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P. G. Ferreira, Cosmological tests of gravity, Annual Review of Astronomy and Astrophysics 57
Original
1902
Earlier work this paper cites.
A. G. Kim et al. , Testing Gravity Using Type Ia Supernovae Discovered by Next-Generation Wide-Field Imaging Surveys, Bull. Am. Astron. Soc. 51
Original
1903
Earlier work this paper cites.
C. Garcia-Quintero, M. Ishak, L. Fox, and J. Dossett, Testing deviations from GR at cosmological scales including dynamical dark energy, massive neutrinos, functional or binned parametrizations, and spatial curvature, Physical Review D 100
Original
1908
Earlier work this paper cites.
A. G. Kim and E. V. Linder, Complementarity of Peculiar Velocity Surveys and Redshift Space Distortions for Testing Gravity, Phys. Rev. D 101
Original
1911
Earlier work this paper cites.
L. Guzzo et al. , A test of the nature of cosmic acceleration using galaxy redshift distortions, Nature 451
Original
1944
Earlier work this paper cites.
Y. Zheng, Robustness of the pairwise kinematic Sunyaev–Zel’dovich power spectrum shape as a cosmological gravity probe, The Astrophysical Journal 904
Original
2001
Earlier work this paper cites.
C. Blake et al. , Testing gravity using galaxy-galaxy lensing and clustering amplitudes in KiDS-1000, BOSS, and 2dflens, Astron. Astrophys. 642
Original
2005
Earlier work this paper cites.
S.-F. Chen, Z. Vlah, and M. White, Consistent modeling of velocity statistics and redshift-space distortions in one-loop perturbation theory, Journal of Cosmology and Astroparticle Physics 2020
Original
2005
Earlier work this paper cites.
P. Zhang, Testing gravity against the early time integrated Sachs–Wolfe effect, Physical Review D 73
2006
Earlier work this paper cites.
R. Bean, D. Bernat, L. Pogosian, A. Silvestri, and M. Trodden, Dynamics of linear perturbations in f ⁡ ( r ) f(r) gravity, Physical Review D 75
2007
Earlier work this paper cites.
W. Hu and I. Sawicki, Models of f ⁡ ( r ) f(r) cosmic acceleration that evade solar-system tests, Physical Review D 76
Original
2007
Earlier work this paper cites.
Y. Zhang et al. , Testing general relativity on cosmological scales at redshift z z ∼ \sim 1.5 with quasar and CMB lensing, Monthly Notices of the Royal Astronomical Society 501
Original
2007
Earlier work this paper cites.
E. V. Linder, Redshift distortions as a probe of gravity, Astroparticle Physics 29
Original
2008
Earlier work this paper cites.
V. Acquaviva, A. Hajian, D. N. Spergel, and S. Das, Next generation redshift surveys and the origin of cosmic acceleration, Physical Review D 78
Original
2008
Earlier work this paper cites.
L. Pogosian and A. Silvestri, Pattern of growth in viable f ⁡ ( r ) f(r) cosmologies, Phys. Rev. D 77
Original
2008
Earlier work this paper cites.

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2022

Constraining Scale Dependent Growth with Redshift Surveys

Denissenya, Mikhail, Linder, Eric V.

Understand

Ongoing and future redshift surveys have the capability to measure the growth rate of large scale structure at the percent level over a broad range of redshifts, tightly constraining cosmological parameters.

Beyond general relativity, however, the growth rate in the linear density perturbation regime can be not only redshift dependent but scale dependent, revealing important clues to modified gravity.
We demonstrate that a fully model independent approach of binning the gravitational strength $G_{\rm eff}(k,z)$ matches scalar-tensor results for the growth rate $f\sigma_8(k,z)$ to $0.02\%$-$0.27\%$ rms accuracy.
For data of the quality of the Dark Energy Spectroscopic Instrument (DESI) we find the bin values can be constrained to 1.4\%-28\%.