Power spectra to 1 per cent accuracy between dynamical dark energy cosmologies

Monthly Notices of the Royal Astronomical Society

Volumn 380, Issue 3, 2007, Pages 1079-1086

  Francis, Matthew J ^a   Lewis, Geraint F ^a   Linder, Eric V ^b  

^a UNIVERSITY OF SYDNEY   (Australia)

^b LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

Author keywords

Dark matter; Large scale structure of Universe; Methods: N body simulations; Methods: numerical

Indexed keywords

EQUATIONS OF STATE; GALAXIES; GRAVITATION; NUMERICAL METHODS; POWER SPECTRUM;

DARK ENERGY; DARK ENERGY EQUATION; DARK MATTER; EQUATION-OF-STATE; LARGE SCALE STRUCTURE OF UNIVERSE; METHOD: NUMERICAL; METHODS:N-BODY SIMULATIONS; POWER-SPECTRA; RED SHIFT; RELATIVE MASS;

COSMOLOGY;

EID: 34548654029     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12139.x     Document Type: Article

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