skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: COSMIC EMULATION: THE CONCENTRATION-MASS RELATION FOR wCDM UNIVERSES

Journal Article · · Astrophysical Journal
; ; ;  [1]
  1. High Energy Physics Division, Argonne National Laboratory, Lemont, IL 60439 (United States)

The concentration-mass relation for dark matter-dominated halos is one of the essential results expected from a theory of structure formation. We present a simple prediction scheme, a cosmic emulator, for the concentration-mass (c-M) relation as a function of cosmological parameters for wCDM models. The emulator is constructed from 37 individual models, with three nested N-body gravity-only simulations carried out for each model. The mass range covered by the emulator is 2 Multiplication-Sign 10{sup 12} M{sub Sun} < M < 10{sup 15} M{sub Sun} with a corresponding redshift range of z = 0-1. Over this range of mass and redshift, as well as the variation of cosmological parameters studied, the mean halo concentration varies from c {approx} 2 to c {approx} 8. The distribution of the concentration at fixed mass is Gaussian with a standard deviation of one-third of the mean value, almost independent of cosmology, mass, and redshift over the ranges probed by the simulations. We compare results from the emulator with previously derived heuristic analytic fits for the c-M relation, finding that they underestimate the halo concentration at high masses. Using the emulator to investigate the cosmology dependence of the c-M relation over the currently allowable range of values, we find-not surprisingly-that {sigma}{sub 8} and {omega}{sub m} influence it considerably, but also that the dark energy equation-of-state parameter w has a substantial effect. In general, the concentration of lower-mass halos is more sensitive to changes in cosmological parameters as compared to cluster mass halos. The c-M emulator is publicly available from http://www.hep.anl.gov/cosmology/CosmicEmu.

OSTI ID:
22126757
Journal Information:
Astrophysical Journal, Vol. 768, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

Similar Records

DARK MATTER HALO PROFILES OF MASSIVE CLUSTERS: THEORY VERSUS OBSERVATIONS
Journal Article · Wed Mar 20 00:00:00 EDT 2013 · Astrophysical Journal · OSTI ID:22126757

COSMIC EMULATION: FAST PREDICTIONS FOR THE GALAXY POWER SPECTRUM
Journal Article · Tue Sep 01 00:00:00 EDT 2015 · Astrophysical Journal · OSTI ID:22126757

The Aemulus Project. II. Emulating the Halo Mass Function
Journal Article · Fri Feb 08 00:00:00 EST 2019 · The Astrophysical Journal (Online) · OSTI ID:22126757