No Slip Gravity

dc.contributor.authorLinder, Eric V.
dc.date.accessioned2019-07-20T08:02:29Z
dc.date.available2019-07-20T08:02:29Z
dc.date.issued2018-01-04
dc.descriptionEnergetic Cosmos Laboratory. ECL Publicationsen_US
dc.description.abstractA 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 matter and G 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.en_US
dc.identifier.citationLinder, E.V. (2018). No Slip Gravity. The 2nd international conference of the Energetic Cosmos Laboratory (ECL) at Nazarbayev University. Retrieved from https://arxiv.org/pdf/1801.01503.pdfen_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/4031
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.subjectECL19en_US
dc.subjectEnergetic Cosmos Laboratory (ECL)en_US
dc.titleNo Slip Gravityen_US
dc.typeArticleen_US
workflow.import.sourcescience

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