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Original
1952
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1974
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1981
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I. Smail, R. S. Ellis, and M. J. Fitchett, “Gravitational lensing of distant field galaxies by rich clusters: I. - faint galaxy redshift distributions,” Mon. Not. Roy. Astron. Soc
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Original
2013
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2013
Cited alongside, same era.
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Original
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Then

I. Sawicki and E. Bellini, “Limits of quasistatic approximation in modified-gravity cosmologies,” Phys. Rev
Original
2015
Later among the works it cites.
F. Sbisà, “Classical and quantum ghosts,” Eur.J.Phys
Original
2015
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L. Perenon, F. Piazza, C. Marinoni, et al
Original
2015
Later among the works it cites.
M. Kilbinger, “Cosmology with cosmic shear observations: a review,” Rept. Prog. Phys
Original
2015
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É. Aubourg et al
Original
2015
Later among the works it cites.

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2017

Parametrizing modified gravity for cosmological surveys

Gleyzes, Jérôme

Understand

One of the challenges in testing gravity with cosmology is the vast freedom opened when extending General Relativity.

For linear perturbations, one solution consists in using the Effective Field Theory of Dark Energy (EFT of DE).
Even then, the theory space is described in terms of a handful of free functions of time.
This needs to be reduced to a finite number of parameters to be practical for cosmological surveys.

Built on

J. Gleyzes, D. Langlois, F. Piazza, et al
Original
1952
Earlier work this paper cites.
G. W. Horndeski, “Second-order scalar-tensor field equations in a four-dimensional space,” Int.J.Theor.Phys
1974
Earlier work this paper cites.
S. Appleby and E. V. Linder, “The Paths of Gravity in Galileon Cosmology,” JCAP
Original
1981
Earlier work this paper cites.
I. Smail, R. S. Ellis, and M. J. Fitchett, “Gravitational lensing of distant field galaxies by rich clusters: I. - faint galaxy redshift distributions,” Mon. Not. Roy. Astron. Soc
1994
Earlier work this paper cites.
W. Hu, “Power spectrum tomography with weak lensing,” Astrophys. J
1999
Earlier work this paper cites.
C. Armendariz-Picon, V. F. Mukhanov, and P. J. Steinhardt, “A Dynamical solution to the problem of a small cosmological constant and late time cosmic acceleration,” Phys.Rev.Lett
2000
Earlier work this paper cites.
A. Lewis, A. Challinor, and A. Lasenby, “Efficient computation of CMB anisotropies in closed FRW models,” Astrophys. J
2000
Earlier work this paper cites.
R. P. Woodard, “Avoiding dark energy with 1/r modifications of gravity,” Lect.Notes Phys
2007
Earlier work this paper cites.
A. Amara and A. Refregier, “Optimal Surveys for Weak Lensing Tomography,” Mon. Not. Roy. Astron. Soc
2007
Earlier work this paper cites.
B. Joachimi, P. Schneider, and T. Eifler, “Analysis of two-point statistics of cosmic shear. 3. Covariances of shear measures made easy,” Astron. Astrophys
Original
2008
Earlier work this paper cites.
C. Deffayet, G. Esposito-Farese, and A. Vikman, “Covariant Galileon,” Phys.Rev
Original
2009
Earlier work this paper cites.
C. Deffayet, O. Pujolas, I. Sawicki, et al
Original
2010
Earlier work this paper cites.
L. Verde, “Statistical methods in cosmology,” Lect. Notes Phys
Original
2010
Earlier work this paper cites.
J. E. Geach et al
Original
2010
Earlier work this paper cites.
T. Giannantonio, C. Porciani, J. Carron, et al
Original
2012
Earlier work this paper cites.