No Run Gravity
arXiv:1903.02010 · doi:10.1088/1475-7516/2019/07/034
Abstract
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 . 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 . 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.
8 pages, 6 figures
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- Self-tuning kinetic gravity braiding: Cosmological dynamics, shift symmetry, and the tadpole
- Singling out modified gravity parameters and datasets reveals a dichotomy between Planck and lensing
- Stealth black hole perturbations in kinetic gravity braiding
- Gravitational wave signatures from dark sector interactions
- A Bright Future? Prospects for Cosmological Tests of GR with Multimessenger Gravitational Wave Events
- New measures to test modified gravity cosmologies