Filament and shape statistics: A quantitative comparison of cold + hot and cold dark matter cosmologies versus CfA1 data

Monthly Notices of the Royal Astronomical Society

Volumn 284, Issue 3, 1997, Pages 607-626

  Davé, Romeel ^a   Hellinger, Doug ^b   Primack, Joel ^b   Nolthenius, Richard ^a   Klypin, Anatoly ^c  

^a University of California at Santa Cruz   (United States)

^b UNIVERSITY OF CALIFORNIA SANTA CRUZ   (United States)

^c NEW MEXICO STATE UNIVERSITY   (United States)

Author keywords

Cosmology: theory; Dark matter; Large scale structure of universe; Methods: data analysis; Methods: numerical

Indexed keywords

COSMOLOGY; GALAXIES; NUMERICAL METHODS;

COLD DARK MATTERS; COSMOLOGY: THEORY; DARK MATTER; HOT DARK MATTER; LARGE SCALE STRUCTURE OF UNIVERSE; METHOD: NUMERICAL; METHODS. DATA ANALYSIS; PLANARITY; RED SHIFT; SHAPE STATISTICS;

STATISTICS;

EID: 0010164317     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/284.3.607     Document Type: Article

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