Concentration, Spin and Shape of Dark Matter Haloes as a Function of the Cosmological Model: WMAP1, WMAP3 and WMAP5 results

Abstract

We investigate the effects of changes in the cosmological parameters between the WMAP 1st, 3rd, and 5th year results on the structure of dark matter haloes. We use a set of simulations that cover 5 decades in halo mass ranging from the scales of dwarf galaxies (V_c ~30 km/s) to clusters of galaxies (V_c ~ 1000 km/s). We find that the concentration mass relation is a power law in all three cosmologies. However the slope is shallower and the zero point is lower moving from WMAP1 to WMAP5 to WMAP3. For haloes of mass log(M_200/Msun) = 10, 12, and 14 the differences in the concentration parameter between WMAP1 and WMAP3 are a factor of 1.55, 1.41, and 1.29, respectively. As we show, this brings the central densities of dark matter haloes in good agreement with the central densities of dwarf and low surface brightness galaxies inferred from their rotation curves, for both the WMAP3 and WMAP5 cosmologies. We also show that none of the existing toy models for the concentration-mass relation can reproduce our simulation results over the entire range of masses probed. In particular, the model of Bullock et al (B01) fails at the higher mass end (M > 1e13 Msun), while the NFW model of Navarro, Frenk & White (1997) fails dramatically at the low mass end (M < 1e12 Msun). We present a new model, based on a simple modification of that of B01, which reproduces the concentration-mass relations in our simulations over the entire range of masses probed (1e10 Msun < M < 1e15 Msun). Haloes in the WMAP3 cosmology (at a fixed mass) are more flatted compared to the WMAP1 cosmology, with a medium to long axis ration reduced by ~10 %. Finally, we show that the distribution of halo spin parameters is the same for all three cosmologies.

arXiv comment16 pages, 16 figures, references updated, minor changes. Accepted for publication on MNRAS. WMAP5 simulations available upon request

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• How Baryonic Processes affect Strong Lensing properties of Simulated Galaxy Clusters
• The last 6 Gyr of dark matter assembly in massive galaxies from the Kilo Degree Survey
• Internal Alignments of Red Versus Blue Discs in Dark Matter Halos
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Disk Galaxy Scaling Relations in the SFI++: Intrinsic Scatter and Applications
• Angular momentum and clustering properties of early dark matter halos
• The impact of galactic feedback on the shapes of dark-matter haloes
• Gamma rays and neutrinos from dark matter annihilation in galaxy clusters
• The Relation Between Halo Shape, Velocity Dispersion and Formation Time
• Abell 2744: Too much substructure for Lambda CDM?
• The mass-concentration relationship of virialized halos and its impact on cosmological observables
• Mass Calibration of the CODEX Cluster Sample using SPIDERS Spectroscopy -- I. The Richness-Mass Relation
• Evidence for inhomogeneous reionization in the local Universe from metal-poor globular cluster systems
• AMICO galaxy clusters in KiDS-DR3: cosmological constraints from large-scale stacked weak lensing profiles
• MOND and IMF variations in early-type galaxies from $ATLA{S}^{3D}$
• The mass function dependence on the dynamical state of dark matter haloes
• Galaxies with grains: unraveling dust evolution and extinction curves with hydrodynamical simulations
• NIHAO III: The constant disc gas mass conspiracy
• SARCS strong-lensing galaxy groups: II - mass-concentration relation and strong-lensing bias
• On the Cluster Physics of Sunyaev-Zel'dovich and X-ray Surveys IV: Characterizing Density and Pressure Clumping due to Infalling Substructures
• The response of dark matter haloes to elliptical galaxy formation: a new test for quenching scenarios
• Supersymmetric Resonant Dark Matter: a Thermal Model for the AMS-02 Positron Excess
• Non-universality of halo profiles and implications for dark matter experiments
• The KMOS Galaxy Evolution Survey (KGES): the angular momentum of star-forming galaxies over the last ~10 Gyr
• On Physical Scales of Dark Matter Halos
• N-body simulations with a cosmic vector for dark energy
• The Core-Cusp Problem Revisited: ULDM vs. CDM
• The Effects of Varying Cosmological Parameters on Halo Substructure
• Probing the galaxy-halo connection with total satellite luminosity
• What do simulations predict for the galaxy stellar mass function and its evolution in different environments?
• Characterizing dark interactions with the halo mass accretion history and structural properties
• Spin Flips - II. Evolution of dark matter halo spin orientation, and its correlation with major mergers
• The connection between the cusp-to-core transformation and observational universalities of DM halos
• Are group- and cluster-scale dark matter halos over-concentrated?
• Distinguishing Dark Matter, Modified Gravity, and Modified Inertia with the Inner and Outer Parts of Galactic Rotation Curves
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• Angular Momentum of Early and Late Type Galaxies: Nature or Nurture?
• The dichotomy of dark matter fraction and total mass density slope of galaxies over five dex in mass
• On the Cosmic Web Elongation in Fuzzy Dark Matter Cosmologies: Effects on Density Profiles, Shapes and Alignments of Halos
• The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
• New evidence for dark matter
• Interaction between dark matter sub-halos & galactic gaseous disk
• Do halos that form early, have high concentration, are part of a pair, or contain a central galaxy potential host more pronounced planes of satellite galaxies?
• A first estimate of the Milky Way dark matter halo spin
• Planck's Dusty GEMS. III. A massive lensing galaxy with a bottom-heavy stellar initial mass function at z=1.5
• Phase-space shapes of clusters and rich groups of galaxies
• Illuminating Dark Matter Halo Density Profiles Without Subhaloes
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Spherically Averaging Ellipsoidal Galaxy Clusters in X-Ray and Sunyaev-Zel'dovich Studies: I. Analytical Relations
• Dark Matter in Elliptical Galaxies
• Searching for Environmental Effects on Galaxy Kinematics in Groups and Clusters at z~1 from the ORELSE Survey
• 21 cm Forest Constraints on Primordial Black Holes
• Fitting and forecasting non-linear coupled dark energy
• Testing Verlinde's emergent gravity in early-type galaxies
• Halo based reconstruction of the cosmic mass density field
• Dark Matter decay and annihilation in the Local Universe: CLUES from Fermi
• Evolution of the luminosity-to-halo mass relation of LRGs from a combined SDSS-DR10+RCS2 analysis
• The scaling relation between baryonic mass and stellar disc size of morphologically late-type galaxies
• Cosmic clocks: A Tight Radius - Velocity Relationship for HI-Selected Galaxies
• The Effect of Adiabatic Compression on Dark Matter Halos and the Radial Acceleration Relation
• Weak lensing clusters from HSC survey first-year data: Mitigating the dilution effect of foreground and cluster member galaxies
• Universal Merger Histories of Dark-Matter Haloes
• A Bayesian Hierarchical Approach to Galaxy-Galaxy Lensing
• Antlia2's role in driving the ripples in the outer gas disk of the Galaxy
• Subhaloes gone Notts: the clustering properties of subhaloes
• Dissecting the spin distribution of Dark Matter halos
• Dark Matter Astrometry: Accuracy of sub-halo positions for the measurement of self-interaction cross sections
• Making sense of the local Galactic escape speed estimates in direct dark matter searches
• Gravitational wave probes on self-interacting dark matter surrounding an intermediate mass black hole
• Dark influences II: gas and star formation in minor mergers of dwarf galaxies with dark satellites
• Towards a new modelling of gas flows in a semi-analytical model of galaxy formation and evolution
• Incorporating baryon-driven contraction of dark matter halos in rotation curve fits
• Probing dark matter signals in neutrino telescopes through angular power spectrum
• On the change of old neutron star masses with galactocentric distance
• Dark Matter and IMF normalization in Virgo dwarf early-type galaxies
• Pushing down the low-mass halo concentration frontier with the Lomonosov cosmological simulations
• Hierarchical inference of the relationship between Concentration and Mass in Galaxy Groups and Clusters
• Primordial Black Hole Merger Rate in Self-Interacting Dark Matter Halo Models
• Hunting for dark halo substructure using submilliarcsecond-scale observations of macrolensed radio jets
• Matter Distribution around Galaxies
• The massive dark halo of the compact, early-type galaxy NGC 1281
• On the coherent rotation of diffuse matter in numerical simulations of galaxy clusters
• Gamma-ray anisotropies from dark matter in the Milky Way: the role of the radial distribution
• Remnants of Galactic subhalos and their impact on indirect dark matter searches
• Mass Bias of Weak Lensing Shear-selected Galaxy Cluster Samples
• Effects of center offset and noise on weak-lensing derived concentration-mass relation of dark matter halos
• Dark influences: imprints of dark satellites on dwarf galaxies
• Dynamical masses of brightest cluster galaxies I: stellar velocity anisotropy and mass-to-light ratios
• DS+: a method for the identification of cluster substructures
• Diffuse Gamma Ray Background from Annihilating Dark Matter in Density Spikes around Supermassive Black Holes
• Dark Matter Deprivation in Field Elliptical Galaxy NGC 7507
• The Tight Empirical Relation between Dark Matter Halo Mass and Flat Rotation Velocity for Late-Type Galaxies
• AMICO galaxy clusters in KiDS-DR3: measuring the splashback radius from weak gravitational lensing
• Normalized additional velocity distribution: testing the radial profile of dark matter halos and MOND
• EDGE: The shape of dark matter haloes in the faintest galaxies
• A detailed statistical analysis of the mass profiles of galaxy clusters
• Spin and structural halo properties at high redshift in a LCDM Universe
• Cosmology through arc statistics I: sensitivity to ${\Omega }_m$ and ${\sigma }_8$
• The non-evolving internal structure of early-type galaxies: the case study SDSS J0728+3835 at z = 0.206
• Domain of validity for pseudo-elliptical NFW lens models
• Reconciling stellar dynamical and hydrostatic X-ray mass measurements of an elliptical galaxy with gas rotation, turbulence and magnetic fields
• The impact of systematic uncertainties in N-body simulations on the precision cosmology from galaxy clustering: a halo model approach
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• Joint Gas and Stellar Dynamical Models of WLM: An isolated dwarf galaxy within a cored, prolate DM halo
• Statistical properties of dark matter mini-haloes at z >= 15
• The Formation of Spiral Galaxies: Adiabatic Compression with Young's Algorithm and the Relation of Dark Matter Haloes to Their Primordial Antecedents
• Testing baryon-induced core formation in $\Lambda$CDM: A comparison of the DC14 and coreNFW dark matter halo models on galaxy rotation curves
• Internal Cluster Structure
• Future sensitivity of neutrino telescopes to dark matter annihilations from the cosmic diffuse neutrino signal
• Stability of Satellite Planes in M31 II: Effects of the Dark Subhalo Population
• The impact of baryons on the internal structure of dark matter haloes from dwarf galaxies to superclusters in the redshift range 0<z<7
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• The Unusually High Halo Concentration of the Fossil Group NGC 6482: Evidence for Weak Adiabatic Contraction
• Dynamical analysis of clusters of galaxies from cosmological simulations
• Boosting small-scale structure via primordial black holes and implications for sub-GeV dark matter annihilation
• Stellar Feedback and the Energy Budget of Late-Type Galaxies: Missing Baryons and Core Creation
• Leo IV & V - A possible dwarf galaxy pair ?
• Dark matter cores in massive high-$z$ galaxies formed by baryonic clumps
• Disentangling cosmic-ray and dark-matter induced gamma-rays in galaxy clusters?
• The cosmology dependence of the concentration-mass-redshift relation
• The Bosma effect revisited - I. HI and stellar disc scaling models
• Abell 315: reconciling cluster mass estimates from kinematics, X-ray, and lensing
• Constraining the nature of dark matter with the star formation history of the faintest Local Group dwarf galaxy satellites
• Searching for dark matter annihilation from individual halos: uncertainties, scatter and signal-to-noise ratios
• BASILISK: Bayesian Hierarchical Inference of the Galaxy-Halo Connection using Satellite Kinematics--I. Method and Validation
• An HSC view of the CMASS galaxy sample. Halo mass as a function of stellar mass, size and Sérsic index
• Constraint on dark matter annihilation with dark star formation using Fermi extragalactic diffuse gamma-ray background data
• Minihalos as probes of the inflationary spectrum: accurate boost factor calculation and new CMB constraints
• Particle ejection during mergers of dark matter halos
• Characterising Strong Lensing Galaxy Clusters using the Millennium-XXL and MOKA simulations
• Gravitational Potential Environment of Galaxies: I. Simulation
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• The tilting rate of the Milky Way's disc
• The Void in the Sculptor Group Spiral Galaxy NGC 247
• How to empirically model star formation in dark matter halos: I. Inferences about central galaxies from numerical simulations
• Increased Prevalence of Bent Lobes for Double-Lobed Radio Galaxies in Dense Environments
• AXES-2MRS: A new all-sky catalogue of extended X-ray galaxy groups
• Discy dwarf disruption and the shape of the Galactic halo
• Quantifying and controlling biases in dark matter halo concentration estimates
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Voronoi Tessellation and Non-parametric Halo Concentration
• Rotation curves of galaxies and the stellar mass-to-light ratio
• The dark matter halo concentration and stellar initial mass function of a CASSOWARY group
• Transonic solutions of isothermal galactic winds in a cold dark matter halo
• Constraining the mass-concentration relation through weak lensing peak function
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• The central dark matter fraction of massive early-type galaxies
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Physical modelling of galaxy clusters using Einasto dark matter profiles
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Transonic galactic outflows in a dark matter halo with a central black hole and its application to the Sombrero galaxy
• Can substructure in the Galactic Halo explain the ATIC and PAMELA results?
• Primordial density perturbations with running spectral index: impact on non-linear cosmic structures
• Semi-empirical catalog of early-type galaxy-halo systems: dark matter density profiles, halo contraction and dark matter annihilation strength
• Cold stream stability during minor mergers
• Virial theorem in clusters of galaxies with MOND
• The importance of the cosmic web and halo substructure for power spectra
• Fingerprints of modified gravity on galaxies in voids
• The extended Planetary Nebula Spectrograph (ePN.S) early-type galaxy survey: The specific angular momentum of ETGs
• Accurate Analytic Mass-Scale Relations for Dark Matter Haloes of all Masses and Redshifts
• A pseudo-spectrum analysis of galaxy-galaxy lensing
• The fundamental plane of evolving red nuggets
• The evolution of galaxy scaling relations in clusters at 0.5<z<1.5
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• The Structure of Cold Dark Matter Halos: Recent Insights from High Resolution Simulations
• Fitting functions for a disk-galaxy model with different LCDM-halo profiles
• The Effect of Interacting Dark Energy on Mass-Temperature Relation in Galaxy Clusters
• Modeling Photoionized Turbulent Material in the Circumgalactic Medium III: Effects of Co-rotation and Magnetic Fields
• The dark matter halo masses of elliptical galaxies as a function of observationally robust quantities
• The quantity of dark matter in early-type galaxies and its relation to the environment
• Dark matter in massive galaxies
• A spiral galaxy's mass distribution uncovered through lensing and dynamics
• On the Galactic radio signal from stimulated decay of axion dark matter
• Star-forming and Quiescent Central Galaxies Cluster Similarly: Implications for the Galaxy-Halo Connection
• High accuracy power spectra including baryonic physics in dynamical Dark Energy models
• HD 42659: The only known roAp star in a spectroscopic binary observed with B photometry, TESS and SALT
• Crazy heart: kinematics of the "star pile" in Abell 545
• Constraining cosmology with the velocity function of low-mass galaxies
• The kinetic Sunyaev-Zel'dovich effect from the diffuse gas in the Local Group
• CHEX-MATE: exploring the kinematical properties of Planck galaxy clusters
• Unravelling the orbits of cluster galaxy populations according to their dominant gas ionization source
• Detecting Adiabatic Contraction in Rotation Curves
• Anatomy of galactic star formation history: Roles of different modes of gas accretion, feedback, and recycling
• Environmental effects on halo abundance and weak lensing peak statistics toward large underdense regions
• Dark matter annihilation into leptons through gravity portals
• A test of invariance of dark matter halo surface density using multiwavelength mock galaxy catalogues
• Statistics for dark matter subhalo searches in gamma rays from a kinematically constrained population model: Fermi-LAT-like telescopes
• Solving the puzzle of subhalo spins
• Massive Black Hole Mergers
• CHEX-MATE: Multi-probe analysis of Abell 1689
• Angular momentum - mass relation for dark matter haloes
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• Host group degeneracy in gravitational lensing time delay determination of $H_0$
• Baryonic Imprints on DM Halos: the concentration-mass relation and its dependence on halo and galaxy properties
• More than just halo mass: Modelling how the red galaxy fraction depends on multiscale density in a HOD framework
• Dark matter halo concentrations: a short review
• Barless flocculent galaxies: a dynamic puzzle
• The connection between halo concentrations and assembly histories: a probe of gravity?
• On the Spin Bias of Satellite Galaxies in the Local Group-like Environment
• Negligible Effects of Baryons on the Angular Momentum Scaling Relations of Galactic Dark Matter Halos
• The distribution of lenticular galaxies in the phase space of present-day galaxy cluster regions
• Primordial Black Hole Mergers as Probes of Dark Matter in Galactic Center
• Signatures of inhomogeneous dark matter annihilation on 21-cm
• Exploring Milky Way rotation curves with Gaia DR3: a comparison between $\Lambda$CDM, MOND, and General Relativistic approaches
• New insights on low-mass dark matter subhalo tidal tracks via numerical simulations
• New probe of modified gravity
• Physical modelling of galaxy clusters and Bayesian inference in astrophysics
• Formation of galactic bulges from the cold gas filaments in high-redshift dark matter halos
• Evolution of the degree of substructures in simulated galaxy clusters
• Analytical insight into dark matter subhalo boost factors for Sommerfeld-enhanced $s$- and $p$-wave $\gamma$-ray signals
• Dark Matter Internal Pair Production -- A Novel Direct Detection Mechanism
• A halo model approach to describe clustering and emission of the two main star forming galaxy populations for Cosmic Infrared Background studies
• Comparing energy and entropy formulations for cosmic ray hydrodynamics
• EDGES of the dark forest: A new absorption window into the composite dark matter and large scale structure
• The AIDA-TNG project: dark matter profiles and concentrations in alternative dark matter models
• Renzo's rule revisited: A statistical study of galaxies' baryon - dark matter coupling
• Impact of baryons on the population of Galactic subhalos and implications for dark matter searches
• The dark halo of the Hydra I galaxy cluster: core, cusp, cosmological? Dynamics of NGC 3311 and its globular cluster system
• Morphology of dark matter haloes beyond triaxiality
• On the Size Evolution of a Galactic Disk in Hierarchical Merging of Cold Dark Matter Halos
• A Random Walk Model for Halo Triaxiality
• The Lowest Metallicity Stars in the LMC: Clues from MaGICC Simulations
• Gas thermodynamics meets galaxy kinematics: Joint mass measurements for eROSITA galaxy clusters
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• Dissecting the 3D structure of elliptical galaxies with gravitational lensing and stellar kinematics
• Reconciling concentration to virial mass relations
• Constraining the population of dark matter halo shapes using hierarchical inference with extragalactic stellar streams
• Modeling mass independent of anisotropy
• The vertical structure of the stellar disk in NGC 551
• Super Interacting Dark Sector: An Improvement on Self-Interacting Dark Matter via Scaling Relations of Galaxy Clusters
• Spikes in the SED and Ripples in the Outskirts of Galaxies
• Systematic variation of central mass density slope in early-type galaxies
• Monophotons from Scalar Portal Dark Matter at Neutrino Experiments
• The galaxy cluster concentration-mass relation in dark energy cosmologies
• The origin of ionized gas in retired galaxies: dynamical clues
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Universal Fitting Formulae for the Peak Concentration of Dark Matter Halos