Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters
Abstract 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...
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croxfordunivpr:10.1111/j.1745-3933.2005.00067.x 2024-06-23T07:56:50+00:00 Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters Angulo, R. Baugh, C. M. Frenk, C. S. Bower, R. G. Jenkins, A. Morris, S. L. 2005 http://dx.doi.org/10.1111/j.1745-3933.2005.00067.x https://academic.oup.com/mnrasl/article-pdf/362/1/L25/54692195/mnrasl_362_1_l25.pdf en eng Oxford University Press (OUP) Monthly Notices of the Royal Astronomical Society: Letters volume 362, issue 1, page L25-L29 ISSN 1745-3933 1745-3925 journal-article 2005 croxfordunivpr https://doi.org/10.1111/j.1745-3933.2005.00067.x 2024-06-04T06:07:32Z Abstract 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 imprint of baryons is visible in the power spectrum of cluster-mass dark matter haloes, in spite of significant differences between the halo power spectrum and the prediction of linear perturbation theory. A measurement of the sound horizon scale can constrain the dark energy equation of state. We show that a survey of clusters at intermediate redshift (z∼ 1), like the Sunyaev–Zel'dovich survey proposed by the South Pole Telescope or a red sequence photometric survey with VISTA or the Dark Energy Survey, could potentially constrain the sound horizon scale to an accuracy of ∼2 per cent, in turn fixing the ratio of the pressure of the dark energy to its density (w) to better than ∼10 per cent. Our approach does not require knowledge of the cluster mass, unlike those that depend upon the abundance of clusters. Article in Journal/Newspaper South pole Oxford University Press Hubble ENVELOPE(158.317,158.317,-80.867,-80.867) South Pole Monthly Notices of the Royal Astronomical Society: Letters 362 1 L25 L29 |
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Open Polar |
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Oxford University Press |
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croxfordunivpr |
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English |
description |
Abstract 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 imprint of baryons is visible in the power spectrum of cluster-mass dark matter haloes, in spite of significant differences between the halo power spectrum and the prediction of linear perturbation theory. A measurement of the sound horizon scale can constrain the dark energy equation of state. We show that a survey of clusters at intermediate redshift (z∼ 1), like the Sunyaev–Zel'dovich survey proposed by the South Pole Telescope or a red sequence photometric survey with VISTA or the Dark Energy Survey, could potentially constrain the sound horizon scale to an accuracy of ∼2 per cent, in turn fixing the ratio of the pressure of the dark energy to its density (w) to better than ∼10 per cent. Our approach does not require knowledge of the cluster mass, unlike those that depend upon the abundance of clusters. |
format |
Article in Journal/Newspaper |
author |
Angulo, R. Baugh, C. M. Frenk, C. S. Bower, R. G. Jenkins, A. Morris, S. L. |
spellingShingle |
Angulo, R. Baugh, C. M. Frenk, C. S. Bower, R. G. Jenkins, A. Morris, S. L. Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
author_facet |
Angulo, R. Baugh, C. M. Frenk, C. S. Bower, R. G. Jenkins, A. Morris, S. L. |
author_sort |
Angulo, R. |
title |
Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
title_short |
Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
title_full |
Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
title_fullStr |
Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
title_full_unstemmed |
Constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
title_sort |
constraints on the dark energy equation of state from the imprint of baryons on the power spectrum of clusters |
publisher |
Oxford University Press (OUP) |
publishDate |
2005 |
url |
http://dx.doi.org/10.1111/j.1745-3933.2005.00067.x https://academic.oup.com/mnrasl/article-pdf/362/1/L25/54692195/mnrasl_362_1_l25.pdf |
long_lat |
ENVELOPE(158.317,158.317,-80.867,-80.867) |
geographic |
Hubble South Pole |
geographic_facet |
Hubble South Pole |
genre |
South pole |
genre_facet |
South pole |
op_source |
Monthly Notices of the Royal Astronomical Society: Letters volume 362, issue 1, page L25-L29 ISSN 1745-3933 1745-3925 |
op_doi |
https://doi.org/10.1111/j.1745-3933.2005.00067.x |
container_title |
Monthly Notices of the Royal Astronomical Society: Letters |
container_volume |
362 |
container_issue |
1 |
container_start_page |
L25 |
op_container_end_page |
L29 |
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1802650190572683264 |