No Run Gravity[Article]

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dc.contributor.authorLinder, Eric V.
dc.date.accessioned2019-07-19T05:56:40Z
dc.date.available2019-07-19T05:56:40Z
dc.date.issued2019-03-05
dc.descriptionEnergetic Cosmos Laboratory. ECL Publication, 2019en_US
dc.description.abstractConsidering 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.en_US
dc.identifier.citationLinder, E.V. (2019). No Run Gravity. The 2nd international conference of the Energetic Cosmos Laboratory (ECL) at Nazarbayev University. Retrieved from https://arxiv.org/pdf/1903.02010.pdfen_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/4018
dc.language.isoenen_US
dc.publisherNURIS; Energetic Cosmos Laboratoryen_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectThe 2nd international conference of the Energetic Cosmos Laboratory (ECL)en_US
dc.subjectEnergetic Cosmos Laboratory (ECL)en_US
dc.subjectECL19en_US
dc.titleNo Run Gravity[Article]en_US
dc.typeArticleen_US
workflow.import.sourcescience

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