Precision Determination of the Mass Function of Dark Matter Halos

Abstract

The predicted mass function of dark matter halos is essential in connecting observed galaxy cluster counts and models of galaxy clustering to the properties of the primordial density field. We determine the mass function in the concordance $\Lambda$CDM cosmology, as well as its uncertainty, using sixteen $1024^3$-particle nested-volume dark-matter simulations, spanning a mass range of over five orders of magnitude. Using the nested volumes and single-halo tests, we find and correct for a systematic error in the friends-of-friends halo-finding algorithm. We find a fitting form and full error covariance for the mass function that successfully describes the simulations' mass function and is well-behaved outside the simulations' resolutions. Estimated forecasts of uncertainty in cosmological parameters from future cluster count surveys have negligible contribution from remaining statistical uncertainties in the central cosmology multiplicity function. There exists a potentially non-negligible cosmological dependence (non-universality) of the halo multiplicity function.

4 pages, 3 figures, submitted to ApJL

References in corpus (8)

• Big Bang Nucleosynthesis (in "The Review of Particle Properties" 2004)
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• Self-Calibration of Cluster Dark Energy Studies: Observable-Mass Distribution
• Galaxy-galaxy Lensing: Dissipationless Simulations Versus the Halo Model
• Robustness of Cosmological Simulations I: Large Scale Structure
• Cosmology and the Halo Occupation Distribution from Small-Scale Galaxy Clustering in the Sloan Digital Sky Survey
• Constraining the Evolution of Dark Energy with a Combination of Galaxy Cluster Observables
• Weighing Neutrinos with Galaxy Cluster Surveys

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• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• On the Abundance of Extreme Voids II: A Survey of Void Mass Functions
• Measuring the scatter of the mass-richness relation in galaxy clusters in photometric imaging surveys by means of their correlation function
• Dark from light (DfL): Inferring halo properties from luminous tracers with machine learning trained on cosmological simulations. I. Method, proof of concept & preliminary testing
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• HIKER: a halo-finding method based on kernel-shift algorithm
• Aemulus $\nu$: Precision halo mass functions in w$\nu$CDM cosmologies
• Sunyaev-Zel'dovich contribution in CMB analysis
• Cosmological Implications of a Neutrino Mass Detection
• Void Formation: Does the Void-in-Cloud Process Matter?
• The same with less: The cosmic web of warm versus cold dark matter dwarf galaxies
• Simulation budgeting for hybrid effective field theories
• The implications of overmassive black holes at $z>5$ for quasar and black hole growth
• Dark Energy Simulations
• Adaptive friends-of-friends algorithm for identifying gravitationally bound cosmological structures
• Probing the Large-Scale Homogeneity of the Universe with Galaxy Redshift Surveys
• Excursion Sets with a "Perfect" Collapse Model
• On the universality of the halo mass function beyond $\Lambda$CDM cosmology
• Impact of a Rapid Diluted Energy Density on the halo mass function
• Reconstructing the velocity field beyond the local universe
• Euclid preparation. L. Calibration of the linear halo bias in $\Lambda (\nu )$CDM cosmologies
• X-ray flux -- mass relation for $z\gtrsim 0.7$ galaxy clusters
• The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
• Slicing cluster mass functions with a Bayesian razor
• Scalar field theory for warm dark matter
• Investigation of homogeneity and matter distribution on large scales using large quasar groups
• Universality of the halo mass function in modified gravity cosmologies
• Searching for dark matter isocurvature initial conditions with N-body Simulations
• Mass functions from the excursion set model
• Using Dark Matter Haloes to Learn about Cosmic Acceleration: A New Proposal for a Universal Mass Function
• Segmenting proto-halos with vision transformers
• Web-Halo Model (WHM): Accurate non-linear matter power spectrum predictions without free parameters
• Tracing cosmic voids with fast simulations
• A revisited Correction to the Halo Mass Function for local-type Primordial non-Gaussianity