Spacetimes with vector distortion: Inflation from generalised Weyl geometry

Spacetime with general linear vector distortion is introduced. Thus, the torsion and the nonmetricity of the affine connection are assumed to be proportional to a vector field (and not its derivatives). The resulting two-parameter family of non-Riemannian geometries generalises the conformal Weyl ge...

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Main Authors: Jose Beltrán Jiménez, Tomi S. Koivisto
Format: Article
Language:English
Published: Elsevier 2016-05-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316300181
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author Jose Beltrán Jiménez
Tomi S. Koivisto
author_facet Jose Beltrán Jiménez
Tomi S. Koivisto
author_sort Jose Beltrán Jiménez
collection DOAJ
description Spacetime with general linear vector distortion is introduced. Thus, the torsion and the nonmetricity of the affine connection are assumed to be proportional to a vector field (and not its derivatives). The resulting two-parameter family of non-Riemannian geometries generalises the conformal Weyl geometry and some other interesting special cases. Taking into account the leading nonlinear correction to the Einstein–Hilbert action results uniquely in the one-parameter extension of the Starobinsky inflation known as the alpha-attractor. The most general quadratic curvature action introduces, in addition to the canonical vector kinetic term, novel ghost-free vector-tensor interactions.
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spelling doaj.art-8264c14d83114024acf8998bb6cfdb842022-12-21T23:21:08ZengElsevierPhysics Letters B0370-26931873-24452016-05-01756C40040410.1016/j.physletb.2016.03.047Spacetimes with vector distortion: Inflation from generalised Weyl geometryJose Beltrán Jiménez0Tomi S. Koivisto1CPT, Aix Marseille Université, UMR 7332, 13288 Marseille, FranceNordita, KTH Royal Institute of Technology and Stockholm University, Roslagstullsbacken 23, 10691 Stockholm, SwedenSpacetime with general linear vector distortion is introduced. Thus, the torsion and the nonmetricity of the affine connection are assumed to be proportional to a vector field (and not its derivatives). The resulting two-parameter family of non-Riemannian geometries generalises the conformal Weyl geometry and some other interesting special cases. Taking into account the leading nonlinear correction to the Einstein–Hilbert action results uniquely in the one-parameter extension of the Starobinsky inflation known as the alpha-attractor. The most general quadratic curvature action introduces, in addition to the canonical vector kinetic term, novel ghost-free vector-tensor interactions.http://www.sciencedirect.com/science/article/pii/S0370269316300181
spellingShingle Jose Beltrán Jiménez
Tomi S. Koivisto
Spacetimes with vector distortion: Inflation from generalised Weyl geometry
Physics Letters B
title Spacetimes with vector distortion: Inflation from generalised Weyl geometry
title_full Spacetimes with vector distortion: Inflation from generalised Weyl geometry
title_fullStr Spacetimes with vector distortion: Inflation from generalised Weyl geometry
title_full_unstemmed Spacetimes with vector distortion: Inflation from generalised Weyl geometry
title_short Spacetimes with vector distortion: Inflation from generalised Weyl geometry
title_sort spacetimes with vector distortion inflation from generalised weyl geometry
url http://www.sciencedirect.com/science/article/pii/S0370269316300181
work_keys_str_mv AT josebeltranjimenez spacetimeswithvectordistortioninflationfromgeneralisedweylgeometry
AT tomiskoivisto spacetimeswithvectordistortioninflationfromgeneralisedweylgeometry