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Prog. Theor. Phys. Vol. 111 No. 1 (2004) pp. 1-12
Cluster Abundance Evolution and the Sunyaev-Zeldovich Effect in Various Cosmological Models
Kenji Tomita*
Yukawa Institute for Theoretical Physics, Kyoto University,
Kyoto 606-8502, Japan
(Received June 1, 2003)
Abstract:
The redshift dependence of the observed cluster abundance due to the
Sunyaev-Zeldovich effect (SZE) is studied in various cosmological
models, including
flat and open homogeneous (CDM) models and an inhomogeneous model with
a large-scale local void. The Press-Schechter formalism is used to derive the
abundance at epochs in the range 0 < z < 2, and the cluster mass
limit M lim is obtained from a flux limit for SZE. It is shown
that SZE is useful for constraining
the cosmological model parameters, and the abundance in the inhomogeneous model
may be comparable with that in the low-density homogeneous models.
The significance of relative difference of abundances in the various models
is discussed.
URL :
http://ptp.ipap.jp/link?PTP/111/1/
DOI : 10.1143/PTP.111.1
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