Unified cosmology with scalar–tensor theory of gravity

Abstract Unlike the Noether symmetry, a metric independent general conserved current exists for non-minimally coupled scalar–tensor theory of gravity if the trace of the energy-momentum tensor vanishes. Thus, in the context of cosmology, a symmetry exists both in the early vacuum and radiation domin...

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Main Authors: Behzad Tajahmad, Abhik Kumar Sanyal
Format: Article
Language:English
Published: SpringerOpen 2017-04-01
Series:European Physical Journal C: Particles and Fields
Subjects:
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-4785-x
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author Behzad Tajahmad
Abhik Kumar Sanyal
author_facet Behzad Tajahmad
Abhik Kumar Sanyal
author_sort Behzad Tajahmad
collection DOAJ
description Abstract Unlike the Noether symmetry, a metric independent general conserved current exists for non-minimally coupled scalar–tensor theory of gravity if the trace of the energy-momentum tensor vanishes. Thus, in the context of cosmology, a symmetry exists both in the early vacuum and radiation dominated era. For slow roll, symmetry is sacrificed, but at the end of early inflation, such a symmetry leads to a Friedmann-like radiation era. Late-time cosmic acceleration in the matter dominated era is realized in the absence of symmetry, in view of the same decayed and redshifted scalar field. Thus, unification of early inflation with late-time cosmic acceleration with a single scalar field may be realized.
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spelling doaj.art-373f9938ed5c4a69afb09fbd0202e6662022-12-22T00:49:22ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-04-017741910.1140/epjc/s10052-017-4785-xUnified cosmology with scalar–tensor theory of gravityBehzad Tajahmad0Abhik Kumar Sanyal1Faculty of Physics, University of TabrizDepartment of Physics, Jangipur CollegeAbstract Unlike the Noether symmetry, a metric independent general conserved current exists for non-minimally coupled scalar–tensor theory of gravity if the trace of the energy-momentum tensor vanishes. Thus, in the context of cosmology, a symmetry exists both in the early vacuum and radiation dominated era. For slow roll, symmetry is sacrificed, but at the end of early inflation, such a symmetry leads to a Friedmann-like radiation era. Late-time cosmic acceleration in the matter dominated era is realized in the absence of symmetry, in view of the same decayed and redshifted scalar field. Thus, unification of early inflation with late-time cosmic acceleration with a single scalar field may be realized.http://link.springer.com/article/10.1140/epjc/s10052-017-4785-xScalar FieldCosmic Microwave Background RadiationHubble ParameterDeceleration ParameterDark Energy Model
spellingShingle Behzad Tajahmad
Abhik Kumar Sanyal
Unified cosmology with scalar–tensor theory of gravity
European Physical Journal C: Particles and Fields
Scalar Field
Cosmic Microwave Background Radiation
Hubble Parameter
Deceleration Parameter
Dark Energy Model
title Unified cosmology with scalar–tensor theory of gravity
title_full Unified cosmology with scalar–tensor theory of gravity
title_fullStr Unified cosmology with scalar–tensor theory of gravity
title_full_unstemmed Unified cosmology with scalar–tensor theory of gravity
title_short Unified cosmology with scalar–tensor theory of gravity
title_sort unified cosmology with scalar tensor theory of gravity
topic Scalar Field
Cosmic Microwave Background Radiation
Hubble Parameter
Deceleration Parameter
Dark Energy Model
url http://link.springer.com/article/10.1140/epjc/s10052-017-4785-x
work_keys_str_mv AT behzadtajahmad unifiedcosmologywithscalartensortheoryofgravity
AT abhikkumarsanyal unifiedcosmologywithscalartensortheoryofgravity