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The first exponential function of this double exponential potential dominates during the radiation dominated era, the second exponential potential dominates during the matter dominated era [8], gives an effective γ(ϕ) varying smoothly · 2018

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2019 1

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Scaling solutions in quintessential inflation

gr-qc · 2019-08-05 · conditional · novelty 5.0

In quintessential inflation, the scalar field misses the scaling-solution attractor during radiation, so a single exponential tail can drive both inflation and dark energy.

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  • Scaling solutions in quintessential inflation gr-qc · 2019-08-05 · conditional · none · ref 2

    In quintessential inflation, the scalar field misses the scaling-solution attractor during radiation, so a single exponential tail can drive both inflation and dark energy.