The parameterized post-Friedmann framework for theories of modified gravity: Concepts, formalism, and examples

Tessa Baker, Pedro G. Ferreira, and Constantinos Skordis
Phys. Rev. D 87, 024015 – Published 7 January 2013

Abstract

A unified framework for theories of modified gravity will be an essential tool for interpreting the forthcoming deluge of cosmological data. We present such a formalism, the parameterized post-Friedmann framework (PPF), which parameterizes the cosmological perturbation theory of a wide variety of modified gravity models. PPF is able to handle spin-0 degrees of freedom from new scalar, vector, and tensor fields, meaning that it is not restricted to simple models based solely on cosmological scalar fields. A direct correspondence is maintained between the parameterization and the underlying space of theories, which allows us to build up a “dictionary” of modified gravity theories and their PPF correspondences. In this paper we describe the construction of the parameterization and demonstrate its use through a number of worked examples relevant to the current literature. We indicate how the formalism will be implemented numerically, so that the dictionary of modified gravity can be pitted against forthcoming observations.

  • Received 11 September 2012

DOI:https://doi.org/10.1103/PhysRevD.87.024015

© 2013 American Physical Society

Authors & Affiliations

Tessa Baker* and Pedro G. Ferreira

  • Astrophysics, University of Oxford, Denys Wilkinson Building, Keble Road, Oxford, OX1 3RH, United Kingdom

Constantinos Skordis

  • School of Physics and Astronomy, University of Nottingham, University Park, Nottingham, NG7 2RD, United Kingdom

  • *tessa.baker@astro.ox.ac.uk
  • p.ferreira1@physics.ox.ac.uk
  • skordis@nottingham.ac.uk

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Issue

Vol. 87, Iss. 2 — 15 January 2013

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