Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings

The simplest way to modify gravity is to extend the gravitational sector to include an additional scalar degree of freedom. The most general metric that can be built in such a theory includes disformal terms, so that standard model fields move on a metric which is the sum of the space time metric an...

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Main Authors: van de Bruck, Carsten, Burrage, Clare, Morrice, Jack
Format: Article
Published: IOPScience 2016
Online Access:https://eprints.nottingham.ac.uk/42091/
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author van de Bruck, Carsten
Burrage, Clare
Morrice, Jack
author_facet van de Bruck, Carsten
Burrage, Clare
Morrice, Jack
author_sort van de Bruck, Carsten
building Nottingham Research Data Repository
collection Online Access
description The simplest way to modify gravity is to extend the gravitational sector to include an additional scalar degree of freedom. The most general metric that can be built in such a theory includes disformal terms, so that standard model fields move on a metric which is the sum of the space time metric and a tensor constructed from first derivatives of the scalar. In such a theory gravitational waves and photons can propagate at different speeds, and these can in turn be different from the maximum speed limit for matter particles. In this work we show that disformal couplings can cause charged particles to emit Cherenkov radiation and bremsstrahlung apparently in vacuum, depending on the background evolution of the scalar field. We discuss the implications of this for observations of cosmic rays, and the constraints that arise for models of dark energy with disformal couplings.
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spelling nottingham-420912020-05-04T18:08:05Z https://eprints.nottingham.ac.uk/42091/ Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings van de Bruck, Carsten Burrage, Clare Morrice, Jack The simplest way to modify gravity is to extend the gravitational sector to include an additional scalar degree of freedom. The most general metric that can be built in such a theory includes disformal terms, so that standard model fields move on a metric which is the sum of the space time metric and a tensor constructed from first derivatives of the scalar. In such a theory gravitational waves and photons can propagate at different speeds, and these can in turn be different from the maximum speed limit for matter particles. In this work we show that disformal couplings can cause charged particles to emit Cherenkov radiation and bremsstrahlung apparently in vacuum, depending on the background evolution of the scalar field. We discuss the implications of this for observations of cosmic rays, and the constraints that arise for models of dark energy with disformal couplings. IOPScience 2016-08-02 Article PeerReviewed van de Bruck, Carsten, Burrage, Clare and Morrice, Jack (2016) Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings. Journal of Cosmology and Astroparticle Physics, 2016 (08). 003/1-003/16. ISSN 1475-7516 http://iopscience.iop.org/article/10.1088/1475-7516/2016/08/003/meta doi:10.1088/1475-7516/2016/08/003 doi:10.1088/1475-7516/2016/08/003
spellingShingle van de Bruck, Carsten
Burrage, Clare
Morrice, Jack
Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings
title Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings
title_full Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings
title_fullStr Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings
title_full_unstemmed Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings
title_short Vacuum Cherenkov radiation and bremsstrahlung from disformal couplings
title_sort vacuum cherenkov radiation and bremsstrahlung from disformal couplings
url https://eprints.nottingham.ac.uk/42091/
https://eprints.nottingham.ac.uk/42091/
https://eprints.nottingham.ac.uk/42091/