hellman

PMC · DOI: 10.1098/rsos.241951 · Royal Society Open Science · 2025-04-30

## TL;DR

This paper models mutation in sexually reproducing populations as a game-theoretic process, showing how mutations can change evolutionary outcomes by altering the game's structure.

## Contribution

The paper introduces a novel game-theoretic framework where mutations are modeled as changes to the game's action set, affecting evolutionary dynamics.

## Key findings

- Populations converge to pure Nash equilibria in the absence of mutations.
- Game-changing mutations can shift populations to new equilibria with higher fitness.
- The model is applied to understand fitness valley crossing and evolutionary contingency.

## Abstract

We present a model of the effect of mutation on haploid sexually reproducing populations by modelling the reproductive dynamics as occurring in the context of a common interests game played by the loci, with the alleles in the role of pure actions. Absent mutations, the population will deterministically converge to a pure Nash equilibrium of the game. A novel mutation adds new alleles, hence is tantamount to a change of the game by the addition of new actions. If the new game defined by the mutation removes the former pure Nash equilibrium the game changing mutation becomes in addition a Nash equilibrium changing mutation, as the population will then move to a new equilibrium with an increase in fitness. A graph of common interests games is defined, and evolution by mutation is modelled as a path through this graph. We discuss two applications—fitness valley crossing and evolutionary contingency.

## Full-text entities

- **Diseases:** PDMP (MESH:D010335)
- **Species:** Homo sapiens (human, species) [taxon 9606]

## Full text

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## Figures

6 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12041896/full.md

## References

33 references — full list in the complete paper: https://tomesphere.com/paper/PMC12041896/full.md

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Source: https://tomesphere.com/paper/PMC12041896