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C. Deffayet, O. Pujolas, I. Sawicki, A. Vikman, Imperfect Dark Energy from Kinetic Gravity Braiding, JCAP 1010, 026 (2010) [arXiv:1008.0048]
Original
2010
Earlier work this paper cites.
A. de Felice, T. Kobayashi, S. Tsujikawa, Effective gravitational couplings for cosmological perturbations in the most general scalar-tensor theories with second-order field equations, Phys. Lett. B 706, 123 (2011) [arXiv:1108.4242]
Original
2011
Earlier work this paper cites.
F. Beutler et al., The 6dF Galaxy Survey: z ≈ 0 z\approx 0 measurements of the growth rate and σ 8 \sigma_{8} , Mon. Not. R. Astron. Soc. 423, 3430 (2012) [arXiv:1204.4725]
Original
2012
Earlier work this paper cites.
C. Blake et al., The WiggleZ Dark Energy Survey: Joint measurements of the expansion and growth history at z < 1 z<1 , Mon. Not. R. Astron. Soc. 425, 405 (2012) [arXiv:1204.3674]
Original
2012
Earlier work this paper cites.
L. Amendola, M. Kunz, M. Motta, I.D. Saltas, I. Sawicki, Observables and unobservables in dark energy cosmologies, Phys. Rev. D 87, 023501 (2013) [arXiv:1210.0439]
Original
2013
Earlier work this paper cites.
M. Motta, I. Sawicki, I.D. Saltas, L. Amendola, M. Kunz, Probing Dark Energy through Scale Dependence, Phys. Rev. D 88, 124035 (2013) [arXiv:1305.0008]
Original
2013
Earlier work this paper cites.
G. Gubitosi, F. Piazza, F. Vernizzi, The effective field theory of dark energy, JCAP 1302, 032 (2013) [arXiv:1210.0201]
Original
2013
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C. Blake et al., Galaxy And Mass Assembly (GAMA): improved cosmic growth measurements using multiple tracers of large-scale structure, Mon. Not. R. Astron. Soc. 436, 3089 (2013) [arXiv:1309.5556]
Original
2013
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S. de la Torre et al., The VIMOS Public Extragalactic Redshift Survey (VIPERS). Galaxy clustering and redshift-space distortions at z ≈ 0.8 z\approx 0.8 in the first data release, Astron. Astroph. 557, 54 (2013) [arXiv:1303.2622]
Original
2013
Earlier work this paper cites.
I.D. Saltas, I. Sawicki, L. Amendola, M. Kunz, Anisotropic stress as signature of non-standard propagation of gravitational waves, Phys. Rev. Lett. 113, 191101 (2014) [arXiv:1406.7139]
Original
2014
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E.V. Linder, Are Scalar and Tensor Deviations Related in Modified Gravity?, Phys. Rev. D 90, 083536 (2014) [arXiv:1407.8184]
Original
2014
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Similar

E. Bellini, I. Sawicki, Maximal freedom at minimum cost: linear large-scale structure in general modifications of gravity, JCAP 1407, 050 (2014) [arXiv:1404.3713]
Original
2014
Cited alongside, same era.
J. Gleyzes, D. Langlois, F. Vernizzi, A unifying description of dark energy, Int. J. Mod. Phys. D 23, 1443010 (2014) [arXiv:1411.3712]
Original
2014
Cited alongside, same era.
I. Sawicki, E. Bellini, Limits of Quasi-Static Approximation in Modified-Gravity Cosmologies, Phys. Rev. D 92, 084061 (2015) [arXiv:1503.06831]
Original
2015
Cited alongside, same era.
L. Lombriser, A. Taylor, Breaking a Dark Degeneracy with Gravitational Waves, JCAP 1603, 031 (2016) [arXiv:1509.08458]
Original
2016
Cited alongside, same era.
E.V. Linder, G. Sengör, S. Watson, Is the Effective Field Theory of Dark Energy Effective?, JCAP 1605, 053 (2016) [arXiv:1512.06180]

Then

I. Sawicki, I.D. Saltas, M. Motta, L. Amendola, M. Kunz, Non-standard gravitational waves imply gravitational slip: on the difficulty of partially hiding new gravitational degrees of freedom, Phys. Rev. D 95, 083520 (2017) [arXiv:1612.02002]
Original
2017
Later among the works it cites.
M. Zumalacárregui, E. Bellini. I. Sawicki, J. Lesgourgues, P.G. Ferreira, hi_class: Horndeski in the Cosmic Linear Anisotropy Solving System, JCAP 1708, 019 (2017) [arXiv:1605.06102]
Original
2017
Later among the works it cites.
G. D’Amico, Z. Huang, M. Mancarella, F. Vernizzi, Weakening gravity on redshift-survey scales with kinetic matter mixing, JCAP 1702, 014 (2017) [arXiv:1609.01272]
Original
2017
Later among the works it cites.
M. Denissenya, E.V. Linder, Subpercent Accurate Fitting of Modified Gravity Growth, JCAP 1711, 052 (2017) [arXiv:1709.08709]
Original
2017
Later among the works it cites.

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2018

No Slip Gravity

Linder, Eric V.

Understand

A subclass of the Horndeski modified gravity theory we call No Slip Gravity has particularly interesting properties: 1) a speed of gravitational wave propagation equal to the speed of light, 2) equality between the effective gravitational coupling strengths to matter and light, $G_{\rm matter}$ and $G_{\rm light}$, hence no slip between the metric potentials, yet difference from Newton's constant, and 3) suppressed growth to give better agreement with galaxy clustering observations.

We explore the characteristics and implications of this theory, and project observational constraints.
We also give a simple expression for the ratio of the gravitational wave standard siren distance to the photon standard candle distance, in this theory and others, and enable a direct comparison of modified gravity in structure growth and in gravitational waves, an important crosscheck.