Model-independent constraints on dark energy and modified gravity with the SKA

Gong-Bo Zhao, David Bacon, Roy Maartens, Mario Santos, Alvise Raccanelli

Research output: Chapter in Book/Report/Conference proceedingConference contribution

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Abstract

Employing a nonparametric approach of the principal component analysis (PCA), we forecast the future constraint on the equation of state w(z) of dark energy, and on the effective Newton constant µ(k, z), which parameterise the effect of modified gravity, using the planned SKA HI galaxy survey. Combining with the simulated data of Planck and Dark Energy Survey (DES), we find that SKA Phase 1 (SKA1) and SKA Phase 2 (SKA2) can well constrain 3 and 5 eigenmodes of w(z) respectively. The errors of the best measured modes can be reduced to 0.04 and 0.023 for SKA1 and SKA2 respectively, making it possible to probe dark energy dynamics. On the other hand, SKA1 and SKA2 can constrain 7 and 20 eigenmodes of µ(k, z) respectively within 10% sensitivity level. Furthermore, 2 and 7 modes can be constrained within sub percent level using SKA1 and SKA2 respectively. This is a significant improvement compared to the combined
datasets without SKA.
Original languageEnglish
Title of host publicationAdvancing Astrophysics with the Square Kilometre Array
PublisherProceedings of Science
Publication statusPublished - 15 Jan 2015
EventAdvancing Astrophysics with the Square Kilometre Array - Giardini Naxos, Italy
Duration: 9 Jun 201413 Jun 2014

Conference

ConferenceAdvancing Astrophysics with the Square Kilometre Array
CountryItaly
CityGiardini Naxos
Period9/06/1413/06/14

Keywords

  • astro-ph.CO
  • RCUK
  • STFC
  • ST/K0090X/1

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