Quintessential inflation from a variable cosmological constant in a 5D vacuum

DOI10.1016/J.PHYSLETB.2006.08.043zbMath1248.83166arXivgr-qc/0606119OpenAlexW2081486877MaRDI QIDQ712823

Mauricio Bellini, Agustin Membiela

Publication date: 18 October 2012

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

Full work available at URL: https://arxiv.org/abs/gr-qc/0606119

zbMATH Keywords

effective 4D cosmological model

Mathematics Subject Classification ID

Relativistic cosmology (83F05)

Related Items (4)

Cosmological relevance of scaling solutions: a recipe for quintessential inflation ⋮ Warm Little Inflaton becomes dark energy ⋮ Unification of inflation and dark energyà laquintessential inflation ⋮ Non-minimal gravitational reheating during kination

Cites Work

• EQUIVALENCE BETWEEN SPACE–TIME–MATTER AND BRANE-WORLD THEORIES
• Kaluza–Klein equations, Einstein’s equations, and an effective energy-momentum tensor
• An Alternative to Compactification
• Cosmological Imprint of an Energy Component with General Equation of State

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