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Cosmological perturbations in generalised dark Lagrangians

Edholm, James; Pearson, Jonathan

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Authors

James Edholm

Jonathan Pearson



Abstract

We describe a new method to parameterise dark energy theories including massive gravity, elastic dark energy and tensor-metric theories. We first examine the existing framework which describes any second order Lagrangian which depends on the variation of the metric and find new constraints on the parameters. We extend the method to Lorentz violating theories which depend on the variation of the time and spatial parts of the metric separately. We show how this can describe massive gravity and elastic dark energy, while ruling out the whole class of theories where the Lagrangian depends only on the variation of the time part of the metric. We further generalise our method to tensor-metric theories, both with and without splitting the metric into time and spatial parts. Our method extends existing physics by providing a mechanism to easily evaluate large classes of dark energy theories.

Citation

Edholm, J., & Pearson, J. (2018). Cosmological perturbations in generalised dark Lagrangians. Journal of High Energy Physics, 2018(11), Article 180. https://doi.org/10.1007/jhep11%282018%29180

Journal Article Type Article
Acceptance Date Nov 22, 2018
Online Publication Date Nov 28, 2018
Publication Date Nov 28, 2018
Deposit Date Jan 4, 2019
Publicly Available Date Jan 4, 2019
Journal Journal of High Energy Physics
Print ISSN 1126-6708
Electronic ISSN 1029-8479
Publisher Scuola Internazionale Superiore di Studi Avanzati (SISSA)
Peer Reviewed Peer Reviewed
Volume 2018
Issue 11
Article Number 180
DOI https://doi.org/10.1007/jhep11%282018%29180
Public URL https://durham-repository.worktribe.com/output/1310719

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Publisher Licence URL
http://creativecommons.org/licenses/by/4.0/

Copyright Statement
This article is distributed under the terms of the Creative Commons Attribution License (CC-BY 4.0), which permits any use, distribution and reproduction in any medium, provided the original author(s) and source are credited.





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