Non-minimal derivative coupling theories compatible with GW170817

In this work we aim to revive the interest for non-minimal derivative coupling theories of gravity, in light of the GW170817 event. These theories include a string motivated non-minimal kinetic term for the scalar field of the form ∼ξ(ϕ)Gμν∂μϕ∂νϕ and predict that the primordial tensor perturbations...

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Main Author: V.K. Oikonomou
Format: Article
Language:English
Published: Elsevier 2024-03-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321324000336
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author V.K. Oikonomou
author_facet V.K. Oikonomou
author_sort V.K. Oikonomou
collection DOAJ
description In this work we aim to revive the interest for non-minimal derivative coupling theories of gravity, in light of the GW170817 event. These theories include a string motivated non-minimal kinetic term for the scalar field of the form ∼ξ(ϕ)Gμν∂μϕ∂νϕ and predict that the primordial tensor perturbations have a speed that it is distinct from the speed of light. Due to the fact that the Universe is classical during and in the post-inflationary epoch, there is no fundamental reason for the graviton to change its mass, the GW170817 event severely constrained these theories. We analyze and formalize the inflationary phenomenology of these theories, using both the latest Planck data and the GW170817 event data to constrain these theories. Due to the fact that there is no constraint in the choice of the scalar potential and the non-minimal coupling function, we provide several classes of viable models, using convenient forms of the minimal coupling function in terms of the scalar potential, aiming for analyticity, and we discuss the advantages and disadvantages of each viable model.
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spelling doaj.art-1a15c53315c54150a0c9ae6d9313776c2024-03-06T05:25:28ZengElsevierNuclear Physics B0550-32132024-03-011000116467Non-minimal derivative coupling theories compatible with GW170817V.K. Oikonomou0Department of Physics, Aristotle University of Thessaloniki, Thessaloniki 54124, Greece; L.N. Gumilyov Eurasian National University, Astana, 010008, KazakhstanIn this work we aim to revive the interest for non-minimal derivative coupling theories of gravity, in light of the GW170817 event. These theories include a string motivated non-minimal kinetic term for the scalar field of the form ∼ξ(ϕ)Gμν∂μϕ∂νϕ and predict that the primordial tensor perturbations have a speed that it is distinct from the speed of light. Due to the fact that the Universe is classical during and in the post-inflationary epoch, there is no fundamental reason for the graviton to change its mass, the GW170817 event severely constrained these theories. We analyze and formalize the inflationary phenomenology of these theories, using both the latest Planck data and the GW170817 event data to constrain these theories. Due to the fact that there is no constraint in the choice of the scalar potential and the non-minimal coupling function, we provide several classes of viable models, using convenient forms of the minimal coupling function in terms of the scalar potential, aiming for analyticity, and we discuss the advantages and disadvantages of each viable model.http://www.sciencedirect.com/science/article/pii/S0550321324000336
spellingShingle V.K. Oikonomou
Non-minimal derivative coupling theories compatible with GW170817
Nuclear Physics B
title Non-minimal derivative coupling theories compatible with GW170817
title_full Non-minimal derivative coupling theories compatible with GW170817
title_fullStr Non-minimal derivative coupling theories compatible with GW170817
title_full_unstemmed Non-minimal derivative coupling theories compatible with GW170817
title_short Non-minimal derivative coupling theories compatible with GW170817
title_sort non minimal derivative coupling theories compatible with gw170817
url http://www.sciencedirect.com/science/article/pii/S0550321324000336
work_keys_str_mv AT vkoikonomou nonminimalderivativecouplingtheoriescompatiblewithgw170817