Three channel dissipative warm Higgs inflation with global inference via genetic algorithms
Wei Cheng

TL;DR
This paper develops a three-channel dissipative Warm Higgs Inflation model, employing genetic algorithms and priors to explore multi-channel solutions and their cosmological implications.
Contribution
It introduces a novel three-channel dissipation framework with structural priors and a layered warmness criterion, enhancing the exploration of multi-channel inflationary solutions.
Findings
Significantly increased viable multi-channel solutions with priors.
Discovery of a 'channel relay' dynamical feature during evolution.
Microscopic dissipation origins can be multi-faceted within a single inflationary history.
Abstract
This paper constructs and analyzes a three channel dissipative framework for Warm Higgs Inflation, wherein the total dissipation coefficient, , is decomposed into low temperature, high temperature, and threshold activated contributions. A genetic algorithm is employed for the global numerical solution and statistical inference of the background field dynamics. To overcome the single channel dominance degeneracy in high dimensional parameter scans, two classes of structural priors are introduced into the objective function: a \texttt{mixing} prior to suppress extreme channel fractions and an \texttt{entropy} prior to favor multi channel coexistence. Furthermore, the adoption of a layered warmness criterion (e.g., ) decouples model selection from cosmological observables, thereby enhancing analytical transparency. The complete workflow is demonstrated…
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Taxonomy
TopicsCosmology and Gravitation Theories · Particle physics theoretical and experimental studies · Galaxies: Formation, Evolution, Phenomena
