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Dark-energy dynamics required to solve the cosmic coincidence

Egan, Chas; Lineweaver, Charles

Description

Dynamic dark-energy (DDE) models are often designed to solve the cosmic coincidence (why, just now, is the dark-energy density ρde the same order of magnitude as the matter density ρm?) by guaranteeing ρde∼ρm for significant fractions of the age of

dc.contributor.authorEgan, Chas
dc.contributor.authorLineweaver, Charles
dc.date.accessioned2015-12-08T22:29:52Z
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/1885/34261
dc.description.abstractDynamic dark-energy (DDE) models are often designed to solve the cosmic coincidence (why, just now, is the dark-energy density ρde the same order of magnitude as the matter density ρm?) by guaranteeing ρde∼ρm for significant fractions of the age of
dc.publisherAmerican Physical Society
dc.sourcePhysical Review D-Particles, Fields, Gravitation and Cosmology
dc.titleDark-energy dynamics required to solve the cosmic coincidence
dc.typeJournal article
local.description.notesImported from ARIES
local.identifier.citationvolume78
dc.date.issued2008
local.identifier.absfor020102 - Astronomical and Space Instrumentation
local.identifier.absfor040302 - Extraterrestrial Geology
local.identifier.ariespublicationu4047674xPUB111
local.type.statusPublished Version
local.contributor.affiliationEgan, Chas, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLineweaver, Charles, College of Physical and Mathematical Sciences, ANU
local.description.embargo2037-12-31
local.bibliographicCitation.startpage083528-1 - 083528-13
local.identifier.doi10.1103/PhysRevD.78.083528
dc.date.updated2015-12-08T09:24:56Z
local.identifier.scopusID2-s2.0-55649111596
local.identifier.thomsonID000260574900049
CollectionsANU Research Publications

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