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We review the well-known Peebles-Vilenkin (PV) quintessential inflation model and discuss its possible improvements in agreement with the recent observations.
1903
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1904
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1999
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1999
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M. Giovannini, Production and detection of relic gravitons in quintessential inflationary models,
1999
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G. Felder, L. Kofman and A. Linde, Instant Preheating
1999
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G. Felder, L. Kofman and A. Linde, Inflation and Preheating in NO models
1999
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A. R. Liddle and R. J. Scherrer, A classification of scalar field potentials with cosmological scaling solutions
1999
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V. Sahni and L. M. Wang, A New cosmological model of quintessence and dark matter,
2000
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T. Barreiro, E. J. Copeland and N. J. Nunes, Quintessence arising from exponential potentials,
2000
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2016
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P. A. R. Ade et al., Planck 2015 results. XIII. Cosmological parameters
2016
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J. de Haro, On the viability of quintessential inflation models from observational data,
2017
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J. de Haro and L. Aresté Saló, Reheating constraints in quintessential inflation,
2017
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L. A. Ureña-López and T. Matos, A New cosmological tracker solution for quintessence,
2000
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D. J. H. Chung, P. Crotty, E. W. Kolb and A. Riotto, On the gravitational production of superheavy dark matter
2001
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K. Dimopoulos and J. W. F. Valle, Modeling Quintessential Inflation
2002
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M. Giovannini, Low scale quintessential inflation,
2003
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B. A. Bassett, S. Tsujikawa and D. Wands, Inflation Dynamics and Reheating
2006
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E. J. Copeland, M. Sami and S. Tsujikawa, Dynamics of dark energy
2006
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2017
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L. Aresté Saló and J. de Haro, Quintessential inflation at low reheating temperatures,
2017
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J. Rubio and C. Wetterich, Emergent scale symmetry: Connecting inflation and dark energy
2017
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J. Haro and S. Pan, Bulk viscous quintessential inflation,
2018
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Y. Akrami et al., Planck 2018 results. X. Constraints on inflation
2018
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Y. Akrami et al., Planck 2018 results. VI. Cosmological parameters
2018
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2018
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2018
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Y. Ema, K. Nakayama and Y. Tang, Production of Purely Gravitational Dark Matter
2018
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2019
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2019
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J. Haro, Different reheating mechanisms in quintessence inflation
2019
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