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 Λ cold dark matter Hubble Volume simulation, we show that the impr...

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Bibliographic Details
Published in:Monthly Notices of the Royal Astronomical Society: Letters
Main Authors: Angulo, R., Baugh, C. M., Frenk, C. S., Bower, R. G., Jenkins, A. R., Morris, S. L.
Format: Article in Journal/Newspaper
Language:unknown
Published: Blackwell 2005
Subjects:
Online Access:http://dro.dur.ac.uk/4219/
http://dro.dur.ac.uk/4219/1/4219.pdf
https://doi.org/10.1111/j.1745-3933.2005.00067.x