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By making use of a class of steep exponential type of potentials, which has been recently used to describe quintessential inflation, we show how a unified picture for both inflation, dark energy and dark matter can emerge entirely through dissipative effects.
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2008
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I. G. Moss and C. Xiong, On the consistency of warm inflation
2008
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N. Bose and A. S. Majumdar, Unified Model of k-Inflation, Dark Matter & Dark Energy
2009
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M. Bastero-Gil, A. Berera, B. M. Jackson and A. Taylor, Hybrid Quintessential Inflation
2009
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A. Berera, I. G. Moss and R. O. Ramos, Warm Inflation and its Microphysical Basis
2009
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2009
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2009
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2015
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2016
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M. Bastero-Gil, A. Berera, R. O. Ramos and J. G. Rosa, Warm Little Inflaton
2016
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M. Bastero-Gil, R. Cerezo and J. G. Rosa, Inflaton dark matter from incomplete decay
2016
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2017
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2017
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S. Ahmad, R. Myrzakulov and M. Sami, Relic gravitational waves from Quintessential Inflation
2017
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2017
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J. E. Bautista et al
2018
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2018
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2018
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2019
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M. Motaharfar, V. Kamali and R. O. Ramos, Warm inflation as a way out of the swampland
2019
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S. Das, Warm Inflation in the light of Swampland Criteria
2019
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J. G. Rosa and L. B. Ventura, Warm Little Inflaton becomes Cold Dark Matter
2019
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I. G. Moss and C. M. Graham, Particle production and reheating in the inflationary universe
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