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On galaxy cluster sizes and temperatures

Verde, Licia and Kamionkowski, Marc and Mohr, Joseph J. and Benson, Andrew J. (2001) On galaxy cluster sizes and temperatures. Monthly Notices of the Royal Astronomical Society, 321 (1). L7-L13. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20200519-170818941

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Abstract

We show that the distribution of the sizes and temperatures of clusters can be used to constrain cosmological models. The size-temperature (ST) distribution predicted in a flat Gaussian cluster-abundance-normalized Ω₀ = 0.3 model agrees well with the fairly tight ST relation observed. A larger power-spectrum amplitude σ₈ would give rise to a larger scatter about the ST relation as would a larger value of Ω₀ and/or long non-Gaussian high-density tails in the probability density function. For Gaussian initial conditions, the ST distribution suggests a constraint σ₈Ω₀⁰·²⁶ ≃ 0.76. The ST relation is expected to get tighter at high redshifts. In the process, we derive a simple formula for the halo formation-redshift distribution for non-Gaussian models. We also suggest that the discrepancy between the naive zero-redshift ST relation and that observed may be owing, at least in part, to the fact that lower-mass clusters form over a wider range of redshifts. An Appendix derives an equation for the formation-redshift distribution of haloes.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1046/j.1365-8711.2001.04185.xDOIArticle
https://arxiv.org/abs/astro-ph/0007426arXivDiscussion Paper
ORCID:
AuthorORCID
Verde, Licia0000-0003-2601-8770
Kamionkowski, Marc0000-0001-7018-2055
Benson, Andrew J.0000-0001-5501-6008
Additional Information:© 2001 RAS. Accepted 2000 November 6. Received 2000 October 25; in original form 2000 August 3. Published: 11 February 2001. We thank P. Goldreich for asking questions that stimulated this investigation. This research was supported in part by the NSF under grant no. PHY94-07194 to the Institute for Theoretical Physics (Santa Barbara), where part of this research was completed. LV was supported by a TMR grant and thanks Caltech for hospitality. MK was supported in part by NSF AST-0096023, NASA NAG5-8506, and DoE DE-FG03-92-ER40701. JJM is supported by Chandra Fellowship grant PF8-1003, awarded through the Chandra Science Center. The Chandra Science Center is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-39073. AJB was supported by a PPARC studentship.
Funders:
Funding AgencyGrant Number
NSFPHY94-07194
NSFAST-0096023
NASANAG5-8506
Department of Energy (DOE)DE-FG03-92-ER40701
NASAPF8-1003
NASANAS8-39073
Particle Physics and Astronomy Research Council (PPARC)UNSPECIFIED
Subject Keywords:galaxies: clusters: general, galaxies: formation, galaxies: high-redshift, galaxies: structure, cosmology: theory
Issue or Number:1
Record Number:CaltechAUTHORS:20200519-170818941
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20200519-170818941
Official Citation:Licia Verde, Marc Kamionkowski, Joseph J. Mohr, Andrew J. Benson, On galaxy cluster sizes and temperatures, Monthly Notices of the Royal Astronomical Society, Volume 321, Issue 1, February 2001, Pages L7–L13, https://doi.org/10.1046/j.1365-8711.2001.04185.x
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:103338
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:20 May 2020 22:26
Last Modified:20 May 2020 22:30

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