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We discuss how dissipative effects and the presence of a thermal radiation bath, which are inherent characteristics of the warm inflation dynamics, can evade the recently proposed Swampland conjectures.
1929
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A. Berera, Warm Inflation
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A. Berera, M. Gleiser, and R. O. Ramos, Strong dissipative behavior in quantum field theory , Phys. Rev. D 58
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A. Berera, M. Gleiser, and R. O. Ramos, A First principles warm inflation model that solves the cosmological horizon / flatness problems , Phys. Rev. Lett. 83
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L. M. H. Hall, I. G. Moss, and A. Berera, Scalar perturbation spectra from warm inflation , Phys. Rev. D 69
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H. Ooguri and C. Vafa, On the geometry of the string landscape and the Swampland
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M. A. Cid, S. del Campo, and R. Herrera, Warm inflation on the brane
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A. Berera, I. G. Moss, and R. O. Ramos, Warm inflation and its microphysical basis
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M. Bastero-Gil and A. Berera, Warm inflation model building
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R. O. Ramos and L. A. da Silva, Power spectrum for inflation models with quantum and thermal noises
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A. Kehagias and A. Riotto, A note on inflation and the Swampland
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