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Generalized slow-roll inflation

2000/04/17 by Valerio Faraoni · 1 citation
Physics and Astronomy · #Attractor #Black Holes and Theoretical Physics #Cosmology and Gravitation Theories #Coupling (piping) #Coupling parameter #Field (mathematics) #Inflation (cosmology) #Inflaton #Phase space #Pulsars and Gravitational Waves Research #Spacetime #astro-ph #gr-qc #hep-th

paper · pdf · doi:10.1016/s0375-9601(00)00257-7

published as Phys.Lett.A269:209-213,2000 · 14 pages, LaTeX, some typos corrected

arxiv created 2000/04/17 · openalex publication_date 2000/05/01 · arxiv updated 2011/08/11 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

The slow-roll approximation to inflation is ultimately justified by the presence of inflationary attractors for the orbits of the solutions of the dynamical equations in phase space. There are many indications that the inflaton field couples nonminimally to the spacetime curvature: the existence of attractor points for inflation with nonminimal coupling is demonstrated, subject to a condition on the inflaton potential and the value of the coupling constant.

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