Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities

In theories where a scalar field couples nonminimally to gravity, the effective gravitational “constant” becomes dependent on the value of the scalar field. This note first gives a brief review on how the cosmological evolution provides a dynamical stabilization for the gravitational “constant” as t...

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Main Author: Laur Järv
Format: Article
Language:English
Published: MDPI AG 2017-04-01
Series:Universe
Subjects:
Online Access:http://www.mdpi.com/2218-1997/3/2/37
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author Laur Järv
author_facet Laur Järv
author_sort Laur Järv
collection DOAJ
description In theories where a scalar field couples nonminimally to gravity, the effective gravitational “constant” becomes dependent on the value of the scalar field. This note first gives a brief review on how the cosmological evolution provides a dynamical stabilization for the gravitational “constant” as the system relaxes towards general relativity in matter dominated and potential dominated regimes for scalar-(curvature)tensor and scalar-torsion gravities. Second part summarizes the radius dependence of the gravitational “constant” around a point mass in the parametrized post-Newtonian formalism for scalar-tensor and multiscalar-tensor gravity.
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spelling doaj.art-9274ffe403534461ac9eddb2ccd1c3ed2022-12-22T04:25:12ZengMDPI AGUniverse2218-19972017-04-01323710.3390/universe3020037universe3020037Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion GravitiesLaur Järv0Institute of Physics, University of Tartu, W. Ostwaldi 1, 50411 Tartu, EstoniaIn theories where a scalar field couples nonminimally to gravity, the effective gravitational “constant” becomes dependent on the value of the scalar field. This note first gives a brief review on how the cosmological evolution provides a dynamical stabilization for the gravitational “constant” as the system relaxes towards general relativity in matter dominated and potential dominated regimes for scalar-(curvature)tensor and scalar-torsion gravities. Second part summarizes the radius dependence of the gravitational “constant” around a point mass in the parametrized post-Newtonian formalism for scalar-tensor and multiscalar-tensor gravity.http://www.mdpi.com/2218-1997/3/2/37scalar-tensor gravitymultiscalar-tensor gravityscalar-torsion gravityparametrized post-Newtonian formalismcosmologyeffective Newton’s constant
spellingShingle Laur Järv
Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities
Universe
scalar-tensor gravity
multiscalar-tensor gravity
scalar-torsion gravity
parametrized post-Newtonian formalism
cosmology
effective Newton’s constant
title Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities
title_full Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities
title_fullStr Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities
title_full_unstemmed Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities
title_short Effective Gravitational “Constant” in Scalar-(Curvature)Tensor and Scalar-Torsion Gravities
title_sort effective gravitational constant in scalar curvature tensor and scalar torsion gravities
topic scalar-tensor gravity
multiscalar-tensor gravity
scalar-torsion gravity
parametrized post-Newtonian formalism
cosmology
effective Newton’s constant
url http://www.mdpi.com/2218-1997/3/2/37
work_keys_str_mv AT laurjarv effectivegravitationalconstantinscalarcurvaturetensorandscalartorsiongravities