Can early dark energy be detected in non-linear structure?

Monthly Notices of the Royal Astronomical Society

Volumn 394, Issue 2, 2009, Pages 605-614

  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

FUNCTIONS; GALAXIES; NUMERICAL METHODS;

ANALYTIC APPROACH; DARK ENERGY; DARK MATTER; LARGE SCALE STRUCTURE OF UNIVERSE; MASS FUNCTIONS; METHOD: NUMERICAL; METHODS:N-BODY SIMULATIONS; N-BODY SIMULATION; NON LINEAR; NONLINEAR STRUCTURE;

ACOUSTIC INTENSITY MEASUREMENT;

EID: 62549113882     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.14286.x     Document Type: Article

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