{"id":"W2117363750","doi":"10.1046/j.1365-8711.2003.06503.x","title":"Stable clustering, the halo model and non-linear cosmological power spectra","year":2003,"lang":"en","type":"article","venue":"Monthly Notices of the Royal Astronomical Society","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2079,"is_retracted":false,"has_abstract":true,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Scaling; Nonlinear system; Cluster analysis; Matter power spectrum; Halo; Spectral line; Dark matter; Statistical physics; Cold dark matter; Astrophysics; Cosmology; Power law; Theoretical physics; Computational physics; Galaxy; Quantum mechanics; Dark energy; Statistics; Geometry; Computer science; Artificial intelligence","routes":{"ca_aff":true,"ca_fund":false,"ca_venue":false,"about_ca":false,"invisible_to_affiliation_only":false},"retraction":null,"screen":null,"machine_scores":{"provisional":true,"baseline":true,"maturity_gate_passed":false,"score_opus":0.008496714617576092,"score_gpt":0.199228125653076,"score_spread":0.1907314110354999,"validation_status":"score_only:v0-immature-baseline","note":"Baseline scores from an immature model (maturity gate not passed). Scores rank; they never assert a category."}}