Modelling the clustering of dark matter haloes in resummed perturbation theories

Monthly Notices of the Royal Astronomical Society

Volumn 416, Issue 3, 2011, Pages 1703-1716

  Elia, A ^a   Kulkarni, S ^a   Porciani, C ^a   Pietroni, M ^b   Matarrese, S ^b,c  

^a UNIVERSITY OF BONN   (Germany)

^b SEZIONE DI PADOVA   (Italy)

^c UNIVERSITY OF PADOVA   (Italy)

Author keywords

Cosmology: theory; Galaxies: haloes; Large scale structure of Universe; Methods: analytical

Indexed keywords

COSMOLOGY; GALAXIES; GRAVITATION; PERTURBATION TECHNIQUES; STATISTICAL MECHANICS; VELOCITY;

CLUSTERINGS; COSMOLOGY: THEORY; DARK MATTER HALOS; DENSITY FIELDS; GALAXY DISTRIBUTION; GALAXY:HALO; LARGE SCALE STRUCTURE OF UNIVERSE; METHODS:ANALYTICAL; PERTURBATION THEORY; POWER-SPECTRA;

POWER SPECTRUM;

EID: 84860389597     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.18761.x     Document Type: Article

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