The Structure of Dark Matter Haloes in Dwarf Galaxies

Abstract

Recent observations indicate that dark matter haloes have flat central density profiles. Cosmological simulations with non-baryonic dark matter predict however self similar haloes with central density cusps. This contradiction has lead to the conclusion that dark matter must be baryonic. Here it is shown that the dark matter haloes of dwarf spiral galaxies represent a one parameter family with self similar density profiles. The observed global halo parameters are coupled with each other through simple scaling relations which can be explained by the standard cold dark matter model if one assumes that all the haloes formed from density fluctuations with the same primordial amplitude. We find that the finite central halo densities correlate with the other global parameters. This result rules out scenarios where the flat halo cores formed subsequently through violent dynamical processes in the baryonic component. These cores instead provide important information on the origin and nature of dark matter in dwarf galaxies.

uuencoded Z-compressed postscript file, 10 pages, 3 figures included, to appear in ApJ Letters

References in corpus (1)

• Observational and Theoretical Constraints on Singular Dark Matter Halos

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• Corrective effect of many-body interactions in dynamical friction
• Probing the small-scale structure in strongly lensed systems via transdimensional inference
• Simulating Supersonic Turbulence in Galaxy Outflows
• What is the Halo Mass Function in a Fuzzy Dark Matter Cosmology?
• A Photometric and Kinematic Analysis of UDG1137+16 (dw1137+16): Probing Ultra-Diffuse Galaxy Formation in a Group Environment
• Tidal-induced lopsidedness in Magellanic-type galaxies
• "Fundamental-Plane"-Like Relations From Collisionless Stellar Dynamics: A Comparison of Mergers and Collapses
• The role of gas infall in the evolution of disc galaxies
• New mass bound on fermionic dark matter from a combined analysis of classical dSphs
• Cosmology Intertwined: A Review of the Particle Physics, Astrophysics, and Cosmology Associated with the Cosmological Tensions and Anomalies
• CLASH-VLT: Testing the Nature of Gravity with Galaxy Cluster Mass Profiles
• Jeans type instability of a complex self-interacting scalar field in general relativity
• Beyond subhalos: Probing the collective effect of the Universe's small-scale structure with gravitational lensing
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Dark Matter and the CACTUS Gamma-Ray Excess from Draco
• The dark matter halos of the bluest low surface brightness galaxies
• CLASH-VLT: Constraints on the Dark Matter Equation of State from Accurate Measurements of Galaxy Cluster Mass Profiles
• Neutrinos from captured dark matter annihilation in a galactic population of neutron stars
• Search for $\gamma$-ray emission from dark matter particle interactions from Andromeda and Triangulum Galaxies with the Fermi Large Area Telescope
• Dark matter halo cores and the tidal survival of Milky Way satellites
• Wino Dark Matter in light of the AMS-02 2015 Data
• Cosmic Ray Driven Outflows from the Large Magellanic Cloud: Contributions to the LMC Filament
• Improved $(g-2{)}_{\mu }$ Measurements and Wino/Higgsino Dark Matter
• The Cold Dark Matter crisis on galactic and subgalactic scales
• Estimating non-circular motions in barred galaxies using numerical N-body simulations
• Anisotropic cosmic optical background bound for decaying dark matter in light of the LORRI anomaly
• Constraining global properties of the Draco dwarf spheroidal galaxy
• Cosmic ray driven winds in the Galactic environment and the cosmic ray spectrum
• Observational insights on the origin of giant low surface brightness galaxies
• Towards the use of asteroseismology to investigate the nature of dark matter
• On the isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metallicity gradients
• Dark matter halos and scaling relations of extremely massive spiral galaxies from extended HI rotation curves
• Simulating the galaxy cluster "El Gordo" and identifying the merger configuration
• Probing the Milky Way's Dark Matter Halo for the 3.5 keV Line
• Mirror Matter, Mirror Gravity and Galactic Rotational Curves
• The dynamics of z~1 clusters of galaxies from the GCLASS survey
• The distribution of dark and luminous matter inferred from extended rotation curves
• Gravitational Lensing of Schwarzschild and Charged Black Holes Immersed in Perfect Fluid Dark Matter Halo
• Strong Optimized Conservative Fermi-LAT Constraints on Dark Matter Models from the Inclusive Photon Spectrum
• How Ram Pressure Drives Radial Gas Motions in the Surviving Disk
• Cosmological Inhomogeneities with Bose-Einstein Condensate Dark Matter
• Modified gravity models and the central cusp of dark matter halos in galaxies
• Mass models from high-resolution HI data of the dwarf galaxy NGC 1560
• Galaxy Kinematics and Mass Calibration in Massive SZE Selected Galaxy Clusters to z=1.3
• The angular momentum of disc galaxies: implications for gas accretion, outflows, and dynamical friction
• Gamma rays from the Galactic Centre region: a review
• The Dark Matter Distribution in the Spiral $NGC3198$ out to 0.22 $R_{vir}$
• The Kinematics and Dark Matter Fractions of TNG50 Galaxies at z=2 from an Observational Perspective
• Transforming gas-rich low-mass disky galaxies into ultra-diffuse galaxies by ram pressure
• Non-Thermal Production of WIMPs, Cosmic $e^{\pm }$ Excesses and $\gamma$-rays from the Galactic Center
• Increasing the Neutralino Relic Abundance with Slepton Coannihilations: Consequences for Indirect Dark Matter Detection
• Formation of the Small Magellanic Cloud: ancient major merger as a solution to the kinematical differences between old stars and HI gas
• Static Configurations of Dark Energy and Dark Matter
• Hobby-Eberly Telescope Observations of the Dark Halo in NGC 821
• Signatures of clumpy dark matter in the global 21 cm background signal
• Structural properties of non-spherical dark halos in Milky Way and Andromeda dwarf spheroidal galaxies
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• A Line-Of-Sight Galaxy Cluster Collision: Simulated X-Ray Observations
• The Mutual Interaction Between Population III Stars and Self-Annihilating Dark Matter
• Effective field theory interpretation of searches for dark matter annihilation in the Sun with the IceCube Neutrino Observatory
• Origin of structural and kinematical properties of the Small Magellanic Cloud
• Possibility of the Traversable Wormholes in the Galactic Halos within $4D$ Einstein-Gauss-Bonnet Gravity
• Inside-out Galaxy Formation
• On the Mass Profile of Galaxy Cluster CL 0024+1654 Inferred from Strong Lensing
• Cosmic Axion Force
• Upward muon signals at neutrino detectors as a probe of dark matter properties
• A dynamics-based density profile for dark haloes -- II. Fitting function
• Statistical properties of the dark matter haloes of dwarf galaxies and correlations with the environment
• Dynamical constraints on the dark matter distribution of the Sculptor dwarf spheroidal from stellar proper motions
• Offsets between the X-ray and the Sunyaev-Zel'dovich-effect peaks in merging galaxy clusters and their cosmological implications
• Star Formation and Feedback in Dwarf Galaxies
• The mass discrepancy-acceleration relation: a universal maximum dark matter acceleration and implications for the ultra-light scalar field dark matter model
• Collider and Dark Matter Searches in Models with Mixed Modulus-Anomaly Mediated SUSY Breaking
• A Survey of Satellite Galaxies around NGC 4258
• A Multi-frequency analysis of dark matter annihilation interpretations of recent anti-particle and gamma-ray excesses in cosmic structures
• Decaying Superheavy Dark Matter and Subgalactic Structure of the Universe
• Gamma-ray evidences of the dark matter clumps
• Search for Gamma-ray Spectral Lines from Dark Matter Annihilation up to 100 TeV towards the Galactic Center with MAGIC
• Testing the Dark Matter Interpretation of the PAMELA Excess through Measurements of the Galactic Diffuse Emission
• Dark matter profiles of SPARC galaxies: a challenge to fuzzy dark matter
• Implications of Compressed Supersymmetry for Collider and Dark Matter Searches
• Modeling star formation in dwarf spheroidal galaxies: a case for extended dark matter halos
• Strongly-Interacting Ultralight Millicharged Particles
• High-resolution three-dimensional simulations of gas removal from ultrafaint dwarf galaxies. I. Stellar feedback
• Halos of Unified Dark Matter Scalar Field
• Ruling out $\sim 100-300$ GeV thermal relic annihilating dark matter by radio observation of the Andromeda galaxy
• The Global Star-Formation Law by Supernova Feedback
• Astrophysical and cosmological probes of dark matter
• A Malin 1 'cousin' with counter-rotation: internal dynamics and stellar content of the giant low surface brightness galaxy UGC 1922
• Formation of ultra-compact dwarf galaxies: tests of the galaxy threshing scenario in Fornax
• Leptophilic dark matter in gauged $L_{\mu }-L_{\tau }$ extension of MSSM
• Fornax globular cluster distributions: implications for the cusp-core problem
• Extreme mass ratio inspirals in galaxies with dark matter halos
• Simulating Metal Mixing of Both Common and Rare Enrichment Sources in a Low Mass Dwarf Galaxy
• Hints on halo evolution in SFDM models with galaxy observations
• The connection between the cusp-to-core transformation and observational universalities of DM halos
• The continuous rise of bulges out of galactic disks
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• Formation of Dark Matter Torii Around Supermassive Black Holes Via The Eccentric Kozai-Lidov Mechanism
• Spacetime metrics and ringdown waveforms for galactic black holes surrounded by a dark matter spike
• The Power of Halometry
• Fuzzy dark matter black holes and droplets
• Dormant dwarf spheroidal galaxies, deactivated by Type Ia supernovae
• The dichotomy of dark matter fraction and total mass density slope of galaxies over five dex in mass
• Re-examining the Too-Big-To-Fail Problem for Dark Matter Haloes with Central Density Cores
• Mixed Higgsino Dark Matter from a Large SU(2) Gaugino Mass
• The Scientific Reach of Multi-Ton Scale Dark Matter Direct Detection Experiments
• Looking for a heavy wino LSP in collider and dark matter experiments
• The global mass - to - light ratio of SLACS lenses
• Indirect Detection of eV Dark Matter via Infrared Spectroscopy
• Radio emission from dark matter annihilation in the Large Magellanic Cloud
• Scalar field haloes as gravitational lenses
• Revisiting the Stellar Velocity Ellipsoid - Hubble type relation: observations versus simulations
• The Morphology of the Galactic Dark Matter Synchrotron Emission with Self-Consistent Cosmic Ray Diffusion Models
• Dark matter concentrations in galactic nuclei according to polytropic models
• Rotation Curves of Galaxies by Fourth Order Gravity
• Dark and luminous mass components of Omega Centauri with stellar kinematics
• Dynamical friction and scratches of orbiting satellite galaxies on host systems
• Extracting the Dark Matter Profile of a Relaxed Galaxy Cluster
• Embedding globular clusters in dark matter minihalos solves the cusp-core and timing problems in the Fornax dwarf galaxy
• Photometric Mass Estimation and the Stellar Mass-Halo Mass Relation for Low Mass Galaxies
• Core mass -- halo mass relation of bosonic and fermionic dark matter halos harbouring a supermassive black hole
• Gamma-Ray Dark Matter Searches in Milky Way Satellites -- A Comparative Review of Data Analysis Methods and Current Results
• Gravitational lensing by wave dark matter halos
• 3D global simulations of a cosmic-ray-driven dynamo in dwarf galaxies
• Limits to gauge coupling in the dark sector set by the non-observation of instanton-induced decay of Super-Heavy Dark Matter in the Pierre Auger Observatory data
• Galaxy Zoo: constraining the origin of spiral arms
• Self-Interacting Superfluid Dark Matter Droplets
• Supernova Enrichment of Dwarf Spheroidal Galaxies
• Observational Evidence of Evolving Dark Matter Profiles at $z\le 1$
• Building the Stellar Halo Through Feedback in Dwarf Galaxies
• Absorption Line Signatures of Gas in Mini Dark Matter Halos
• Could pressureless dark matter have pressure?
• Known Unknowns of Dark Matter Annihilation over Cosmic Time
• Horizon growth of supermassive black hole seeds fed with collisional dark matter
• Core Formation in High-z Massive Haloes: Heating by Post Compaction Satellites and Response to AGN Outflows
• Possible Connection between Dark Matter and Supermassive Black Holes
• Predictive model of fermionic dark matter halos with a quantum core and an isothermal atmosphere
• Constraining Self-Interacting Dark Matter with Dwarf Spheroidal Galaxies and High-resolution Cosmological $N$-body Simulations
• X-ray Spectra of Circumgalactic Medium Around Star-Forming Galaxies: Connecting Simulations to Observations
• UGC 1378 -- a Milky Way-sized galaxy embedded in a giant low-surface brightness disc
• Heavy dark matter particle annihilation in dwarf spheroidal galaxies: radio signals at the SKA telescope
• Effects of mass models on dynamical mass estimate: the case of ultra diffuse galaxy NGC1052-DF2
• Hadronically decaying heavy dark matter and high-energy neutrino limits
• Search for Galactic disk and halo components in the arrival directions of high-energy astrophysical neutrinos
• Ophiuchus: an optical view of a very massive cluster of galaxies hidden behind the Milky Way
• Photoionized Gas in Dark-Matter Minihalos in the Galactic Halo and Local Group
• The Failure of Self-Interacting Dark Matter to solve the Overabundance of Dark Satellites and the Soft Core Question
• Updated galactic radio constraints on Dark Matter
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• The First Billion Years project: dark matter haloes going from contraction to expansion and back again
• Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• Galaxy rotation curves and universal scaling relations: comparison between phenomenological and fermionic dark matter profiles
• Diffuse gamma-ray background and cosmic-ray positrons from annihilating dark matter
• Periodic orbits and their gravitational wave radiations in black hole with dark matter halo
• Density Wakes due to Dynamical Friction in Cored Potentials
• Dark Matter in Cosmology
• Not quite black holes as dark matter
• The Response of Dark Matter Haloes to Gas Ejection: CuspCore II
• A Baryonic Effect on the Merger Timescale of Galaxy Clusters
• Detecting Axion Dark Matter through the Radio Signal from Omega Centauri
• First supernovae in dwarf protogalaxies
• The distribution of dark matter and gas spanning six megaparsecs around the post-merger galaxy cluster MS0451-03
• Foreground effect on the $J$-factor estimation of classical dwarf spheroidal galaxies
• Towards resolving strongly-interacting dark sectors at colliders
• The CMSSM Survives Planck, the LHC, LUX-ZEPLIN, Fermi-LAT, H.E.S.S. and IceCube
• Interaction between collisionless galactic discs and nonaxissymmetric dark matter haloes
• Strong Gravitational Lensing in a Brane-World Black Hole
• A Multi-Phase Chemo-Dynamical SPH Code for Galaxy Evolution
• Constraining dark matter annihilation with cosmic ray antiprotons using neural networks
• Nonlinear resonant oscillation of gravitational potential induced by ultralight axion in $f(R)$ gravity
• Search for dark matter annihilation in the dwarf irregular galaxy WLM with H.E.S.S
• Intermittent behavior of cosmic mass field revealed by QSO's Ly_alpha forests
• A novel JEAnS analysis of the Fornax dwarf using evolutionary algorithms: mass follows light with signs of an off-centre merger
• The impact of propagation uncertainties on the potential Dark Matter contribution to the Fermi LAT mid-latitude gamma-ray data
• Zooming into the Cosmic Horseshoe: new insights on the lens profile and the source shape
• Dark halo structure in the Carina dwarf spheroidal galaxy: joint analysis of multiple stellar components
• Non-Gaussian Features of Transmitted Flux of QSO's Ly$\alpha$ Absorption: Intermittent Exponent
• Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter
• The quasinormal modes, pseudospectrum and time evolution of Proca fields in quantum Oppenheimer-Snyder-de Sitter spacetime
• Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
• The Shape of Dark Matter Haloes, V. Analysis of observations of edge-on galaxies
• Subhalo sinking and off-center massive black holes in dwarf galaxies
• Dark Matter Inelastic Up-Scattering with the Interstellar Plasma: An Exciting New Source of X-Ray Lines, including at 3.5 keV
• Navarro-Frenk-White dark matter profile and the dark halos around disk systems
• Universal profiles for radio searches of dark matter in dwarf galaxies
• Tully-Fisher Distances and Dynamical Mass Constraints for 24 Host Galaxies of Reverberation-Mapped AGN
• WALLABY Pilot Survey: First Look at the Hydra I Cluster and Ram Pressure Stripping of ESO 501-G075
• The role of baryons in self-interacting dark matter mergers
• Constraining axion and compact dark matter with interstellar medium heating
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• HSTPROMO Internal Proper Motion Kinematics of Dwarf Spheroidal Galaxies: I. Velocity Anisotropy and Dark Matter Cusp Slope of Draco
• Searching for Dark Matter Annihilation in the Smith High-Velocity Cloud
• The structure of spiral galaxies: radial profiles in stellar Mass-to-Light ratio and the Dark Matter distribution
• Dwarfs in the Milky Way halo outer rim: first in-fall or backsplash satellites?
• Cosmological perturbations during the Bose-Einstein condensation of dark matter
• It's a Breeze: The Circumgalactic Medium of a Dwarf Galaxy is Easy to Strip
• Galactic rotation dynamics in a new $f(\mathcal{R})$ gravity model
• Revisiting perfect fluid dark matter: Observational constraints from our galaxy
• Galaxy Formation in Triaxial Halos: Black Hole-Bulge-Dark Halo Correlation
• Cosmological simulations of self-interacting Bose-Einstein condensate dark matter
• Indirect dark-matter detection with MadDM v3.2 -- Lines and Loops
• Constraining annihilating dark matter by radio data of M33
• Constraints on sterile neutrino dark matter from XMM--Newton observation of M33
• Collisional dark matter density profiles around supermassive black holes
• A heuristic wave equation parameterizing BEC dark matter halos with a quantum core and an isothermal atmosphere
• Modeling the star formation in galaxies using the Chemo - dynamical SPH code
• Redshift evolution of primordial black hole merger rate
• Modeling the black holes surrounded by a dark matter halo in the galactic center of M87
• Comment on the paper "Calorimetric Dark Matter Detection with Galactic Center Gas Clouds"
• Stress-Testing Cosmic Ray Physics: The Impact of Cosmic Rays on the Surviving Disk of Ram Pressure Stripped Galaxies
• Normalized additional velocity distribution: testing the radial profile of dark matter halos and MOND
• Dark matter electron anisotropy: a universal upper limit
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Puzzling Outer-Density Profile of the Dark Matter Halo in the Andromeda Galaxy
• Discriminating power of milli-lensing observations for dark matter models
• Extragalactic diffuse gamma-rays from dark matter annihilation: revised prediction and full modelling uncertainties
• A shallow dark matter halo in Ultra Diffuse Galaxy AGC 242019: are UDGs structurally similar to low surface brightness galaxies?
• On the radial density profile of intracluster gas tracing the isothermal dark halo with a finite core
• A Counterpart to the Radial Orbit Instability in Triaxial Stellar Systems
• On self-gravitating strange dark matter halos around galaxies
• Indirect Signals from Dark Matter in Split Supersymmetry
• Diluted Axion Star Collisions with Neutron Stars
• A Giant Disk Galaxy Two Billion Years After The Big Bang
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Search for gas accretion imprints in voids: II. The galaxy Ark 18 as a result of a dwarf-dwarf merger
• Gravitational Magnus effect
• Origin of dwarf irregular galaxies with outer early-type structures
• Dissipative dark matter halos: The steady state solution
• BDM Dark Matter: CDM with a core profile and a free streaming scale
• Cusp-core problem and strong gravitational lensing
• Could compact stars in globular clusters constrain dark matter?
• Effect of Population III Multiplicity on Dark Star Formation
• Radial structure, inflow & central mass of stationary radiative galaxy clusters
• Galaxy luminosity function and Tully-Fisher relation: reconciled through rotation-curve studies
• Testing modified gravity at large distances with the HI Nearby Galaxy Survey's rotation curves
• Strong Lensing with Finite Temperature Scalar Field Dark Matter
• Dynamical friction in globular cluster-rich ultra-diffuse galaxies: the case of NGC5846-UDG1
• Foreground effect on the $J$-factor estimation of ultra-faint dwarf spheroidal galaxies
• Pressure from dark matter annihilation and the rotation curve of spiral galaxies
• The effect of non-sphericity on mass and anisotropy measurements in dSph galaxies with Schwarzschild method
• Self-gravitating Equilibria of Non-minimally Coupled Dark Matter Halos
• Galaxy chemical evolution models: The role of molecular gas formation
• Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos
• Project Dinos II: Redshift evolution of dark and luminous matter density profiles in strong-lensing elliptical galaxies across 0.1 < z < 0.9
• Disk mass and disk heating in the spiral galaxy NGC 3223
• Comparing the dark matter models, modified Newtonian dynamics and modified gravity in accounting for the galaxy rotation curves
• Analytical halo models of cosmic tidal fields
• Constraints on dark matter annihilation from the FAST observation of the Coma Berenices dwarf galaxy
• Halo Acceleration Relation
• On the dark matter haloes inner structure and galaxy morphology
• Fossil group origins. XI. The dependence of galaxy orbits on the magnitude gap
• Starburst Nuclei as Light Dark Matter Laboratories
• Do High-Velocity Clouds trace the Dark Matter subhalo population?
• The Dark Matter distribution function and Halo Thermalization from the Eddington equation in Galaxies
• A search for neutrino signal from dark matter annihilation in the center of the Milky Way with Baikal NT200
• A solution to the problems of cusps and rotation curves in dark matter halos in the cosmological standard model
• Gamma-rays From Warm WIMP Dark Matter Annihilation
• Is a Miracle-less WIMP Ruled Out?
• Dark matter halos in the multicomponent model. II. Density profiles of galactic halos
• The Celestial Buffet: multiple populations and globular cluster formation in dwarf galaxies
• $J$-factors for Velocity-dependent Dark Matter
• The Structure of Dark Matter Halos in an Annihilating Dark Matter Model
• Impact of UV Radiation from Giant Spirals on the Evolution of Dwarf Galaxies
• Neutrino astronomy as a probe of physics beyond the Standard Model: decay of sub-MeV $B$-$L$ gauge boson dark matter
• Dark matter cores in massive high-$z$ galaxies formed by baryonic clumps
• Dynamical condition of neutral hydrogen envelopes of dwarf galaxies and their possible morphological evolution
• Thermodynamics of static and stationary black holes in Einstein-Gauss-Bonnet gravity with dark matter
• Looking for Traces of Non-minimally Coupled Dark Matter in the X-COP Galaxy Clusters Sample
• The Bosma effect revisited - I. HI and stellar disc scaling models
• Influence of early dark matter halos on the primordial black holes merger rate
• The possible hierarchical scales of observed clumps in high-redshift disc galaxies
• Scaling relations for dark matter core density and radius from Chandra X-ray cluster sample
• The Formation of Binary Star Clusters in the Milky Way and Large Magellanic Cloud
• Axial Anomaly in Galaxies and the Dark Universe
• Empirical Evidence of Non-Minimally Coupled Dark Matter in the Dynamics of Local Spiral Galaxies?
• Sub-GeV Dark Matter Annihilation: Limits from Milky Way observations with INTEGRAL
• The weak dependence of velocity dispersion on disk fractions, mass-to-light ratio and redshift: Implications for galaxy and black hole evolution
• Abell 315: reconciling cluster mass estimates from kinematics, X-ray, and lensing
• Structure of visible and dark matter components in spiral galaxies at redshifts z = 0.5-0.9
• If dark matter is fuzzy, the first stars form in massive pancakes
• A test of constancy of dark matter halo surface density and radial acceleration relation in relaxed galaxy groups
• Galactic Center constraints on self-interacting sterile neutrinos from fermionic dark matter ("ino") models
• Constraining superheavy decaying dark matter with directional ultra-high energy gamma-ray limits
• Galaxy rotation curves disfavor traditional and self-interacting dark matter halos, preferring a disk component or Einasto function
• Constraints on dark matter self-interaction from galactic core size
• A spherical scalar-tensor galaxy model
• Testing multiflavored ULDM models with SPARC
• On the Origin of the Rotation Curves of Dark-Matter-Dominated Galaxies
• Gamma-Ray Constraints on the First Stars from Annihilation of Light WIMPs
• Chemodynamical gas flow cycles and their influence on the chemical evolution of dwarf irregular galaxies
• The Milky Way rotation curve in Horava - Lifshitz theory
• Probing superheavy dark matter through lunar radio observations of ultrahigh-energy neutrinos and the impacts of neutrino cascades
• Relaxation of dark matter halos: how to match observational data?
• The degeneracy of M33 mass modelling and its physical implications
• Self-gravitating equilibrium models of dwarf galaxies and the minimum mass for star formation
• Searching for Dark Matter in Messier 33
• Listening for Dark Photon Radio from the Galactic Centre
• Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC Observatory
• Origin and Evolution of Structure and Nucleosynthesis for Galaxies in the Local Group
• What made discy galaxies giant?
• Constraint on dark matter central density in the Eddington inspired Born-Infeld (EiBI) gravity with input from Weyl gravity
• Energy extraction through magnetic reconnection from a Kerr-Newman black hole in perfect fluid dark matter
• The Logotropic Dark Fluid: Observational and Thermodynamic Constraints
• Reconstructing a Model for Gravity at Large Distances from Dark Matter Density Profiles
• Gravitational Lensing by Burkert Halos
• A galactic weigh-in: mass models of SINGS galaxies using chemospectrophotometric galactic evolution models
• The 3.5 keV line from non-perturbative Standard Model dark matter balls
• Dynamical system analysis of logotropic dark fluid with a power law in the rest-mass energy density
• Constraints on annihilating dark matter in the Omega Centauri cluster
• Consequences for the Scalar Field Dark Matter model from The McGaugh Observed-Baryon Acceleration Correlation
• Solitons and halos for self-interacting scalar dark matter
• The self-confinement of electrons and positrons from dark matter
• The insight into the dark side. I. The pitfalls of the dark halo parameters estimation
• Dark Matter in split extended supersymmetry
• A Multi-frequency analysis of possible Dark Matter Contributions to M31 Gamma-Ray Emissions
• The GMRT archive atomic gas survey -- II. Mass modelling and dark matter halo properties across late-type spirals
• Core-Cusp revisited and Dark Matter Phase Transition Constrained at O(0.1) eV with LSB Rotation Curve
• Gravitational Lensing of Spherically Symmetric Black Holes in Dark Matter Halos
• Astrometric Microlensing of Primordial Black Holes with Gaia
• A new logotropic model based on a complex scalar field with a logarithmic potential
• Gamma-ray and Synchrotron Radiation from Dark Matter annihilations in Ultra-faint Dwarf Galaxies
• Electroweak Baryogenesis, Large Yukawas and Dark Matter
• Equilibrium axisymmetric halo model for the Milky Way and its implications for direct and indirect DM searches
• Gravitomagnetic corrections to the lensing deflection angle for spiral galaxy models
• Testing Grumiller's modified gravity at galactic scales
• Physical Processes in Star-Gas Systems
• Covariant formulation of refracted gravity
• $J$-factor estimation of Draco, Sculptor and Ursa Minor dwarf spheroidal galaxies with the member/foreground mixture model
• Inferring dark matter halo properties for HI-selected galaxies
• Towards understanding thermal history of the Universe through direct and indirect detection of dark matter
• Dark matter halos and the M-σrelation for supermassive black holes
• Dissipative dark matter halos: The steady state solution II
• Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
• GalRotpy: an educational tool to understand and parametrize the rotation curve and gravitational potential of disk-like galaxies
• Dark halo microphysics and massive black hole scaling relations in galaxies
• The central dark matter fraction of massive early-type galaxies
• Gravitational Lensing by Galaxy Groups in the Hubble Deep Field
• Galactic phase transition at Ec=0.11 eV from rotation curves of cored LSB galaxies and nonperturbative dark matter mass
• Dark Matter with multi-annihilation channels and AMS-02 positron excess and antiproton
• Dependence of accessible dark matter annihilation cross-sections on the density profiles of dwarf spheroidal galaxies with the Cherenkov Telescope Array
• Molecular Gas of the Most Massive Spiral Galaxies I: a Case Study of NGC 5908
• Empirical velocity profiles for galactic rotation curves
• The black hole shadow of quantum Oppenheimer-Snyder-de Sitter spacetime
• Addressing $\gamma$-ray emissions from dark matter annihilations in 45 milky way satellite galaxies and in extragalactic sources with particle dark matter models
• Cosmic constraints rule out s-wave annihilation of light dark matter
• On the dwarf galaxies rotation curves diversity problem
• Ultra light Thomas-Fermi Dark Matter
• Weakly interacting massive particle cross section limits from LOFAR observations of dwarf spheroidal galaxies
• Charged black hole surrounded by a galactic halo in de Sitter universe
• SpheCow: flexible dynamical models for galaxies and dark matter haloes
• Transonic solutions of isothermal galactic winds in a cold dark matter halo
• Transonic galactic outflows in a dark matter halo with a central black hole and its application to the Sombrero galaxy
• Upper limits on the dark matter content in globular clusters
• Scaling relations of the slightly self-interacting cold dark matter in galaxies and clusters
• An analytical approach to the dwarf galaxies cusp problem
• cp3-bench: A tool for benchmarking symbolic regression algorithms tested with cosmology
• Fluorescent rings in star-free dark matter haloes
• The Distribution of Dark Matter in Galaxies: Constant-Density Dark Halos Envelop the Stellar Disks
• Probing the Nature of the First Galaxies with JWST and ALMA
• Modelling Einstein cluster using Einasto profile
• Effect of small scale density perturbations on the formation of dark matter halo profiles
• Contribution of the first galaxies to the cosmic far-infrared/sub-millimeter background - I. Mean background level
• The Realistic Scattering of Puffy Dark Matter
• Universal dark halo scaling relation for the dwarf spheroidal satellites
• Multiwavelength analysis of low surface brightness galaxies to study possible dark matter signature
• Impact of a Warm Dark Matter late-time velocity dispersion on large-scale structures
• Dynamics of Molecular Gas in the Central Region of the Quasar IZwicky1
• New Constraints on Decaying Dark Matter from INTEGRAL/SPI
• CLMM: a LSST-DESC Cluster weak Lensing Mass Modeling library for cosmology
• Polytropic dark halos of elliptical galaxies
• Resolution of the small scale structure issues with dissipative dark matter from multiple Standard Model sectors
• NIHAO XXVIII: Collateral effects of AGN on dark matter concentration and stellar kinematics
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Discovery potential for split supersymmetry with thermal dark matter
• Exploring millicharged dark matter components from the shadows
• On the Galactic Halos Rotation by Planck Data
• Self-gravitating systems in Extended Gravity
• Self-gravitating Newtonian models of fermions with anisotropy and cutoff energy in their distribution function
• A MARVEL-ous study of how well galaxy shapes reflect Dark Matter halo shapes in Cold Dark Matter Simulations
• Present and Future constraints on Secluded Dark Matter in the Galactic Halo with TeV Gamma-ray Observatories
• Self-similar solutions for Fuzzy Dark Matter
• Constraining primordial black holes in dark matter with kinematics of dwarf galaxies
• The Effect of Interacting Dark Energy on Mass-Temperature Relation in Galaxy Clusters
• On the Galactic radio signal from stimulated decay of axion dark matter
• Constraints on metastable superheavy dark matter coupled to sterile neutrinos with the Pierre Auger Observatory
• Fitting functions for a disk-galaxy model with different LCDM-halo profiles
• The information on halo properties contained in spectroscopic observations of late-type galaxies
• Indirect detection prospects for d${}^{\ast }$(2380) dark matter
• Structure and kinematics of the polar ring galaxies: new observations and estimation of the dark halo shape
• Phenomenology of a two-component dark matter model
• On the theory of mass loss in dwarf galaxies: I - basic equations and the case of wave/thermal driven winds
• Black strings from dark matter
• Total and dark mass from observations of galaxy centers with Machine Learning
• Dark Kinetic Heating of Exoplanets and Brown Dwarfs
• Relaxing Constraints on Dark Matter Annihilation Near the Supermassive Black Hole in M87
• The dark side of early galaxies: $\text{geko}$ uncovers dark-matter fractions at $z\sim 4-6$
• Perfect fluid dark matter: a viability test with galaxy rotation curves
• Unexpected clustering pattern in dwarf galaxies challenges formation models
• A test of invariance of dark matter halo surface density using multiwavelength mock galaxy catalogues
• Dwarf galaxies with central cores in modified Newtonian dynamics (MOND) gravity
• Weak field limit for embedding gravity
• An Equilibrium Dark Matter Halo with the Burkert Profile
• Requirements to Detect the Monoenergetic Photon Signature of Thermal Cold Dark Matter in PeV-Scale Split Supersymmetry
• Mass decomposition of SLACS lens galaxies in Weyl conformal gravity
• High Velocity-dispersion Cold Gas in ULIRG Outflows. I: Direct Simulations
• Outer and inner mass distributions of the irregular galaxies UGC 4284 and UGC 11861: Constraining the baryonic content through stellar population synthesis studies
• Hollow cores in Warm Dark Matter halos from the Vlasov-Poisson equation
• Radial density and temperature profiles of the intracluster gas constructed jointly from the X-ray surface brightness measurement and the universal density profile
• Disk Mass-to-Light ratio distribution from stellar population synthesis: Application to rotation curve decomposition of NGC 5278 (KPG 390A)
• Constraints on the Dark Matter Annihilations by Neutrinos with Substructure Effects Included
• Semi analytical description of formation of galaxies and clusters of galaxies
• Constraining Dwarf Spheroidal Dark Matter Halos With The Galactic Center Excess
• Chemodynamical Modelling of Galaxy Formation and Evolution
• Shadows and Observational Images of a Schwarzschild-like Black Hole Surrounded by a Dehnen-type Dark Matter Halo
• Evolution of dwarf spheroidal satellites in the common surface-density dark halos
• Exploring sub-GeV Dark Matter Physics with Cosmic Ray and Future Telescopes
• Microlensing of dark matter models in the Milky Way
• Low surface brightness galaxies mass profiles as a consequence of galactic evolution
• Observational Manifestations of the First Protogalaxies in the 21 cm Line
• Anomalous Star-Formation Activity of Less-Luminous Galaxies in Cluster Environment
• Strong Constraints on Dark Photon and Scalar Dark Matter Decay from INTEGRAL and AMS-02 data
• Mass content of UGC 6446 and UGC 7524 through HI rotation curves: deriving the stellar discs from stellar population synthesis models
• On Filaments, Prolate Halos and Rotation Curves
• Boosting Asymmetric Charged DM via Thermalization
• On the structure of galactic halos and the microwave temperature maps
• Analytical analysis of the origin of core-cusp matter density distributions in galaxies
• Dynamical response to supernova-induced gas removal in spiral galaxies with dark matter halo
• The Impact of Dark Matter on Gravitational Wave Detection by Space-based Interferometers
• MeV scale model of SIMP dark matter, neutrino mass and leptogenesis
• HI absorption from the epoch of reionization and primordial magnetic fields
• KDG 64: a large dwarf spheroidal or a small ultradiffuse satellite of Messier 81
• Dark Matter constraints from Planck observations of the Galactic polarized synchrotron emission
• Signatures of particle decay in 21 cm absorptions from first minihalos
• Barless flocculent galaxies: a dynamic puzzle
• Redshift Horizon for Detecting the First Galaxies in Far-Infared Surveys
• The Effects of Inertial Forces on the Dynamics of Disk Galaxies
• Optimal observing strategies for velocity-suppressed dark matter annihilation
• Constraining the Secluded and Catalyzed Annihilation Dark Matter with Fermi-LAT and Planck Data
• Search for GeV-scale Dark Matter from the Galactic Center with IceCube-DeepCore
• Dynamical reconstruction of SPARC galactic halos within self-interacting fuzzy dark matter
• Cluster density slopes from Dark Matter-Baryons Energy Transfer
• Reply to "Comment on 'Scalar-tensor gravity coupled to a global monopole and flat rotation curves' "
• Sub-keV dark matter can strongly ionize molecular clouds
• Distinguishing dark matter halos with Extreme mass ratio inspirals
• Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
• Observational properties of a Schwarzschild black hole surrounded by a Dehnen-type dark matter halo
• Caustic and hydrostatic mass bias: Implications for modified gravity
• Stellar Profile Independent Determination of the Dark Matter Distribution of the Fornax Local Group Dwarf Spheroidal Galaxy
• Roche Lobe Overflow from Dwarf Stellar Systems
• The Possible Equation Of State Of Dark Matter in Low Surface Brightness Galaxies
• From particles to orbits: precise dark matter density profiles using dynamical information
• Impact of Dynamical Friction on the Tidal Formation of NGC 1052-DF2
• Reanalysis of the Systematic Uncertainties in Cosmic-Ray Antiproton Flux
• Revisiting Puffy Dark Matter with Novel Insights: Partial Wave Analysis
• Structure and mass distribution of spiral galaxies at intermediate redshifts
• Smoothed one-core and core--multi-shell regular black holes
• An Instability in Triaxial Stellar Systems
• Confronting the dark matter capture rate with a continuous gravitational wave probe of local neutron stars
• Searching for Particle Dark Matter with eROSITA Early Data
• A necessary condition for best fitting analytical to simulated density profiles in dark matter haloes
• Gamma Ray and Neutrino Flux from Annihilation of Neutralino Dark Matter at Galactic Halo Region in mAMSB Model
• Modelling Observational Constraints for Dark Matter Halos
• Dark Matter and Fundamental Physics Searches with IACTs
• Reexamine the dark matter scenario accounting for the positron excess in a new cosmic ray propagation model
• Indirect searches for dark matter with the Fermi LAT instrument
• Gravitational and distributed heating effects of a cD galaxy on the hydrodynamical structure of its host cluster
• Addressing the core-cusp and diversity problem of dwarf and disk galaxies using cold collisionless DARKexp theory
• Investigating sub-MeV dark matter annihilation to neutrinos using direct detection experiments
• Metamorphosis of dwarf halo density profile under dark matter decays
• Study of Various Dark Matter Halo Profiles in Milky Way and M31 Galaxies within the Standard Cosmology Framework
• New probe of modified gravity
• 3-3-1 Self Interacting Dark Matter and the Galaxy Core-Cusp problem
• Ring Formation from an Oscillating Black Hole
• On the radial acceleration of disk galaxies
• Prospects for annihilating dark matter from M31 and M33 observations with the Cherenkov Telescope Array
• Self-gravitating clusters of Bose-Einstein gas with planar, cylindrical, or spherical symmetry: gaseous density profiles and onset of condensation
• General circular velocity relation of a test particle in a 3D gravitational potential: application to the rotation curves analysis and total mass determination of UGC 8490 and UGC 9753
• Constraints on superheavy dark matter decaying into $h\nu$, $Z\nu$ and $W\ell$ -- Benchmark example within an extended seesaw framework
• Searching for Dark Matter Annihilation with IceCube and P-ONE
• Direct and Indirect Detection of Neutralino Dark Matter and Collider Signatures in an $SO(10)$ Model with Two Intermediate Scales
• Testing the predictions of axisymmetric distribution functions of galactic dark matter with hydrodynamical simulations
• A numerical fit of analytical to simulated density profiles in dark matter haloes
• Ringdown of a black hole sourced by a Burkert-density effective anisotropic source
• A test of invariance of halo surface density for FIRE-2 simulations with cold dark matter and self-interacting dark matter
• LHAASO Galactic Plane $\gamma$-rays Strongly Constrain Heavy Dark Matter
• On the Energy Distribution of the Galactic Center Excess' Sources
• Can hidden correlations mimic a variable fine structure constant?
• Scalarization and superradiant instability of black hole induced by dark matter halo in the scalar-tensor theory of gravity
• New model of density distribution for fermionic dark matter halos
• Cusped Mass Density Profiles and Magnification Ratios of Double Image Gravitational Lenses
• The mass profile of NGC 3377 from a Bayesian approach
• Effects of non-vanishing dark matter pressure in the Milky Way galaxy
• Can dark-matter Q-balls grow to the mass gap masses?
• Effect of dark matter halo substructures on galaxy rotation curves
• Data-driven modeling of rotation curves with artificial neural networks
• GammaBayes: a Bayesian pipeline for dark matter detection with CTA
• The dark halo of the Hydra I galaxy cluster: core, cusp, cosmological? Dynamics of NGC 3311 and its globular cluster system
• Astrophysical Constraints on Dark Matter
• Gravitational and mass distribution effects on stationary superwinds
• On the role of dust in the microwave emission of galactic halos
• The baryonic self similarity of dark matter
• Rotation Curves in z~1-2 Star-Forming Disks: Comparison of Dark Matter Fractions and Disk Properties for Different Fitting Methods
• Non-Thermal Dark Matter, High Energy Cosmic Rays and Late-Decaying Particles From Inflationary Quantum Fluctuations
• Baryon-driven decontraction in Milky Way mass haloes
• Detecting Dark Photons from Atomic Rearrangement in the Galaxy
• Helium reionization in the presence of self-annihilating clumpy dark matter
• Origin of Weak MgII and Higher Ionization Absorption Lines in an Outflow from an Intermediate-Redshift Dwarf Satellite Galaxy
• Modeling Dark Matter Halos with Nonlinear Field Theories
• A Model for Dark Matter Halos
• Systematic variation of central mass density slope in early-type galaxies
• Origin of the spectacular tidal shells of galaxy NGC474
• Studying dark matter with MadDM: lines and loops
• On the Tidal Formation of Dark Matter Deficient Galaxies
• Comparison of Modeling SPARC spiral galaxies' rotation curves: halo models vs MOND
• A Mass Dependent Density Profile from Dwarfs to Clusters
• Imprints of tidal interactions on the stellar distribution of satellite galaxies: implications for dark matter deficient galaxies
• Distinguishing Dark Matter Cusps from Cores using Globular Clusters
• Chemo-dynamical Evolution of the ISM in Galaxies
• Structure-wide dark matter density depletion induced by local degeneracies
• Tensorial solution of the Poisson equation and the dark matter amount and distribution of UGC 8490 and UGC 9753
• On the Presence of Angular-Velocity Offsets in Disk Galaxies
• Dark matter detection in gamma astroparticle experiments
• Uncertainty-Aware Neural Networks for Fuzzy Dark Matter Model Selection from \texorpdfstring{$x_{\mathrm{HI}}$}{x_HI} Measurements
• Universal Basic Mass Density inside Dark Matter Halos
• Determination of the best dark matter profile for the Milky Way with Gaia DR3 using Bayesian Model Comparison
• Starbursts in isolated galaxies. I. The influence of stellar birth function and IMF
• The potential of diffuse Galactic Ridge neutrino measurements to constrain dark matter
• Boson dark matter halos with a dominant noncondensed component
• Extragalactic Searches for Dark Matter Annihilation
• Bulge formation from SSCs in a responding cuspy dark matter halo
• Combined analyses of the antiproton production from cosmic-ray interactions and its possible dark matter origin
• Gravitational emissions and light curves of quasi-periodic orbits in Schwarzschild spacetime embedded in a Dehnen-type dark matter halo