Model-independent dark energy differentiation with the integrated Sachs-Wolfe effect

PS Corasaniti, BA Bassett, Carlo Ungarelli, EJ Copeland

Research output: Contribution to journalArticle

40 Citations (Scopus)

Abstract

We study the integrated Sachs-Wolfe effect using a model-independent parametrization of the dark energy equation of state, w(z). Cosmic variance severely restricts the class of models distinguishable from one based on cold dark matter and a cosmological constant unless w(z) currently satisfies w(o)(Q)>-0.8, or exhibits a rapid, late-time, transition at redshifts z
Original languageEnglish
Pages (from-to)091303
Number of pages1
JournalPhysical Review Letters
Volume90
Issue number9
Early online date1 Mar 2003
DOIs
Publication statusPublished - 1 Mar 2003

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