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Cosmic Background Anisotropies in Cold Dark Matter Cosmology

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Sugiyama, Naoshi·1995·The Astrophysical Journal Supplement Series

Abstract

Cosmic microwave background (CMB) anisotropies and density fluctuations are calculated for flat cold dark matter (CDM) models with a wide range of parameters, viz., Ω0, h, and ΩB, for standard recombination and for various epochs of reionization. Tables of the power spectrum of CMB anisotropies in the form of C1 values as a function of l are presented. Although the Harrison-Zeldovich initial spectrum is assumed in these tables, we present simple approximations for obtaining the C1 values corresponding to a tilted spectrum from those with a Harrison-Zeldovich spectrum. Values of σ8 are derived for the matter density spectrum, with α(10°), fixed Qrms-PS and COBE Differential Microwave Radiometer (DMR) 2 yr normalizations. Simple modifications of the fitting formula for the density transfer function are given which are applicable for models with high baryon density. By using both numerical results and these fitting formulae, we calculate the relation between α8 and Qrms-PS and find good agreement. In addition, the velocity fields are calculated.

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Metadata

Authors
Sugiyama, N.
Venue
The Astrophysical Journal Supplement Series
Published
1995-10
Volume
100
Pages
281
ISSN
  • 0067-0049 (ISSN-L)
  • 1538-4365
OpenAlex
W2951915383
Cited by
462
References
0
Type
conference abstract
Language
en
Open access
green

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CoChat. (2026). Citation check: Cosmic Background Anisotropies in Cold Dark Matter Cosmology. https://app.cochat.ai/papers/10.1086/192220
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Sugiyama, N. (1995). Cosmic Background Anisotropies in Cold Dark Matter Cosmology. The Astrophysical Journal Supplement Series. https://doi.org/10.1086/192220

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