dc.creatorManolis Plionis
dc.date2011-06
dc.date.accessioned2023-07-25T16:24:21Z
dc.date.available2023-07-25T16:24:21Z
dc.identifierhttp://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1803
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/7806995
dc.descriptionWe derive an exact analytical solution for the redshift evolution of linear and scale-independent bias, by solving a second order differential equation based on linear perturbation theory. This bias evolution model is applicable to all different types of dark energy and modified gravity models. We propose that the combination of the current bias evolution model with data on the bias of extragalactic mass tracers could provide an efficient way to discriminate between “geometrical” dark energy models and dark energy models that adhere to general relativity.
dc.formatapplication/pdf
dc.languageeng
dc.publisherPhysical review D: Particles and fields
dc.relationcitation:Basilakos, S., et al., (2011), The generalized evolution of linear bias: a tool to test gravity, Physical review D: Particles and fields, Vol. 83(12):1-5
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/4.0
dc.subjectinfo:eu-repo/classification/Inspec/Extragalactic mass
dc.subjectinfo:eu-repo/classification/Inspec/Dark energy models
dc.subjectinfo:eu-repo/classification/Inspec/Test gravity
dc.subjectinfo:eu-repo/classification/cti/1
dc.subjectinfo:eu-repo/classification/cti/21
dc.subjectinfo:eu-repo/classification/cti/21
dc.titleThe generalized evolution of linear bias: a tool to test gravity
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/acceptedVersion
dc.audiencestudents
dc.audienceresearchers
dc.audiencegeneralPublic


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