Observational and Theoretical Constraints on Singular Dark Matter Halos

Abstract

The distribution of dark matter around galactic or cluster halos has usually been assumed to be approximately isothermal with a non-zero core radius, which is expected to be of the order of the size of the visible matter distribution. Recently, the possibility has been raised that dark matter halos might be singular in the sense that the dark matter density $\rho$ could increase monotonically with radius $r$ down to a very small distance from the center of galaxies or clusters. Such central cusps in the dark matter density could lead to a high flux of gamma rays from WIMP dark matter annihilation. Here we analyze two possibilities that have been discussed in the literature, $\rho \propto r^{-n}$ with $n\approx 1\mathrm{or}2$, and point out that such density profiles are excluded by gravitional lensing analyses on cluster scales and by the rotation curves of gas-rich, halo-dominated dwarf spirals on small scales. We also point out that if spiral galaxies form by gas infall inside dark matter halos, as they are expected to do in any hierarchical clustering model, such profiles almost always lead to falling rotation curves after infall, contrary to observations.

15 pages incl 4 figs, submitted to Astrophys J Lett, uuencoded compressed postscript, preprint SCIPP 93/01-rev

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• Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows
• Dark matter in disk galaxies I: a Markov Chain Monte Carlo method and application to DDO 154
• The Missing Satellite Problem Outside of the Local Group. II. Statistical Properties of Satellites of Milky Way-like Galaxies
• Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• Escalating core formation with dark matter self-heating
• The survival of globular clusters in a cuspy Fornax
• AGN and Dwarf Galaxy Gas Kinematics
• Dark Matter at the Fermi Scale
• Investigation of two colliding solitonic cores in Fuzzy Dark Matter models
• Late decaying 2-component dark matter scenario as an explanation of the AMS-02 positron excess
• The effect of dark matter-dark radiation interactions on halo abundance -- a Press-Schechter approach
• Density Wakes due to Dynamical Friction in Cored Potentials
• The Response of Dark Matter Haloes to Gas Ejection: CuspCore II
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• The impact of propagation uncertainties on the potential Dark Matter contribution to the Fermi LAT mid-latitude gamma-ray data
• Intermittent behavior of cosmic mass field revealed by QSO's Ly_alpha forests
• Dark matter halos in the multicomponent model. I. Substructure
• Hydrodynamics of galactic dark matter
• Nonlinear resonant oscillation of gravitational potential induced by ultralight axion in $f(R)$ gravity
• A study of dark matter halos and gas properties in clusters of galaxies from ROSAT data
• New Dissipation Mechanisms from Multi-level Dark Matter Scattering
• The SLUGGS Survey: The Inner Dark Matter Density Slope of the Massive Elliptical Galaxy NGC 1407
• Subhalo sinking and off-center massive black holes in dwarf galaxies
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Extreme mass ratio inspirals in rotating dark matter spikes
• Non-Gaussian Features of Transmitted Flux of QSO's Ly$\alpha$ Absorption: Intermittent Exponent
• HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco
• Gravitino dark matter from increased thermal relic particles
• Non-Axisymmetric Structure in the Satellite Dwarf Galaxy NGC2976: Implications for its Dark/Bright Mass Distribution and Evolution
• Dynamical flows through Dark Matter Haloes II: one and two points statistics at the virial radius
• Fluctuations in strongly coupled cosmologies
• Constraining SuperWIMPy and Warm Subhalos with Future Submillilensing
• Core formation from self-heating dark matter
• Scalar Field Dark Matter mass model and evolution of rotation curves for Lsb galaxies
• A general relativistic approach to the Navarro-Frenk-White (NFW) galactic halos
• Energy transfer from baryons to dark matter as a unified solution to small-scale structure issues of the $\Lambda$CDM model
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Strongly Interacting Neutrino Portal Dark Matter
• Globular clusters as tracers of the host galaxy mass distribution: the Fornax dSph test case
• Small scale structures in coupled scalar field dark matter
• Constraint on the mass of fuzzy dark matter from the rotation curve of the Milky Way
• Testing the parametric model for self-interacting dark matter using matched halos in cosmological simulations
• The Merian Survey: Design, Construction, and Characterization of a Filter Set Optimized to Find Dwarf Galaxies and Measure their Dark Matter Halo Properties with Weak Lensing
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Asymmetric dark matter with a spontaneously broken $U(1{)}^{\prime }$: self-interaction and gravitational waves
• Probing cold dark matter subhalos with simulated ALMA observations of macrolensed sub-mm galaxies
• Pressure from dark matter annihilation and the rotation curve of spiral galaxies
• Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
• Radial structure, inflow & central mass of stationary radiative galaxy clusters
• X-ray morphology of cluster-mass haloes in self-interacting dark matter
• A Unified Fitting of HI and HeII LyαTransmitted Flux of QSO HE2347 with LCDM Hydrodynamic Simulations
• HI in the Outskirts of Nearby Galaxies
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Neutralino dark matter stars can not exist
• Dark Stars and Gravitational Waves: Topical Review
• X-Ray Shapes of Elliptical Galaxies and Implications for Self-Interacting Dark Matter
• The spacetime associated with galactic dark matter halos
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• On the dark matter haloes inner structure and galaxy morphology
• Accurate mass estimates from the proper motions of dispersion-supported galaxies
• Dynamical Models for Disk Galaxies with Triaxial Halos
• Numerical Simulations of Galaxy Formation
• An efficient positive potential-density pair expansion for modelling galaxies
• Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
• Cosmological constraints on the velocity-dependent baryon-dark matter coupling
• Constraints on conformal ultralight dark matter couplings from the European Pulsar Timing Array
• Effects of Coupled Dark Energy on the Milky Way and its Satellites
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• Self-Interacting Dark Matter and the Delay of Super-Massive Black Hole Growth
• The dark matter content of the blue compact dwarf NGC 2915
• The eccentricity enhancement effect of intermediate-mass-ratio-inspirals: dark matter and black hole mass
• The Structure of Dark Matter Halos in an Annihilating Dark Matter Model
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Globular clusters as probes of dark matter cusp-core transformations
• Dark matter cores in massive high-$z$ galaxies formed by baryonic clumps
• Sloshing of Galaxy Cluster Core Plasma in the Presence of Self-Interacting Dark Matter
• The Halo Density Profiles with Non-Standard N-body Simulations
• Cuspy dark matter density profiles in massive dwarf galaxies
• Constraints on Minimal SUSY models with warm dark matter neutralinos
• GHASP: an H$\alpha$ kinematics survey of spiral galaxies - XII. Distribution of luminous and dark matter in spiral and irregular nearby galaxies using R${}_c$-band photometry
• Global velocity field and bubbles in the BCD Mrk86
• The Structural and Kinematic Evolution of Central Star Clusters in Dwarf Galaxies and Their Dependence on Dark Matter Halo Profiles
• Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations
• Constraining neutrino-DM interactions with Milky Way dwarf spheroidals and supernova neutrinos
• Exploring Self-Interacting Dark Matter Halos with Diverse Baryonic Distributions: A Parametric Approach
• Constraints on dark matter self-interaction from galactic core size
• Universal scaling laws and density slope for dark matter haloes
• HI synthesis observations of the blue compact dwarf NGC 1705
• The Photon Spectrum of Asymmetric Dark Stars
• The Dark Matter Distributions in Low-Mass Disk Galaxies. I. H$\alpha$ Observations Using the Palomar Cosmic Web Imager
• Gravitino Dark Matter with Weak-Scale Right-Handed Sneutrino
• Chandrasekhar's Dynamical Friction and non-extensive statistics
• The degeneracy of M33 mass modelling and its physical implications
• Can we use Weak Lensing to Measure Total Mass Profiles of Galaxies on 20 kiloparsec Scales?
• EDGE: the puzzling ellipticity of Eridanus II's star cluster and its implications for dark matter at the heart of an ultra-faint dwarf
• Scope of strongly self-interacting thermal WIMPs in a minimal $U(1{)}_D$ extension and its future prospects
• Solitons and halos for self-interacting scalar dark matter
• Dark matter halo mass functions and density profiles from mass and energy cascade
• SIMPly add a dark photon
• The Effect of Multiple Cooling Channels on the Formation of Dark Compact Objects
• The Supersonic Project: The eccentricity and rotational support of SIGOs and DM GHOSts
• Constraints on Self-Interacting dark matter from relaxed galaxy groups
• The spatial distribution of satellites in galaxy clusters
• Maximum entropy distributions of dark matter in $\Lambda$CDM cosmology
• The MUSE-Faint survey. III. Constraining scalar field dark matter with Antlia B
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Early formation of supermassive black holes from the collapse of strongly self-interacting dark matter
• On the dwarf galaxies rotation curves diversity problem
• A Cusp-Core like challenge for Modified Newtonian Dynamics
• Gravitational Lensing by Galaxy Groups in the Hubble Deep Field
• Dark halo microphysics and massive black hole scaling relations in galaxies
• Cosmic constraints rule out s-wave annihilation of light dark matter
• The Distribution of Dark Matter in Galaxies: Constant-Density Dark Halos Envelop the Stellar Disks
• Threshold Drop in Accretion Density if Dark Energy is Accreting onto a Supermassive Black Hole
• Strong Dark Matter Self-Interaction from a Stable Scalar Mediator
• Andromeda XXV -- a dwarf galaxy with a low central dark matter density
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Ubiquity of density slope oscillations in the central regions of galaxy and cluster-sized systems
• MIGHTEE-HI: The radial acceleration relation with resolved stellar mass measurements
• Testing the Origins of Neutrino Mass with Supernova Neutrino Time Delay
• Observational constraint on axion dark matter in a realistic halo profile with gravitational waves
• Polytropic dark halos of elliptical galaxies
• Fate of an Accretion Disc around a Black Hole when both the Viscosity and Dark Energy is Effecting
• Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma
• On the Galactic radio signal from stimulated decay of axion dark matter
• The mass distribution in Spiral galaxies
• Testing the Collisionless Nature of Dark Matter with the Radial Acceleration Relation in Galaxy Clusters
• A 5deg x 5deg deep HI survey of the M81 group: II. HI distribution and kinematics of IC 2574 and HIJASS J1021+68
• Can tides explain the low dark matter density in Fornax?
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Coherent Self-Interactions of Dark Matter in the Bullet Cluster
• Mass Modeling the Andromeda Dwarf Galaxies: Andromeda VI and Andromeda XXIII
• Power Spectrum and Intermittency of Ly$\alpha$ Transmitted Flux of QSO He2347-4342
• Sub-horizon Perturbation Behavior in Extended Quintessence
• Central densities of dark matter halos in FIRE-2 simulations of low-mass galaxies with cold dark matter and self-interacting dark matter
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• The Maxwell--Boltzmann gas with non-standard self--interactions: a novel approach to galactic dark matter
• Naturalness and a light $Z^{\prime }$
• Flattening of dark matter cusps during mergers: model of M31
• Co-Interacting Dark Matter
• Super-Resonant Dark Matter
• Phenomenology of a two-component dark matter model
• Displaced Lepton Jet Signatures from Self-Interacting Dark Matter Bound States
• Detecting Adiabatic Contraction in Rotation Curves
• Signatures of Fuzzy Dark Matter Inside Radial Critical Curves
• Microlensing of dark matter models in the Milky Way
• Constraining Dwarf Spheroidal Dark Matter Halos With The Galactic Center Excess
• Nuclear star clusters as probes of dark matter halos: the case of the Sagittarius Dwarf Spheroidal Galaxy
• Analytical analysis of the origin of core-cusp matter density distributions in galaxies
• Cosmological Zoom-In Simulations of Milky Way Host Mass Dark Matter Halos with a Blue-Tilted Primordial Power Spectrum
• Fingerprint matching of beyond-WIMP dark matter: neural network approach
• Dark sector domain walls could explain the observed planes of satellites
• Effects of Angular Momentum on Halo Profiles
• Composite self-interacting dark matter and Higgs
• Realization of Sneutrino Self-interacting Dark Matter in the Focus Point Supersymmetry
• Barions and $\Lambda$CDM Model Problems
• Detectability of dark matter density distribution via gravitational waves from binary black holes in the Galactic center
• Cosmological scalar fields that mimic the $\Lambda CDM$ cosmological model
• Non-thermal warm dark matter limits from small-scale structure
• On the evolution process of two-component dark matter in the Sun
• From particles to orbits: precise dark matter density profiles using dynamical information
• On the Origin of the Variety of Velocity Dispersion Profiles of Galaxies
• Feedback from intermediate mass black holes on dwarf galaxy morphology at z=2
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Can dark matter see itself?
• Composite dark matter and direct-search experiments
• Stellar Profile Independent Determination of the Dark Matter Distribution of the Fornax Local Group Dwarf Spheroidal Galaxy
• Impact of the vector dark matter on polarization of the CMB photon
• Halo heating from fluctuating gas in a model dwarf
• Neutrino masses and self-interacting dark matter with mass mixing $Z-Z^{\prime }$ gauge portal
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• Dark halo densities, substructure, and the initial power spectrum
• Metamorphosis of dwarf halo density profile under dark matter decays
• 3-3-1 Self Interacting Dark Matter and the Galaxy Core-Cusp problem
• Segue 2 Recently Collided with the Cetus-Palca Stream: New Opportunities to Constrain Dark Matter in an Ultra-Faint Dwarf
• Diverse Rotation Curves of Galaxies in a Simulated Universe: the Observed Dependence on Stellar Mass and Morphology Reproduced
• Co-interacting dark matter and conformally coupled light scalars
• MONDian predictions for Newtonian M/L ratios for ultrafaint dSphs
• Cosmological Dark Matter in a Conformal Model
• Gravitational and distributed heating effects of a cD galaxy on the hydrodynamical structure of its host cluster
• On Dark Matter Self-Interactions from Higher Dimensional Gravity
• Dynamical disequilibrium in dwarf galaxies: rethinking gas dynamics, rotation curves, and dark matter inference
• Confronting global 21-cm signal with ${\mathbb{Z}}_3$ symmetric dark matter models
• Core collapse in resonant self-interacting dark matter across two decades in halo mass
• Invisible Matter
• Chameleon Gravity as an Alternative to Dark Matter
• Gravitational SIMPs
• 21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter
• Dark matter haloes in the multicomponent model. III. From dwarfs to galaxy clusters
• The Hierarchical Structure of Galactic Haloes: Generalised N-Dimensional Clustering with CluSTAR-ND
• Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Supplying Dark Energy from Scalar Field Dark Matter
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• The APOSTLE simulations: Rotation curves derived from synthetic 21-cm observations
• An Interpretable AI Framework to Disentangle Self-Interacting and Cold Dark Matter in Galaxy Clusters: The CKAN Approach
• Asymmetric Reheating by Primordial Black Holes
• Tidal stripping as a mechanism for placing globular clusters on wide orbits: the case of MGC1 in M31
• Comparison of simulations and semi-analytical model for WDM subhalo mass functions
• Structure-wide dark matter density depletion induced by local degeneracies
• CROCODILE-DWARF: Assembly and Kinematics of Field Dwarf Galaxies with GADGET4-OSAKA
• Structural parameters and possible association of the Ultra-Faint Dwarfs Pegasus III and Pisces II from deep Hubble Space Telescope photometry
• Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations
• Towards a theory of dissipative Dark Matter I: the Born limit
• Overview of the ESCAPE Dark Matter Test Science Project for Astronomers
• A Mass Dependent Density Profile from Dwarfs to Clusters
• On the Tidal Formation of Dark Matter Deficient Galaxies
• Structure Formation under Inelastic Two-Component Dark Matter: Halo Statistics and Matter Power Spectra in the High-$z$ Universe
• LYRA II: Cosmological dwarf galaxy formation with inhomogeneous Population III enrichment
• Constraining the shape of Milky Way satellites with distance gradients
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• Compact Groups in GDM Cosmological Simulations
• Universal Basic Mass Density inside Dark Matter Halos
• Broken Expectations: The Effects of Modelling Assumptions on the Inferred Dark Matter Distribution in the Milky Way's Satellites
• Effect of dark matter halos on the orbital and escape dynamics of barred galaxies
• Scattering meets absorption in dark matter detection