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Warm quintessential inflation

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Publication:2326279
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DOI10.1016/j.physletb.2019.07.017zbMath1422.83020arXiv1906.09648OpenAlexW2952132991MaRDI QIDQ2326279

Konstantinos Dimopoulos, Leonora Donaldson-Wood

Publication date: 7 October 2019

Published in: Physics Letters. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1906.09648



Mathematics Subject Classification ID

Relativistic cosmology (83F05)


Related Items (11)

Relic gravitons from stiff curvature perturbations ⋮ Inflation in string field theory ⋮ Waterfall stiff period can generate observable primordial gravitational waves ⋮ Palatini R 2 quintessential inflation ⋮ Hubble-induced phase transitions: Walls are not forever ⋮ Warm dark energy ⋮ The paradigm of warm quintessential inflation and spontaneous baryogenesis ⋮ Cosmological relevance of scaling solutions: a recipe for quintessential inflation ⋮ Towards a reliable effective field theory of inflation ⋮ Warm inflation, neutrinos and dark matter: a minimal extension of the standard model ⋮ Quintessential α-attractor inflation: forecasts for Stage IV galaxy surveys



Cites Work

  • Non-minimal gravitational reheating during kination
  • The Landscape, the Swampland and the Era of Precision Cosmology


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