Disformal dark energy at colliders

Disformally coupled, light scalar fields arise in many of the theories of dark energy and modified gravity that attempt to explain the accelerated expansion of the Universe. They have proved difficult to constrain with precision tests of gravity because they do not give rise to fifth forces around s...

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Main Authors: Brax, Philippe, Burrage, Clare, Englert, Christoph
Format: Article
Published: American Physical Society 2015
Online Access:https://eprints.nottingham.ac.uk/42094/
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author Brax, Philippe
Burrage, Clare
Englert, Christoph
author_facet Brax, Philippe
Burrage, Clare
Englert, Christoph
author_sort Brax, Philippe
building Nottingham Research Data Repository
collection Online Access
description Disformally coupled, light scalar fields arise in many of the theories of dark energy and modified gravity that attempt to explain the accelerated expansion of the Universe. They have proved difficult to constrain with precision tests of gravity because they do not give rise to fifth forces around static nonrelativistic sources. However, because the scalar field couples derivatively to standard model matter, measurements at high-energy particle colliders offer an effective way to constrain and potentially detect a disformally coupled scalar field. Here we derive new constraints on the strength of the disformal coupling from LHC run 1 data and provide a forecast for the improvement of these constraints from run 2. We additionally comment on the running of disformal and standard model couplings in this scenario under the renormalization group flow.
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spelling nottingham-420942020-05-04T17:14:48Z https://eprints.nottingham.ac.uk/42094/ Disformal dark energy at colliders Brax, Philippe Burrage, Clare Englert, Christoph Disformally coupled, light scalar fields arise in many of the theories of dark energy and modified gravity that attempt to explain the accelerated expansion of the Universe. They have proved difficult to constrain with precision tests of gravity because they do not give rise to fifth forces around static nonrelativistic sources. However, because the scalar field couples derivatively to standard model matter, measurements at high-energy particle colliders offer an effective way to constrain and potentially detect a disformally coupled scalar field. Here we derive new constraints on the strength of the disformal coupling from LHC run 1 data and provide a forecast for the improvement of these constraints from run 2. We additionally comment on the running of disformal and standard model couplings in this scenario under the renormalization group flow. American Physical Society 2015-08-20 Article PeerReviewed Brax, Philippe, Burrage, Clare and Englert, Christoph (2015) Disformal dark energy at colliders. Physical Review D, D92 (4). 044036/1-044036/11. ISSN 2470-0029 https://journals.aps.org/prd/abstract/10.1103/PhysRevD.92.044036 doi:10.1103/PhysRevD.92.044036 doi:10.1103/PhysRevD.92.044036
spellingShingle Brax, Philippe
Burrage, Clare
Englert, Christoph
Disformal dark energy at colliders
title Disformal dark energy at colliders
title_full Disformal dark energy at colliders
title_fullStr Disformal dark energy at colliders
title_full_unstemmed Disformal dark energy at colliders
title_short Disformal dark energy at colliders
title_sort disformal dark energy at colliders
url https://eprints.nottingham.ac.uk/42094/
https://eprints.nottingham.ac.uk/42094/
https://eprints.nottingham.ac.uk/42094/