Disformal transformations on the CMB

In this work we study the role of disformal transformation on cosmological backgrounds and its relation to the speed of sound for tensor modes. A speed different from one for tensor modes can arise in several contexts, such as Galileons theories or massive gravity, nevertheless the speed is very con...

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Main Authors: Burrage, Clare, Cespedes, Sebastian, Davis, Anne-Christine
Format: Article
Published: IOPScience 2016
Online Access:https://eprints.nottingham.ac.uk/39508/
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author Burrage, Clare
Cespedes, Sebastian
Davis, Anne-Christine
author_facet Burrage, Clare
Cespedes, Sebastian
Davis, Anne-Christine
author_sort Burrage, Clare
building Nottingham Research Data Repository
collection Online Access
description In this work we study the role of disformal transformation on cosmological backgrounds and its relation to the speed of sound for tensor modes. A speed different from one for tensor modes can arise in several contexts, such as Galileons theories or massive gravity, nevertheless the speed is very constrained to be one by observations of gravitational wave emission. It has been shown that in inflation a disformal trans- formation allows to set the speed for tensor modes to one without making changes to the curvature power spectrum. Here we show that this invariance does not hold when considering the CMB anisotropy power spectrum. It turns out that the after doing the transformation there is an imprint on the acoustic peaks and the diffusion damping. This has interesting consequences; here we explore quartic galileon theories which allow a modified speed for tensor modes. For these theories the transformation can be used to constraint the parameter space in different regimes
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spelling nottingham-395082020-05-04T18:07:10Z https://eprints.nottingham.ac.uk/39508/ Disformal transformations on the CMB Burrage, Clare Cespedes, Sebastian Davis, Anne-Christine In this work we study the role of disformal transformation on cosmological backgrounds and its relation to the speed of sound for tensor modes. A speed different from one for tensor modes can arise in several contexts, such as Galileons theories or massive gravity, nevertheless the speed is very constrained to be one by observations of gravitational wave emission. It has been shown that in inflation a disformal trans- formation allows to set the speed for tensor modes to one without making changes to the curvature power spectrum. Here we show that this invariance does not hold when considering the CMB anisotropy power spectrum. It turns out that the after doing the transformation there is an imprint on the acoustic peaks and the diffusion damping. This has interesting consequences; here we explore quartic galileon theories which allow a modified speed for tensor modes. For these theories the transformation can be used to constraint the parameter space in different regimes IOPScience 2016-08-11 Article PeerReviewed Burrage, Clare, Cespedes, Sebastian and Davis, Anne-Christine (2016) Disformal transformations on the CMB. Journal of Cosmology and Astroparticle Physics, 2016 . ISSN 1475-7516 http://iopscience.iop.org/article/10.1088/1475-7516/2016/08/024/meta doi:10.1088/1475-7516/2016/08/024 doi:10.1088/1475-7516/2016/08/024
spellingShingle Burrage, Clare
Cespedes, Sebastian
Davis, Anne-Christine
Disformal transformations on the CMB
title Disformal transformations on the CMB
title_full Disformal transformations on the CMB
title_fullStr Disformal transformations on the CMB
title_full_unstemmed Disformal transformations on the CMB
title_short Disformal transformations on the CMB
title_sort disformal transformations on the cmb
url https://eprints.nottingham.ac.uk/39508/
https://eprints.nottingham.ac.uk/39508/
https://eprints.nottingham.ac.uk/39508/