Hostname: page-component-745bb68f8f-l4dxg Total loading time: 0 Render date: 2025-01-13T10:49:37.083Z Has data issue: false hasContentIssue false
  • English
  • Français

Microwave Background Anisotropies in a Baryon-Dominated Universe

Published online by Cambridge University Press:  03 August 2017

Yasushi Suto ,
Naoteru Gouda  and
Misao Sasaki
Yasushi Suto
Affiliation:
Department of Astronomy, University of California, Berkeley
Naoteru Gouda
Affiliation:
Department of Physics, Kyoto University, Japan
Misao Sasaki
Affiliation:
RITP, Hiroshima University, Japan

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We have calculated the anisotropies of the cosmic microwave background radiation in a baryon-dominated model (BDM), using a gauge invariant method. The results on a 4.5′ angular scale are as follows (h = 0.5 and initially Zel'dovich power spectrum assumed):

Type
Appendix 1: Poster Papers
Information
Symposium - International Astronomical Union , Volume 130: Large Scale Structures of the Universe , 1988 , pp. 513
Copyright
Copyright © Reidel 1988