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Analysis

This paper explores a three-channel dissipative framework for Warm Higgs Inflation, using a genetic algorithm and structural priors to overcome parameter space challenges. It highlights the importance of multi-channel solutions and demonstrates a 'channel relay' feature, suggesting that the microscopic origin of dissipation can be diverse within a single inflationary history. The use of priors and a layered warmness criterion enhances the discovery of non-trivial solutions and analytical transparency.
Reference

The adoption of a layered warmness criterion decouples model selection from cosmological observables, thereby enhancing analytical transparency.