Built on

H. Cramér, Mathematical methods of statistic, §32.3 (Princeton U. Press: 1946); M. Kendall and A. Stuart, Advanced Theory of Statistics, 4th ed., §17 (Oxford U. Press: 1979)
1979
Earlier work this paper cites.
L. Knox, R. Scoccimarro, S. Dodelson, The Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy, Phys. Rev. Lett. 81, 2004 (1998) [arXiv:astro-ph/9805012]
1998
Earlier work this paper cites.
G. Dvali, G. Gabadadze, M. Porrati, 4D Gravity on a Brane in 5D Minkowski Space, Phys. Lett. B 485, 208 (2000) [arXiv:hep-th/0005016]
2000
Earlier work this paper cites.
C. Deffayet, G. Dvali, G. Gabadadze, Accelerated Universe from Gravity Leaking to Extra Dimensions, Phys. Rev. D 65, 044023 (2002) [arXiv:astro-ph/0105068]
2002
Earlier work this paper cites.
P. Zhang, Testing Gravity Against Early Time Integrated Sachs-Wolfe Effect, Phys. Rev. D 73, 123504 (2006) [arXiv:astro-ph/0511218]
2006
Earlier work this paper cites.
E.V. Linder, Biased Cosmology: Pivots, Parameters, and Figures of Merit, Astropart. Phys. 26, 102 (2006) [arXiv:astro-ph/0604280]
2006
Earlier work this paper cites.
S. Dodelson, C. Shapiro, M. White, Reduced Shear Power Spectrum, Phys. Rev. D 73, 023009 (2006) [arXiv:astro-ph/0508296]
2006
Earlier work this paper cites.
W. Hu and I. Sawicki, Models of f ⁡ ( R ) f(R) Cosmic Acceleration that Evade Solar-System Tests, Phys. Rev. D 76, 064004 (2007) [arXiv:0705.1158]
Original
2007
Earlier work this paper cites.

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A. Joyce, B. Jain, J. Khoury, M. Trodden, Beyond the Cosmological Standard Model, Phys. Rept. 568, 1 (2015) [arXiv:1407.0059]
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2017

Subpercent Accurate Fitting of Modified Gravity Growth

Denissenya, Mikhail, Linder, Eric V.

Understand

Adding to our previous method for dealing with gravitational modifications at redshift $z\gtrsim3$ through a single parameter, we investigate treatment of lower redshift modifications to linear growth observables.

We establish subpercent accurate fits to the redshift space distortion observable $f\sigma_8(a)$ using two parameters binned in redshift, testing the results for modifications with time dependence that rises, falls, is nonmonotonic, is multipeaked, and corresponds to $f(R)$ and braneworld gravity.
The residuals are then propagated to cosmological parameter biases for DESI observations, and found to cause a shift in the dark energy joint confidence contour by less than the equivalent of $\sim0.1\sigma$.
The proposed 2--3 parameter modified gravity description also can reveal physical characteristics of the underlying theory.

Built on

H. Cramér, Mathematical methods of statistic, §32.3 (Princeton U. Press: 1946); M. Kendall and A. Stuart, Advanced Theory of Statistics, 4th ed., §17 (Oxford U. Press: 1979)
1979
Earlier work this paper cites.
L. Knox, R. Scoccimarro, S. Dodelson, The Impact of Inhomogeneous Reionization on Cosmic Microwave Background Anisotropy, Phys. Rev. Lett. 81, 2004 (1998) [arXiv:astro-ph/9805012]
1998
Earlier work this paper cites.
G. Dvali, G. Gabadadze, M. Porrati, 4D Gravity on a Brane in 5D Minkowski Space, Phys. Lett. B 485, 208 (2000) [arXiv:hep-th/0005016]
2000
Earlier work this paper cites.
C. Deffayet, G. Dvali, G. Gabadadze, Accelerated Universe from Gravity Leaking to Extra Dimensions, Phys. Rev. D 65, 044023 (2002) [arXiv:astro-ph/0105068]
2002
Earlier work this paper cites.
P. Zhang, Testing Gravity Against Early Time Integrated Sachs-Wolfe Effect, Phys. Rev. D 73, 123504 (2006) [arXiv:astro-ph/0511218]
2006
Earlier work this paper cites.
E.V. Linder, Biased Cosmology: Pivots, Parameters, and Figures of Merit, Astropart. Phys. 26, 102 (2006) [arXiv:astro-ph/0604280]
2006
Earlier work this paper cites.
S. Dodelson, C. Shapiro, M. White, Reduced Shear Power Spectrum, Phys. Rev. D 73, 023009 (2006) [arXiv:astro-ph/0508296]
2006
Earlier work this paper cites.
W. Hu and I. Sawicki, Models of f ⁡ ( R ) f(R) Cosmic Acceleration that Evade Solar-System Tests, Phys. Rev. D 76, 064004 (2007) [arXiv:0705.1158]
Original
2007
Earlier work this paper cites.