No slip gravity

dc.contributor.authorLinder, Eric V.
dc.contributor.authorLinder, Eric V.
dc.date.accessioned2025-08-19T09:15:10Z
dc.date.available2025-08-19T09:15:10Z
dc.date.issued2018-03-05
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, Gmatter and Glight, 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.
dc.identifier.doi10.1088/1475-7516/2018/03/005
dc.identifier.issn1475-7516
dc.identifier.otherFilename:10.1088_1475-7516_2018_03_005.pdf
dc.identifier.urihttps://doi.org/10.1088/1475-7516/2018/03/005
dc.identifier.urihttps://nur.nu.edu.kz/handle/123456789/9448
dc.language.isoen
dc.publisherIOP Publishing
dc.relation.ispartofJournal of Cosmology and Astroparticle Physicsen
dc.sourceJournal of Cosmology and Astroparticle Physics, 2018(03), 005-005, (2018)en
dc.subjectmodified gravity, cosmological parameters from LSS, dark energy theory, galaxy clustering
dc.titleNo slip gravityen
dc.typeJournal Articleen

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