COMPLEMENTARITY OF PECULIAR VELOCITY SURVEYS AND REDSHIFT SPACE DISTORTIONS FOR TESTING GRAVITY

dc.contributor.authorKim, Alex G.
dc.contributor.authorLinder, Eric V.
dc.date.accessioned2022-07-05T10:42:01Z
dc.date.available2022-07-05T10:42:01Z
dc.date.issued2020
dc.description.abstractPeculiar-velocity surveys of the low-redshift universe have significant leverage to constrain the growth rate of cosmic structure and test gravity. Wide-field imaging surveys combined with multiobject spectrographs [e.g., ZTF2, Large Synoptic Survey Telescope (LSST), DESI, and 4MOST] can use type Ia supernovae as informative tracers of the velocity field, reaching few percent constraints on the growth rate fσ8 at z ≲ 0.2 where density tracers cannot do better than ∼10%. Combining the high-redshift DESI survey mapping redshift space distortions with a low-redshift supernova peculiar velocity survey using LSST and DESI can determine the gravitational growth index to σðγÞ ≈ 0.02, testing general relativity. We study the characteristics needed for the peculiar velocity survey, and how its complementarity with clustering surveys improves when going from a ΛCDM model assumption to a w0–wa cosmologyen_US
dc.identifier.citationKim, A. G., & Linder, E. V. (2020). Complementarity of peculiar velocity surveys and redshift space distortions for testing gravity. Physical Review D, 101(2). https://doi.org/10.1103/physrevd.101.023516en_US
dc.identifier.urihttp://nur.nu.edu.kz/handle/123456789/6373
dc.language.isoenen_US
dc.publisherPHYSICAL REVIEW Den_US
dc.rightsAttribution-NonCommercial-ShareAlike 3.0 United States*
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/us/*
dc.subjectType of access: Open Accessen_US
dc.subjectCosmologyen_US
dc.subjectgravityen_US
dc.titleCOMPLEMENTARITY OF PECULIAR VELOCITY SURVEYS AND REDSHIFT SPACE DISTORTIONS FOR TESTING GRAVITYen_US
dc.typeArticleen_US
workflow.import.sourcescience

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