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On the possibility of braneworld quintessential inflation

2010/02/19 by Mafalda Dias, Andrew R. Liddle, Andrew R Liddle · 13 citations
Physics and Astronomy · #Astrophysics #Black Holes and Theoretical Physics #Context (archaeology) #Cosmology #Cosmology and Gravitation Theories #Dark energy #Galaxies: Formation, Evolution, Phenomena #Geography #Inflation (cosmology) #Inflaton #Philosophy #Physics #Quintessence #Restrictiveness #Theoretical physics #astro-ph.CO

paper · pdf · doi:10.1103/physrevd.81.083515

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 81(8) (American Physical Society) · 11 pages RevTex file with 13 figures

arxiv created 2010/02/19 · openalex publication_date 2010/04/14 · arxiv updated 2010/04/22 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

We examine the possibility of achieving quintessential inflation, where the same field serves as both inflaton and quintessence, in the context of a five-dimensional braneworld. Braneworld cosmology provides an appropriate environment as it permits inflation with much steeper potentials than the conventional scenario, which is favorable to a late-time quintessence. We explore a wide space of models, together with contemporary observational data, to determine in which contexts such a picture is possible. We find that such a scenario, although attractive, is in fact impossible to achieve for the potentials studied due to the restrictiveness of current data.

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