<tt>WI2easy</tt>: warm inflation dynamics made easy

Abstract We present WI2easy , a Mathematica package for high-precision analysis of warm inflation (WI) dynamics, enabling efficient computation of both background evolution and curvature perturbations. Designed with a user-friendly interface, the tool supports a broad spectrum of inflaton potentials — including large-field, small-field, and hybrid models — and accommodates arbitrary dissipation coefficients dependent on temperature, field amplitude, or both, encompassing canonical forms prevalent in WI studies. Users can define custom models through intuitive commands, generating full dynamical trajectories and perturbation spectra in a streamlined workflow. This facilitates rapid confrontation of theoretical predictions with observational constraints, empowering systematic exploration of WI parameter spaces. WI2easy bridges the gap between theoretical models and observational cosmology, offering a robust, adaptable framework for next-generation inflationary analyses.

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Publication Details

Journal
Journal of Cosmology and Astroparticle Physics
Published
2025-09-01
DOI
https://doi.org/10.1088/1475-7516/2025/09/014
Citations
7
Primary Topic
Cosmology and Gravitation Theories
Type
article
Field-Weighted Citation Impact
8.08

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article

<tt>WI2easy</tt>: warm inflation dynamics made easy

Rudnei O. Ramos, Gabriel S. Rodrigues
7 citations
Journal of Cosmology and Astroparticle Physics
Cosmology and Gravitation Theories
8.08
article

<tt>WI2easy</tt>: warm inflation dynamics made easy

Rudnei O. Ramos, Gabriel S. Rodrigues
article en
7 citations

Abstract

Abstract We present WI2easy , a Mathematica package for high-precision analysis of warm inflation (WI) dynamics, enabling efficient computation of both background evolution and curvature perturbations. Designed with a user-friendly interface, the tool supports a broad spectrum of inflaton potentials — including large-field, small-field, and hybrid models — and accommodates arbitrary dissipation coefficients dependent on temperature, field amplitude, or both, encompassing canonical forms prevalent in WI studies. Users can define custom models through intuitive commands, generating full dynamical trajectories and perturbation spectra in a streamlined workflow. This facilitates rapid confrontation of theoretical predictions with observational constraints, empowering systematic exploration of WI parameter spaces. WI2easy bridges the gap between theoretical models and observational cosmology, offering a robust, adaptable framework for next-generation inflationary analyses.

Journal of Cosmology and Astroparticle PhysicsVol. 2025(09)
Universidade do Estado do Rio de Janeiro (BR)
Conselho Nacional de Desenvolvimento Científico e Tecnológico, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro
Openalex Percentile: Top 3%
Cosmology and Gravitation Theories
8.08
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