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A general theory of linear cosmological perturbations: bimetric theories

Abstract:
We implement the method developed in [1] to construct the most general parametrised action for linear cosmological perturbations of bimetric theories of gravity. Specifically, we consider perturbations around a homogeneous and isotropic background, and identify the complete form of the action invariant under diffeomorphism transformations, as well as the number of free parameters characterising this cosmological class of theories. We discuss, in detail, the case without derivative interactions, and compare our results with those found in massive bigravity.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2017/01/047

Authors


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Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Oriel College
Role:
Author



Publisher:
Institute of Physics
Journal:
Journal of Cosmology and Astroparticle Physics More from this journal
Volume:
2017
Issue:
01
Pages:
047
Publication date:
2017-01-01
Acceptance date:
2017-01-11
DOI:
EISSN:
1475-7516


Keywords:
Pubs id:
pubs:648383
UUID:
uuid:9b5d20b5-4dc6-4b5b-bee1-1a068cf00b0b
Local pid:
pubs:648383
Source identifiers:
648383
Deposit date:
2018-01-23

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