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...
Main Authors: | , , , , , |
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Language: | English |
Published: |
2005
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Subjects: | |
Online Access: | http://cds.cern.ch/record/847390 |