Numerical study of halo concentrations in dark-energy cosmologies

Astronomy and Astrophysics

Volumn 416, Issue 3, 2004, Pages 853-864

  Dolag, K ^a   Bartelmann, M ^b   Perrotta, F ^c,d   Baccigalupi, C ^c,d   Moscardini, L ^e   Meneghetti, M ^a   Tormen, G ^a  

^a UNIVERSITY OF PADOVA   (Italy)

^b MAX PLANCK INSTITUT FÜR ASTROPHYSIK   (Germany)

^c SISSA   (Italy)

^d LAWRENCE BERKELEY NATIONAL LABORATORY   (United States)

^e UNIVERSITY OF BOLOGNA   (Italy)

Author keywords

Cosmology: theory; Galaxies: clusters: general; Galaxies: halos

Indexed keywords

ACCELERATION; ALGORITHMS; COMPUTER SIMULATION; GALAXIES; GRAVITATION; PARAMETER ESTIMATION; PERTURBATION TECHNIQUES; SPECTRUM ANALYSIS;

COSMOLOGY: THEORY; GALAXIES: CLUSTERS: GENERAL; GALAXIES: HALOS;

ASTRONOMY;

EID: 1642588148     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20031757     Document Type: Article

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