Accurate universal models for the mass accretion histories and concentrations of dark matter halos

Abstract

A large amount of observations have constrained cosmological parameters and the initial density fluctuation spectrum to a very high accuracy. However, cosmological parameters change with time and the power index of the power spectrum varies with mass scale dramatically in the so-called concordance Lambda CDM cosmology. Thus, any successful model for its structural evolution should work well simultaneously for various cosmological models and different power spectra. We use a large set of high-resolution N-body simulations of a variety of structure formation models (scale-free, standard CDM, open CDM, and Lambda CDM) to study the mass accretion histories (MAHs), the mass and redshift dependence of concentrations and the concentration evolution histories of dark matter halos. We find that there is significant disagreement between the much-used empirical models in the literature and our simulations. According to two simple but tight correlations we find from the simulation results, we develop new empirical models for both the MAHs and the concentration evolution histories of dark matter halos, and the latter can also be used to predict the mass and redshift dependence of halo concentrations. These models are accurate and universal: the same set of model parameters works well for different cosmological models and for halos of different masses at different redshifts and the model predictions are highly accurate even when the histories are traced to very high redshift. These models are also simple and easy to implement. A web calculator and a user-friendly code to make the relevant calculations are available from http://www.shao.ac.cn/dhzhao/mandc.html . We explain why Lambda CDM halos on nearly all mass scales show two distinct phases in their evolution histories.

arXiv comment17 pages, including 22 figures, publicated in ApJ; V2: some new figures added; V3: some typo fixed

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• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• Explaining JWST star formation history at $z\sim 17$ by modifying $\Lambda$CDM
• A Random Walk Model for Dark Matter Halo Concentrations
• Effects of Neutrino Masses and Asymmetries on Dark Matter Halo Assembly
• Towards a Model-Independent Measurement of the Halo Mass Function with Observables
• Nonlinear structure formation in Bound Dark Energy
• Cluster Assembly Times as a Cosmological Test
• Modelling the mass accretion histories of dark matter haloes using a Gamma formalism
• Characterizing the Best Cosmic Telescopes with the Millennium Simulations
• Semi-analytical frameworks for subhalos from the smallest to the largest scale
• Simulation studies of dark energy clustering induced by the formation of dark matter halos
• Galaxy and halo properties around cosmic filaments from Sloan Digital Sky Survey Data Release 7 and the ELUCID simulation
• Characterizing the assembly of dark matter halos with protohalo size histories: I. Redshift evolution, relation to descendant halos, and halo assembly bias
• Accurate dark matter halo elongation from weak-lensing stacking analysis
• The kinetic Sunyaev-Zel'dovich effect from the diffuse gas in the Local Group
• Testing the Reliability of Fast Methods for Weak Lensing Simulations: WL-MOKA on PINOCCHIO
• Gravothermalizing into primordial black holes, boson stars, and cannibal stars
• Massive Black Hole Mergers
• The eventful life journey of galaxy clusters. I. Impact of DM halo and ICM properties on their full assembly histories
• A halo model of extragalactic contamination to CMB lensing, delensing, and cross-correlations
• Discovery of a damped Ly$\alpha$ absorber originating in a spectacular interacting dwarf galaxy pair at $z=0.026$
• Evolution of dwarf galaxy observable parameters
• Halo Concentrations and the Fundamental Plane of Galaxy Clusters
• The Compactness of Galaxy Groups in the Sloan Digital Sky Survey
• ACACIA: a new method to produce on-the-fly merger trees in the RAMSES code
• Splashback radius and the mass accretion rate of RASS MCMF galaxy clusters
• The Dependence of Dark Matter Halo Properties on the Morphology of Their Central Galaxies from Weak Lensing
• Dark matter halo concentrations: a short review
• The connection between halo concentrations and assembly histories: a probe of gravity?
• The Assembly of the Virgo Cluster, Traced by its Galaxy Halos
• Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
• Estimating the evolution of gas in the Fornax dwarf spheroidal galaxy from its star formation history: an illustrative example
• Does stellar mass assembly history vary with environment?
• The impact of baryons on the sparsity of simulated galaxy clusters from The Three Hundred Project
• The environmental dependence of the stellar mass fundamental plane of early-type galaxies
• Semi-Analytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in CDM
• Too small to succeed: the difficulty of sustaining star formation in low-mass haloes
• Describing the Nonuniversal Galaxy Merger Timescales in IllustrisTNG: Effects of Host Halo Mass, Baryons, and Sample Selection
• Direct Collapse Black Hole Candidates from Decaying Dark Matter
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• A Chemical Evolution Model for the Fornax Dwarf Spheroidal Galaxy
• Gravitational potential drives the concentration dependence of the stellar mass-halo mass relation
• Cosmological evolution of gas and supermassive black holes in idealized isolated halos
• Probabilistic Inference of the Structure and Orbit of Milky Way Satellites with Semi-Analytic Modeling
• Cosmo-Paleontology: Statistics of Fossil Groups in a Gravity-Only Simulation
• Strong Conformity and Assembly Bias: Towards a Physical Understanding of the Galaxy-Halo Connection in SDSS Clusters
• Iterative mean-field approach to the spherical collapse of dark matter halos
• Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos
• Towards a universal model for the density profiles of dark matter haloes
• Timing the last major merger of galaxy clusters with large halo sparsity
• Cosmic Reionization On Computers: Baryonic Effects on Halo Concentrations During the Epoch of Reionization
• SDSS-IV MaNGA: How the stellar populations of passive central galaxies depend on stellar and halo mass
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos
• Massive Neutrinos Promote the Size Growth of Early-Type Galaxies
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Extending the SAGA Survey (xSAGA) I: Satellite Radial Profiles as a Function of Host Galaxy Properties
• Co-evolution of the Brightest Cluster Galaxies and their Host Clusters in IllustrisTNG