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Jointly modelling Cosmic Inflation and Dark Energy

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arxiv 2106.14966 v1 pith:H6QWVPXN submitted 2021-06-28 gr-qc astro-ph.COhep-phhep-th

Konstantinos Dimopoulos This is my paper
classification gr-qcastro-ph.COhep-phhep-th
keywords inflationcosmicdarkenergymodellingquintessentialaccountalpha
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abstract

Quintessential inflation utilises a single scalar field to account for the observations of both cosmic inflation and dark energy. The requirements for modelling quintessential inflation are described and two explicit successful models are presented in the context of $\alpha$-attractors and Palatini modified gravity.

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Cited by 1 Pith paper

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  1. Post-Inflationary Constraints on Nonminimally Coupled Quintessential Inflation

    gr-qc 2026-08 conditional novelty 6.0 of 10

    Gravitational-wave constraints on the reheating temperature rule out single-exponential nonminimally coupled quintessential inflation and require a double-exponential coupling that predicts thawing dark energy with w0...

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