A differential method of search for the CMBR spectral-spatial fluctuations

Abstract

The CMBR spectral-spatial fluctuations (SSF) formed in early Universe during the Dark Ages are considered. Main attention is focused on the narrow-band spectral properties of the SSF. Based on these properties we propose to use a differential method in order to search for these fluctuations. Description of the method is given.

Latex, 9 pages with 4 Postscript figures

References in corpus (2)

• The Case for a Positive Cosmological Lambda-term
• A measurement of Omega from the North American test flight of BOOMERANG