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Extended Warm Inflation

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arxiv astro-ph/9910568 v1 pith:P3UIPZZV submitted 1999-11-01 astro-ph

J. M. F. Maia (Universidade Federal do R. G. Norte , Universidade de S. Paulo) , J. A. S. Lima (Universidade Federal do R. G. Norte) This is my paper · ORCID
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A bidimensional parameter space of unitary area is introduced to study phenomenologically the dynamic and thermodynamic behavior of inflationary models driven by a scalar field coupled to a thermal component. In this enlarged context the isentropic and warm pictures are just extreme cases of an infinite two-parametric family of possible inflationary scenarios. It is also shown that strong couplings are responsible by an alteration in the standard slow roll conditions which relax the smallness constraint on the first and the second derivatives of the potential.

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  1. Stage IV CMB forecasts for warm inflation

    astro-ph.CO 2024-12 conditional novelty 5.0 of 10

    Future CMB surveys are forecast to tighten the dissipation parameter of quartic warm inflation by up to an order of magnitude and to exclude the cubic dissipation model under a null tensor-to-scalar ratio.

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