Built on

M. Lagos, M. Fishbach, P. Landry, D.E. Holz, Standard sirens with a running Planck mass, arXiv:1901.03321
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1901
Earlier work this paper cites.
P.G. Ferreira, Cosmological Tests of Gravity, arXiv:1902.10503
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E.V. Linder, Cosmic Growth History and Expansion History, Phys. Rev. D 72, 043529 (2005) [arXiv:astro-ph/0507263]
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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]
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2010
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Similar

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]
Original
2016
Cited alongside, same era.
B.P. Abbott et al., Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A, Astrophys. J. Lett. 848, L13 (2017) [arXiv:1710.05834]
Original
2017
Cited alongside, same era.
M. Denissenya, E.V. Linder, Subpercent Accurate Fitting of Modified Gravity Growth, JCAP 1711, 052 (2017) [arXiv:1709.08709]
Original
2017
Cited alongside, same era.
E.V. Linder, Cosmic Growth and Expansion Conjoined, Astropart. Phys. 86, 41 (2017) [arXiv:1610.05321]

Then

E. da Cunha et al, The Taipan Galaxy Survey: Scientific Goals and Observing Strategy, PASA 34, 47 (2017) [arXiv:1706.01246]
Original
2017
Later among the works it cites.
A. Nishizawa, Generalized framework for testing gravity with gravitational-wave propagation. I. Formulation, Phys. Rev. D 97, 104037 (2018) [arXiv:1710.04825]
Original
2018
Later among the works it cites.
E.V. Linder, No Slip Gravity, JCAP 1803, 005 (2018) [arXiv:1801.01503]
Original
2018
Later among the works it cites.
L. Amendola, M. Kunz, I.D. Saltas, I. Sawicki, The fate of large-scale structure in modified gravity after GW170817 and GRB170817A, Phys. Rev. Lett. 120, 131101 (2018) [arXiv:1711.04825]
Original
2018
Later among the works it cites.
S. Appleby, E.V. Linder, The Well-Tempered Cosmological Constant, JCAP 1807, 034 (2018) [arXiv:1805.00470]

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2019

No Run Gravity

Linder, Eric V.

Understand

Considering the dark energy/gravity landscape if next generation surveys of galaxies, cosmic microwave background radiation, and gravitational waves do not find clear modification of gravity, we develop No Run Gravity as a counterexample to the conclusion that this would imply general relativity with an expansion history described by an equation of state $w(z)$.

No Run Gravity is a cubic Horndeski theory with a constant Planck mass, no gravitational slip, and no modification of gravitational waves, but a rich phenomenology beyond $w(z)$.
We calculate the evolution of gravitational strength, sound speed, and cosmic growth within the theory and project sensitivities for upcoming DESI redshift space distortion data.