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hi_class: Horndeski in the cosmic linear anisotropy solving system

Abstract:
We present the public version of hi-class (www.hiclass-code.net), an extension of the Boltzmann code CLASS to a broad ensemble of modifications to general relativity. In particular, hi-class can calculate predictions for models based on Horndeski's theory, which is the most general scalar-tensor theory described by second-order equations of motion and encompasses any perfect-fluid dark energy, quintessence, Brans-Dicke, f(R) and covariant Galileon models. hi-class has been thoroughly tested and can be readily used to understand the impact of alternative theories of gravity on linear structure formation as well as for cosmological parameter extraction.
Publication status:
Published
Peer review status:
Peer reviewed

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Publisher copy:
10.1088/1475-7516/2017/08/019

Authors


More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; Astrophysics
Role:
Author
More by this author
Institution:
University of Oxford
Division:
MPLS Division
Department:
Physics; 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:
08
Pages:
019
Publication date:
2017-08-16
Acceptance date:
2017-07-23
DOI:
EISSN:
1475-7516


Keywords:
Pubs id:
pubs:693519
UUID:
uuid:b1e10b22-1259-49b4-b322-2a2a9e727a23
Local pid:
pubs:693519
Source identifiers:
693519
Deposit date:
2018-01-23

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