Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters

Acoustic oscillations in the baryon-photon fluid leave a signature in the matter power spectrum. The overall shape of the spectrum and the wavelength of the oscillations depend upon the sound horizon scale at recombination. Using the $\Lambda$ cold dark matter Hubble Volume simulation, we show that...

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Bibliographic Details
Main Authors: Angulo, R, Baugh, C M, Frenk, C S, Bower, R G, Jenkins, A, Morris, S L
Language:English
Published: 2005
Subjects:
Online Access:http://cds.cern.ch/record/847390