Cosmic growth signatures of modified gravitational strength

Mikhail Denissenya, Eric V. Linder

Research output: Contribution to journalArticlepeer-review

5 Citations (Scopus)


Cosmic growth of large scale structure probes the entire history of cosmic expansion and gravitational coupling. To get a clear picture of the effects of modification of gravity we consider a deviation in the coupling strength (effective Newton's constant) at different redshifts, with different durations and amplitudes. We derive, analytically and numerically, the impact on the growth rate and growth amplitude. Galaxy redshift surveys can measure a product of these through redshift space distortions and we connect the modified gravity to the observable in a way that may provide a useful parametrization of the ability of future surveys to test gravity. In particular, modifications during the matter dominated era can be treated by a single parameter, the ''area'' of the modification, to an accuracy of ∼0.3% in the observables. We project constraints on both early and late time gravity for the Dark Energy Spectroscopic Instrument and discuss what is needed for tightening tests of gravity to better than 5% uncertainty.

Original languageEnglish
Article number030
JournalJournal of Cosmology and Astroparticle Physics
Issue number6
Publication statusPublished - Jun 15 2017


  • Galaxy clustering
  • modified gravity
  • redshift surveys

ASJC Scopus subject areas

  • Astronomy and Astrophysics

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