Abstract
Inhomogeneous fluid models for warm inflation are investigated. The early-time acceleration is supported by inhomogeneous fluid whose coupling with radiation leads to the radiation dominated era after inflation. Several examples are analyzed, strong dissipation regime is discussed, and the viability of the models respect to the last Planck data is verified.
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Myrzakul, S., Myrzakulov, R. & Sebastiani, L. Inhomogeneous fluids for warm inflation. Astrophys Space Sci 357, 168 (2015). https://doi.org/10.1007/s10509-015-2397-1
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DOI: https://doi.org/10.1007/s10509-015-2397-1