Cited by 34Cosmology and Gravitation TheoriesNoncommutative and Quantum Gravity TheoriesPulsars and Gravitational Waves Research

Testing gravity with EG: mapping theory onto observations

Open access
Leonard, C. Danielle, Ferreira, Pedro G., Heymans, Catherine·2015·Journal of Cosmology and Astroparticle Physics

Abstract

We present a complete derivation of the observationally motivated definition of the modified gravity statistic E G . Using this expression, we investigate how variations to theory and survey parameters may introduce uncertainty in the general relativistic prediction of E G . We forecast errors on E G for measurements using two combinations of upcoming surveys, and find that theoretical uncertainties may dominate for a futuristic measurement. Finally, we compute predictions of E G under modifications to general relativity in the quasistatic regime, and comment on the pros and cons of using E G to test gravity with future surveys.

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Registry

Crossref · 10.1088/1475-7516/2015/12/051

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  • Leonard et al. (2015) observed a difference between E_G as given by Eq. (111) and E_G as given by Eq. (113).

    “Second, when considering the measure at nonlinear scales, it was observed in Leonard et al. (2015) that there was a difference between as given by Eq. (111) and as given by Eq. (113).”

    From Testing general relativity in cosmology (2019) · cites this paper as Leonard et al. (2015)

  • Leonard et al. attribute the cancellation to nonlinearities entering Upsilon_gm and Upsilon_gg via the same combination of correlation function terms, so they cancel from the ratio.

    “They attribute this to fact that nonlinearities enter into and (i.e., the galaxy-matter and galaxy-galaxy annular differential surface densities) via the same combination of correlation function terms, so they effectively cancel out from the ratio.”

    From Testing general relativity in cosmology (2019) · cites this paper as Leonard et al. (2015)

  • Leonard et al. found that including non-linearities in the correlation function used in E_G does not cause the measure to deviate from the expected GR value at small scales.

    “They found that the inclusion of non-linearities in the correlation function used into do not cause the measure to deviate from the expected GR value at small scales.”

    From Testing general relativity in cosmology (2019) · cites this paper as Leonard et al. (2015)

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References 47 · Cited by 34

Authors
Leonard, C. D., Ferreira, P. G., & Heymans, C.
Affiliations
  • University of Oxford (GB)
  • University of Edinburgh (GB)
Venue
Journal of Cosmology and Astroparticle Physics
Published
2015-12-29
Volume
2015
Issue
12
Pages
051-051
ISSN
  • 1475-7508 (ISSN-L)
  • 1475-7516
OpenAlex
W2192569094
Cited by
34
References
47
Citations by year
2026: 2 · 2025: 1 · 2024: 1 · 2023: 2 · 2021: 4 · 2020: 4 · 2019: 5 · 2018: 7 · 2017: 1 · 2016: 7
FWCI
2.85
Type
journal article
Language
en
Open access
Locations
  • Journal of Cosmology and Astroparticle Physics (publishedVersion)
  • arXiv (Cornell University) (publishedVersion)
  • arXiv (Cornell University)
Funders
  • Natural Sciences and Engineering Research Council of Canada
  • Science and Technology Facilities Council (ST/M001229/1, ST/K00106X/1, ST/J001422/1)
  • H2020 European Research Council (647112)
Topics
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
  • Physical Sciences › Physics and Astronomy › Statistical and Nonlinear Physics › Noncommutative and Quantum Gravity Theories
  • Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Pulsars and Gravitational Waves Research
Keywords
modified gravity, tests of general relativity, large-scale structure

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