Modified gravity with an exponential function of curvature

Abstract The role of an exponential function of the scalar curvature in the modified gravity is analyzed. Two models are proposed. A toy model that complies with local and cosmological constraints and gives appropriate qualitative description of the cosmic evolution. This model contains a saddle mat...

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Main Author: L. N. Granda
Format: Article
Language:English
Published: SpringerOpen 2020-06-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-020-8114-4
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author L. N. Granda
author_facet L. N. Granda
author_sort L. N. Granda
collection DOAJ
description Abstract The role of an exponential function of the scalar curvature in the modified gravity is analyzed. Two models are proposed. A toy model that complies with local and cosmological constraints and gives appropriate qualitative description of the cosmic evolution. This model contains a saddle matter-dominant critical point that can evolve towards a late time de Sitter attractor. Initial conditions have been proposed, showing that this toy model has an acceptable matter era and gives an approximate qualitative behavior of cosmic evolution. A second viable model, behaves very close to $$\Lambda $$ Λ CDM at early times and can satisfy local and cosmological constraints. It behaves as $$R-2\Lambda $$ R-2Λ at $$R\rightarrow \infty $$ R→∞ and tends to zero at $$R\rightarrow 0$$ R→0 , containing flat spacetime solution. The model gives viable cosmological trajectories that, as the first model, connect the matter dominated point with a late time de Sitter attractor. The cosmic evolution of the main density parameters in this model is consistent with current observations with an equation of state very close to $$-1$$ -1 .
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spelling doaj.art-7c9ab9ff470f42ec9c8542630bee4d1a2022-12-22T00:59:05ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522020-06-0180611110.1140/epjc/s10052-020-8114-4Modified gravity with an exponential function of curvatureL. N. Granda0Departamento de Fisica, Universidad del ValleAbstract The role of an exponential function of the scalar curvature in the modified gravity is analyzed. Two models are proposed. A toy model that complies with local and cosmological constraints and gives appropriate qualitative description of the cosmic evolution. This model contains a saddle matter-dominant critical point that can evolve towards a late time de Sitter attractor. Initial conditions have been proposed, showing that this toy model has an acceptable matter era and gives an approximate qualitative behavior of cosmic evolution. A second viable model, behaves very close to $$\Lambda $$ Λ CDM at early times and can satisfy local and cosmological constraints. It behaves as $$R-2\Lambda $$ R-2Λ at $$R\rightarrow \infty $$ R→∞ and tends to zero at $$R\rightarrow 0$$ R→0 , containing flat spacetime solution. The model gives viable cosmological trajectories that, as the first model, connect the matter dominated point with a late time de Sitter attractor. The cosmic evolution of the main density parameters in this model is consistent with current observations with an equation of state very close to $$-1$$ -1 .http://link.springer.com/article/10.1140/epjc/s10052-020-8114-4
spellingShingle L. N. Granda
Modified gravity with an exponential function of curvature
European Physical Journal C: Particles and Fields
title Modified gravity with an exponential function of curvature
title_full Modified gravity with an exponential function of curvature
title_fullStr Modified gravity with an exponential function of curvature
title_full_unstemmed Modified gravity with an exponential function of curvature
title_short Modified gravity with an exponential function of curvature
title_sort modified gravity with an exponential function of curvature
url http://link.springer.com/article/10.1140/epjc/s10052-020-8114-4
work_keys_str_mv AT lngranda modifiedgravitywithanexponentialfunctionofcurvature