Warm dark matter versus bumpy power spectra

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 2, 2003, Pages 617-622

  Little, Brett ^a   Knebe, Alexander ^a   Islam, Ranty R ^b  

^a SWINBURNE UNIVERSITY OF TECHNOLOGY   (Australia)

^b UNIVERSITY OF OXFORD   (United Kingdom)

Author keywords

Cosmology: Theory; Dark matter; Large scale structure of universe; Methods: N body simulations; Methods: Numerical

Indexed keywords

COSMOLOGY; GALAXIES; NUMERICAL METHODS;

COLD DARK MATTERS; COSMOLOGY: THEORY; DARK MATTER; INTEGRATED POWER; LARGE SCALE STRUCTURE OF UNIVERSE; METHOD: NUMERICAL; METHODS:N-BODY SIMULATIONS; POWER; POWER-SPECTRA; SPECTRA'S;

POWER SPECTRUM;

EID: 0142105004     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06437.x     Document Type: Article

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