Subpercent Accurate Fitting of Modified Gravity Growth

dc.contributor.authorDenissenya, Mikhail
dc.contributor.authorLinder, Eric V.
dc.date.accessioned2019-07-20T10:41:23Z
dc.date.available2019-07-20T10:41:23Z
dc.date.issued2017-09-25
dc.descriptionEnergetic Cosmos Laboratory. ECL Publicationsen_US
dc.description.abstractAdding to our previous method for dealing with gravitational modifications at redshiftz&3through a single parameter, we investigate treatment of lower redshift modifications to linear growth observables. We establish sub percent accurate fits to the redshift space distortion observablefσ8(a)using two parameters binned in redshift, testing the results for modifications with time dependence that rises, falls, is nonmonotonic, is multipeaked, and corresponds to f(R) and braneworld gravity. The residuals are then propagated to cosmological parameter biases for DESI observations, and found to cause a shift in the dark energy joint confidence contour by less than the equivalent of∼0.1σ. The proposed 2–3 parameter modified gravity description also can reveal physical characteristics of the underlying theory.en_US
dc.identifier.citationDenissenya, M., & Linder, E. V. (2017). Subpercent accurate fitting of modified gravity growth. Journal of Cosmology and Astroparticle Physics, 2017(11), 1–8. https://doi.org/10.1088/1475-7516/2017/11/052en_US
dc.identifier.issn14757516
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/4035
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.subjectgalaxy clusteringen_US
dc.subjectmodified gravityen_US
dc.subjectredshift surveysen_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.titleSubpercent Accurate Fitting of Modified Gravity Growthen_US
dc.typeArticleen_US
workflow.import.sourcescience

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