Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2930
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dc.contributor.authorMajumdar, S-
dc.date.accessioned2008-07-29T04:53:29Z-
dc.date.available2008-07-29T04:53:29Z-
dc.date.issued2001-07-
dc.identifier.citationAstrophysical Journal, Vol. 555, No. 1, Part 2, pp. L7 - L10en
dc.identifier.issn0004-637X-
dc.identifier.urihttp://hdl.handle.net/2248/2930-
dc.description.abstractStudy of the primary anisotropies of the cosmic microwave background (CMB) can be used to determine the cosmological parameters to a very high precision. The power spectrum of the secondary CMB anisotropies due to the thermal Sunyaev-Zeldovich effect (SZE) by clusters of galaxies can then be studied, to constrain more cluster-specific properties (like gas mass). We show the SZE power spectrum from clusters to be a sensitive probe of any possible evolution (or constancy) of the gas mass fraction. The position of the peak of the SZE power spectrum is a strong discriminatory signature of different gas mass fraction evolution models. For example, for a flat universe, there can be a difference in the l-values (of the peak) of as much as 2500 between a constant gas mass fraction model and an evolutionary one. Moreover, observational determination of the power spectrum, from blank-sky surveys, is devoid of any selection effects that can possibly affect targeted X-ray or radio studies of gas mass fractions in galaxy clusters.en
dc.format.extent93208 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAmerican Astronomical Societyen
dc.relation.urihttp://www.journals.uchicago.edu/doi/abs/10.1086/323159en
dc.subjectCosmology: Cosmic Microwave Backgrounden
dc.subjectCosmology: Observations,en
dc.subjectCosmology: Theoryen
dc.subjectGalaxies: Clusters: Generalen
dc.titleProbing the Evolution of the Gas Mass Fraction with the Sunyaev-Zeldovich Effecten
dc.typeArticleen
Appears in Collections:IIAP Publications

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