Late time acceleration in Palatini gravity

Abstract We investigate the effect of the quadratic correction αR 2 and non-minimal coupling ξϕ 2 R on a quintessence model with an exponential potential V(ϕ) = M 4exp(−λϕ) in the Palatini formulation of gravity. We use dynamical system techniques to analyze the attractor structure of the model and...

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Main Authors: Ignatios Antoniadis, Anthony Guillen, Kyriakos Tamvakis
Format: Article
Language:English
Published: SpringerOpen 2022-11-01
Series:Journal of High Energy Physics
Subjects:
Online Access:https://doi.org/10.1007/JHEP11(2022)144
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author Ignatios Antoniadis
Anthony Guillen
Kyriakos Tamvakis
author_facet Ignatios Antoniadis
Anthony Guillen
Kyriakos Tamvakis
author_sort Ignatios Antoniadis
collection DOAJ
description Abstract We investigate the effect of the quadratic correction αR 2 and non-minimal coupling ξϕ 2 R on a quintessence model with an exponential potential V(ϕ) = M 4exp(−λϕ) in the Palatini formulation of gravity. We use dynamical system techniques to analyze the attractor structure of the model and uncover the possible trajectories of the system. We find that the quadratic correction cannot play a role in the late time dynamics, except for unacceptably large values of the parameter α; although it can play a role at early times. We find viable evolutions, from a matter-dominated phase to an accelerated expansion phase, with the dynamics driven by the non-minimal coupling. These evolutions correspond to trajectories where the field ends up frozen, thus acting as a cosmological constant.
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spelling doaj.art-5f1748b88e0a4167ac20f3eac167c8a82023-03-22T10:15:39ZengSpringerOpenJournal of High Energy Physics1029-84792022-11-0120221112310.1007/JHEP11(2022)144Late time acceleration in Palatini gravityIgnatios Antoniadis0Anthony Guillen1Kyriakos Tamvakis2Laboratoire de Physique Théorique et Hautes Energies — LPTHE, Sorbonne Université, CNRSLaboratoire de Physique Théorique et Hautes Energies — LPTHE, Sorbonne Université, CNRSPhysics Department, University of IoanninaAbstract We investigate the effect of the quadratic correction αR 2 and non-minimal coupling ξϕ 2 R on a quintessence model with an exponential potential V(ϕ) = M 4exp(−λϕ) in the Palatini formulation of gravity. We use dynamical system techniques to analyze the attractor structure of the model and uncover the possible trajectories of the system. We find that the quadratic correction cannot play a role in the late time dynamics, except for unacceptably large values of the parameter α; although it can play a role at early times. We find viable evolutions, from a matter-dominated phase to an accelerated expansion phase, with the dynamics driven by the non-minimal coupling. These evolutions correspond to trajectories where the field ends up frozen, thus acting as a cosmological constant.https://doi.org/10.1007/JHEP11(2022)144Classical Theories of GravityEffective Field Theories
spellingShingle Ignatios Antoniadis
Anthony Guillen
Kyriakos Tamvakis
Late time acceleration in Palatini gravity
Journal of High Energy Physics
Classical Theories of Gravity
Effective Field Theories
title Late time acceleration in Palatini gravity
title_full Late time acceleration in Palatini gravity
title_fullStr Late time acceleration in Palatini gravity
title_full_unstemmed Late time acceleration in Palatini gravity
title_short Late time acceleration in Palatini gravity
title_sort late time acceleration in palatini gravity
topic Classical Theories of Gravity
Effective Field Theories
url https://doi.org/10.1007/JHEP11(2022)144
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AT anthonyguillen latetimeaccelerationinpalatinigravity
AT kyriakostamvakis latetimeaccelerationinpalatinigravity