Dependence of the non-linear mass power spectrum on the equationof state of dark energy

Monthly Notices of the Royal Astronomical Society

Volumn 366, Issue 2, 2006, Pages 547-556

  McDonald, Patrick ^a   Trac, Hy ^b,c   Contaldi, Carlo ^a,d  

^a UNIVERSITY OF TORONTO   (Canada)

^b PRINCETON UNIVERSITY   (United States)

^c PRINCETON UNIVERSITY OBSERVATORY   (United States)

^d IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

Cosmological parameters; Cosmology: theory; Dark matter; Equation of state; Large scale structure of Universe; Methods: N body simulations

Indexed keywords

COSMOLOGY; EQUATIONS OF STATE;

COSMOLOGICAL PARAMETERS; COSMOLOGY: THEORY; DARK ENERGY; DARK MATTER; EQUATION-OF-STATE; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS:N-BODY SIMULATIONS; NON LINEAR; POWER; POWER-SPECTRA;

POWER SPECTRUM;

EID: 33645058167     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2005.09881.x     Document Type: Article

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