Can non-Gaussian cosmological models explain the WMAP high optical depth for reionization?

Monthly Notices of the Royal Astronomical Society

Volumn 346, Issue 3, 2003, Pages

  Chen, Xuelei ^a   Cooray, Asantha ^b   Yoshida, Naoki ^c   Sugiyama, Naoshi ^c  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^c NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Cosmic microwave background; Cosmology: observations; Cosmology: theory; Large scale structure of Universe

Indexed keywords

GAUSSIAN DISTRIBUTION; GAUSSIAN NOISE (ELECTRONIC); OPTICAL PROPERTIES; STARS;

COSMIC MICROWAVES BACKGROUND; COSMOLOGICAL MODELING; COSMOLOGY OBSERVATIONS; COSMOLOGY: THEORY; DENSITY FLUCTUATION; LARGE SCALE STRUCTURE OF UNIVERSE; NON-GAUSSIAN; OPTICAL DEPTH; REIONIZATION; STARS FORMATION;

COSMOLOGY;

EID: 0346267391     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2003.07316.x     Document Type: Article

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