Halo Formation in Warm Dark Matter Models

Abstract

Discrepancies have emerged between the predictions of standard cold dark matter (CDM) theory and observations of clustering on sub-galactic scales. Warm dark matter (WDM) is a simple modification of CDM in which the dark matter particles have initial velocities due either to their having decoupled as thermal relics, or having been formed via non-equilibrium decay. We investigate the nonlinear gravitational clustering of WDM with a high resolution N-body code, and identify a number of distinctive observational signatures. Relative to CDM, halo concentrations and core densities are lowered, core radii are increased, and large halos emerge with far fewer low mass satellites. The number of small halos is suppressed, and those present are formed by `top down' fragmentation of caustics, as part of a `cosmic web' connecting massive halos. Few small halos form outside this web. If we identify small halos with dwarf galaxies, their number, spatial distribution, and formation epoch appear in better agreement with the observations for WDM than they are for CDM.

37 pages, 13 postscript files. Higher resolution and color figures available at http://astro.princeton.edu/~bode/WDM/ . Accepted by ApJ; now uses AASTeX macros

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• Towards a general parametrization of the warm dark matter halo mass function
• New mass bound on fermionic dark matter from a combined analysis of classical dSphs
• Galactic Halos in MONDian Cosmological Simulations
• Warm Dark Matter from keVins
• Galaxy Formation: Warm Dark Matter, Missing Satellites, and the Angular Momentum Problem
• A Dynamical Framework for KeV Dirac Neutrino Warm Dark Matter
• Constraints on warm dark matter from weak lensing in anomalous quadruple lenses
• The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z=1
• Beyond subhalos: Probing the collective effect of the Universe's small-scale structure with gravitational lensing
• Lyman-α Forest and Cosmic Weak Lensing in a Warm Dark Matter Universe
• Flooded Dark Matter and S Level Rise
• Testing cold dark matter with the low mass Tully-Fisher relation
• Differentiable Strong Lensing: Uniting Gravity and Neural Nets through Differentiable Probabilistic Programming
• The dark matter halos of the bluest low surface brightness galaxies
• Searches for sterile neutrinos and axionlike particles from the Galactic halo with eROSITA
• Interactions of Astrophysical Neutrinos with Dark Matter: A model building perspective
• Mixed dark matter: matter power spectrum and halo mass function
• A robust mass estimator for dark matter subhalo perturbations in strong gravitational lenses
• Testing Cold Dark Matter with the hierarchical buildup of stellar light
• The Wide Area VISTA Extra-galactic Survey (WAVES)
• The Effects of Dark Matter and Baryonic Physics on the Milky Way Subhalo Population in the Presence of the Large Magellanic Cloud
• Warm Dark Matter in B-L Inverse Seesaw
• Ringing of a black hole in a dark matter halo
• Non-minimally coupled dark matter: effective pressure and structure formation
• The Cold Dark Matter crisis on galactic and subgalactic scales
• High-precision search for dark photon dark matter with the Parkes Pulsar Timing Array
• Jeans mass-radius relation of self-gravitating Bose-Einstein condensates and typical parameters of the dark matter particle
• Self-heating dark matter via semi-annihilation
• On the isolated dwarf galaxies: from cuspy to flat dark matter density profiles and metallicity gradients
• Using CMB spectral distortions to distinguish between dark matter solutions to the small-scale crisis
• A Robust Measure of Cosmic Structure beyond the Power-Spectrum: Cosmic Filaments and the Temperature of Dark Matter
• Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
• Constraints on interacting dark energy models from galaxy Rotation Curves
• Morphological Evolution of Dwarf Galaxies in the Local Group
• Microlensing of gravitational waves by dark matter structures
• Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. II.Observational constraints on the sub-galactic matter power spectrum
• Hiding an elephant: heavy sterile neutrino with large mixing angle does not contradict cosmology
• Reheating Closed String Inflation
• Cosmological Implications of Light Sterile Neutrinos produced after the QCD Phase Transition
• Reionisation in sterile neutrino cosmologies
• Stellar mass segregation as separating classifier between globular clusters and ultra-faint dwarf galaxies
• ETHOS - an Effective Theory of Structure Formation: detecting dark matter interactions through the Lyman-$\alpha$ forest
• Cosmological searches for a non-cold dark matter component
• An almost dark galaxy with the mass of the Small Magellanic Cloud
• Light Dark Matter from Entropy Dilution
• Hidden Treasures: sterile neutrinos as dark matter with miraculous abundance, structure formation for different production mechanisms, and a solution to the sigma-8 problem
• Strongly Coupled Dark Energy Cosmologies: preserving LCDM success and easing low scale problems II - Cosmological simulations
• Signatures of Dark Matter Halo Expansion in Galaxy Populations
• BIRTH of the COSMOS Field: Primordial and Evolved Density Reconstructions During Cosmic High Noon
• Warm Dark Matter via Ultra-Violet Freeze-In: Reheating Temperature and Non-Thermal Distribution for Fermionic Higgs Portal Dark Matter
• Constraining the Warm Dark Matter Particle Mass through Ultra-Deep UV Luminosity Functions at z=2
• Evolution of linear wave dark matter perturbations in the radiation-dominant era
• The Bound Mass of Substructures in Dark Matter Halos
• Probing wave-optics effects and low-mass dark matter halos with lensing of gravitational waves from massive black holes
• Simulating the Complexity of the Dark Matter Sheet I: Numerical Algorithms
• MaGICC-WDM: the effects of warm dark matter in hydrodynamical simulations of disc galaxy formation
• Confronting fuzzy dark matter with the rotation curves of nearby dwarf irregular galaxies
• Warm Dark Matter and Cosmic Reionization
• Constraining warm dark matter with 21 cm line fluctuations due to minihalos
• Linking haloes to galaxies: how many halo properties are needed?
• The Asymptotic Form of Cosmic Structure: Small Scale Power and Accretion History
• Under the sword of Damocles: plausible regeneration of dark matter cusps at the smallest galactic scales
• Comparison between the Logotropic and $\Lambda$CDM models at the cosmological scale
• The Angular Momentum Distribution within Halos in Different Dark Matter Models
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• The 550 AU Mission: A Critical Discussion
• Gravitational Lensing by a Compound Population of Halos: Standard Models
• Extracting the Subhalo Mass Function from Strong Lens Images with Image Segmentation
• Towards constraining warm dark matter with stellar streams through neural simulation-based inference
• Dynamical constraints on the dark matter distribution of the Sculptor dwarf spheroidal from stellar proper motions
• Velocity Dispersion of the GD-1 Stellar Stream
• Lepton-number violation and right-handed neutrinos in Higgs-less effective theories
• Free streaming in mixed dark matter
• Oscillations and stability of polytropic filaments
• Alternative ideas in cosmology
• Large-Scale Velocity Dispersion and the Cosmic Web
• A Wide Field Survey of Satellite Galaxies around the Spiral Galaxy M106
• Ursa Major III/UNIONS 1: the darkest galaxy ever discovered?
• Reionization in the Warm Dark Matter Model
• Modeling star formation in dwarf spheroidal galaxies: a case for extended dark matter halos
• Dynamics of non-minimally coupled perfect fluids
• ETHOS -- An effective parametrization and classification for structure formation: the non-linear regime at $z\gtrsim 5$
• Lensing constraints on ultradense dark matter halos
• Spurious Small-Scale Structure & Discreteness-Driven Relaxation in Cosmological Simulations
• Statistics of Dark Matter Halos from the Excursion Set Approach
• On dark matter - dark radiation interaction and cosmic reionization
• Fornax globular cluster distributions: implications for the cusp-core problem
• The locations of halo formation and the peaks formalism
• Cosmic Renaissance: The First Sources of Light
• The GOGREEN survey: the internal dynamics of clusters of galaxies at redshift 0.9-1.4
• The galaxy population in cold and warm dark matter cosmologies
• Fast Identification of Bound Structures in Large N-body Simulations
• Testing the warmness of dark matter
• Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
• The Power of Halometry
• Fermionic partner of Quintessence field as candidate for dark matter
• An alternative method to generate pre-initial conditions for cosmological $N$-body simulations
• The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo
• Confronting Cold Dark Matter Predictions with Observed Galaxy Rotations
• Exploring non-cold dark matter in a scenario of dynamical dark energy with DESI DR2 data
• Constraining Warm Dark Matter and Pop III stars with the Global 21-cm Signal
• Post-inflationary axions: a minimal target for axion haloscopes
• Self-heating of Strongly Interacting Massive Particles
• The Shadow of Dark Matter
• The median density of the Universe
• The inner structure of dwarf sized halos in Warm and Cold Dark Matter cosmologies
• Molecular Chemistry for Dark Matter II: Recombination, Molecule Formation, and Halo Mass Function in Atomic Dark Matter
• Gamma rays from the neutralino dark matter annihilations in the Milky Way substructures
• The Evolution of Active Galactic Nuclei in Warm Dark Matter Cosmology
• Galaxy Formation in Sterile Neutrino Dark Matter Models
• Mixed (Cold+Warm) Dark Matter in the Bino-Wino co-annihilation scenario
• Measuring Dark Matter Substructure with Galaxy-Galaxy Flexion Statistics
• Sterile neutrinos produced near the EW scale I: mixing angles, MSW resonances and production rates
• Cosmological evolution of warm dark matter fluctuations II: Solution from small to large scales and keV sterile neutrinos
• Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
• Search for Heavy, Long-Lived Neutralinos that Decay to Photons at CDF II Using Photon Timing
• The sense of rotation of subhaloes in cosmological dark matter haloes
• An alternative to grids and glasses: Quaquaversal pre-initial conditions for N-body simulations
• The 21-cm forest as a simultaneous probe of dark matter and cosmic heating history
• Is the Universe Simpler than LCDM?
• Astrophysical Tests of Dark Matter Self-Interactions
• The PAndAS View of the Andromeda Satellite System. IV Global properties
• The detection of sub-solar mass dark matter halos
• The halo mass function in alternative dark matter models
• Observing the First Stars and Black Holes
• Bulge formation in disk galaxies with MOND
• Baryonic effects on CMB lensing and neutrino mass constraints
• Dark matter as a heavy thermal hot relic
• The PAndAS View of the Andromeda Satellite System. III. Dwarf galaxy detection limits
• Warm dark matter at small scales: peculiar velocities and phase space density
• Novel Adaptive softening for collisionless N-body simulations: Eliminating spurious halos
• The AGORA High-resolution Galaxy Simulations Comparison Project. V: Satellite Galaxy Populations In A Cosmological Zoom-in Simulation of A Milky Way-mass Halo
• Captures of Hot and Warm Sterile Antineutrino Dark Matter on EC-decaying Ho-163 Nuclei
• The Effect of Thermal Velocities on Structure Formation in N-body Simulations of Warm Dark Matter
• Magnification Bias of Distant Galaxies in the Hubble Frontier Fields: Testing Wave vs. Particle Dark Matter Predictions
• 3.5 keV X-ray line and R-Parity Conserving Supersymmetry
• The cusp-core problem in gas-poor dwarf spheroidal galaxies
• Influence of a keV sterile neutrino on neutrino-less double beta decay -- how things changed in the recent years
• Exploring extensions to the standard cosmological model and the impact of baryons on small scales
• Re-Examining Astrophysical Constraints on the Dark Matter Model
• Introducing the AIDA-TNG project: galaxy formation in alternative dark matter models
• Milky Way archaeology using RR Lyrae and type II Cepheids I. The Orphan stream in 7D using RR Lyrae stars
• Primordial black hole versus inflaton
• Angular Momentum Profiles of Warm Dark Matter Halos
• KeV Warm Dark Matter and Composite Neutrinos
• Phenomenology of quintessino dark matter -- Production of NLSP particles
• Production of heavy sterile neutrinos from vector boson decay at electroweak temperatures
• A high-resolution cosmological simulation of a strong gravitational lens
• Cold versus Warm Dark Matter simulations of a galaxy group
• Quantifying tidal stream disruption in a simulated Milky Way
• ETHOS - an effective theory of structure formation: formation of the first haloes and their stars
• Numerical investigation of lenses with substructures using the perturbative method
• Seeking Observable Imprints of Small-Scale Structure on the Properties of Dark Matter Haloes
• Global radiation signature from early structure formation
• Navarro-Frenk-White dark matter profile and the dark halos around disk systems
• The dark matter dispersion tensor in perturbation theory
• Cosmological scalar field perturbations can grow
• Real and counterfeit cores: how feedback expands halos and disrupts tracers of inner gravitational potential in dwarf galaxies
• Ejection of supermassive black holes and implications for merger rates in fuzzy dark matter haloes
• Warm dark matter from a gravitational freeze-in in extra dimensions
• The First Galaxies and the Likely Discovery of their Fossils in the Local Group
• Testing dark matter warmness and quantity via the reduced relativistic gas model
• Modified Dark Matter: Relating Dark Energy, Dark Matter and Baryonic Matter
• Local Group star formation in warm and self-interacting dark matter cosmologies
• Impact of dark matter models on the EoR 21-cm signal bispectrum
• Out of sight, out of mind? The impact of correlated clustering in substructure lensing
• The ages of stellar populations in a warm dark matter universe
• Statistics of Magnification Perturbations by Substructure in the Cold Dark Matter Cosmological Model
• The frequency of very young galaxies in the local Universe: I. A test for galaxy formation and cosmological models
• Current constraints on early and stressed dark energy models and future 21 cm perspectives
• On general features of warm dark matter with reduced relativistic gas
• Constraining SuperWIMPy and Warm Subhalos with Future Submillilensing
• On the growth of supermassive black holes formed from the gravitational collapse of fermionic dark matter cores
• Virial halo mass function in the $Planck$ cosmology
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• A heuristic wave equation parameterizing BEC dark matter halos with a quantum core and an isothermal atmosphere
• CLASH-VLT: The inner slope of the MACS J1206.2-0847 dark matter density profile
• The edge of galaxy formation III: The effects of warm dark matter on Milky Way satellites and field dwarfs
• Probing dark matter interactions with 21cm observations
• Warm Dark Haloes Accretion Histories and their Gravitational Signatures
• Supernova constraints on Multi-coupled Dark Energy
• Not All Subhaloes Are Created Equal: Modelling the Diversity of Subhalo Density Profiles in TNG50
• Ultra-deep Imaging: Structure of Disks and Haloes
• COZMIC. I. Cosmological Zoom-in Simulations with Initial Conditions Beyond Cold Dark Matter
• Is Gravitational Lensing by Intercluster Filaments Always Negligible?
• Introduction to neutrino cosmology
• The effects of the small-scale behaviour of dark matter power spectrum on CMB spectral distortion
• Challenging the Stability of Light Millicharged Dark Matter
• Non-linear clustering during the BEC dark matter phase transition
• Baryon-Interacting Dark Matter: heating dark matter and the emergence of galaxy scaling relations
• Gravitational instability with a dark matter background: Exploring the different scenarios
• Stealth decaying spin-1 dark matter
• Constraints from observational data for a running cosmological constant and warm dark matter with curvature
• The Luminosity Functions and Redshift Evolution of Satellites of Low-Mass Galaxies in the COSMOS Survey
• Dynamics of DiskMass Survey galaxies in refracted gravity
• Phenomenology of keV scale sterile neutrino dark matter with $S_4$ flavor symmetry
• Decaying warm dark matter and structure formation
• The Sejong Suite: Cosmological Hydrodynamical Simulations with Massive Neutrinos, Dark Radiation, and Warm Dark Matter
• Dark Matter Studies Entrain Nuclear Physics
• Towards testing the unitarity of the 3X3 lepton flavor mixing matrix in a precision reactor antineutrino oscillation experiment
• Constraining warm dark matter mass with cosmic reionization and gravitational wave
• Star forming filaments in warm dark matter models
• keV Warm Dark Matter via the Supersymmetric Higgs Portal
• Structural properties of artificial halos in non-standard dark matter simulations
• Degeneracies between baryons and dark matter: the challenge of constraining the nature of dark matter with JWST
• Primordial Black Hole Neutrinogenesis of Sterile Neutrino Dark Matter
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• Fuzzy Aquarius: evolution of a Milky-way like system in the Fuzzy Dark Matter scenario
• Cosmological constraints on the velocity-dependent baryon-dark matter coupling
• Toward an Improved Analytical Description of Lagrangian Bias
• Isotropic extragalactic flux from dark matter annihilations: lessons from interacting dark matter scenarios
• keV Sterile Neutrino Dark Matter and Neutrino Model Building
• Boltzmann hierarchies for self-interacting warm dark matter scenarios
• Galactic satellite systems in CDM, WDM and SIDM
• Constraints on Minimal SUSY models with warm dark matter neutralinos
• Degenerate Fermion Dark Matter from a Broken $U(1{)}_{\mathrm{B}-\mathrm{L}}$ Gauge Symmetry
• Mixed Warm Dark Matter Constraints using Milky Way Satellite Galaxy Counts
• DM particles: how warm they can be?
• Very Light Asymmetric Dark Matter
• Non-sphericity of ultralight axion dark matter haloes in the Galactic dwarf spheroidal galaxies
• Gamma-rays From Warm WIMP Dark Matter Annihilation
• Constraining structure formation using EDGES
• The ALFALFA HI velocity width function
• Constraining models for keV sterile neutrinos by quasi-degenerate active neutrinos
• Study of a viscous $\Lambda$WDM model: Near equilibrium condition, entropy production, and cosmological constraints
• The cosmology dependence of the concentration-mass-redshift relation
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Cosmological implications of a Dark Matter self-interaction energy density
• Probing sub-galactic mass structure with the power spectrum of surface-brightness anomalies in high-resolution observations of galaxy-galaxy strong gravitational lenses. I. Power-spectrum measurement and feasibility study
• Unveiling cosmological information on small scales with line intensity mapping
• Matching the mass function of Milky Way satellites in competing dark matter models
• The current status of observational cosmology
• Subhalo effective density slope measurements from HST strong lensing data with neural likelihood-ratio estimation
• Imprints of Non-thermal Wino Dark Matter on Small-Scale Structure
• Gravitationally produced Dark Matter and primordial black holes
• Using the redshift evolution of the Lyman-$\alpha$ effective opacity as a probe of dark matter models
• If dark matter is fuzzy, the first stars form in massive pancakes
• Cosmological constraints from the masses and abundances of L* galaxies
• Constraining the nature of dark matter with the star formation history of the faintest Local Group dwarf galaxy satellites
• Observational evidences of the Yukawa Potential Interacting Dark Matter
• Massive prompt cusps: A new signature of warm dark matter
• The case for mixed dark matter from sterile neutrinos
• Gravitational lensing in WDM cosmologies: The cross section for giant arcs
• Gravitational-wave event rates as a new probe for dark matter microphysics
• Fate of global symmetries in the Universe: QCD axion, quintessential axion and trans-Planckian inflaton decay-constant
• Impact of bound states on non-thermal dark matter production
• Evaluating Lyman-$\alpha$ Constraints for General Dark-Matter Velocity Distributions: Multiple Scales and Cautionary Tales
• Prospects for Detecting Gaps in Globular Cluster Stellar Streams in External Galaxies with the Nancy Grace Roman Space Telescope
• The Epoch of Assembly of Two Galaxy Groups: A comparative study
• Detecting sterile dark matter in space
• Nonlinear growth of structure in cosmologies with damped matter fluctuations
• How much cosmological information can be measured?
• The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
• Constraining Mixed Dark Matter models with high redshift Lyman-alpha forest data
• Starlight from JWST: Implications for star formation and dark matter models
• Theoretical foundations of the reduced relativistic gas in the cosmological perturbed context
• Interacting warm dark matter
• Inferring subhalo effective density slopes from strong lensing observations with neural likelihood-ratio estimation
• Statistical characteristics of observed Ly-$\alpha$ forest and the shape of initial power spectrum
• Light cold dark matter from non-thermal decay
• Jet substructure probe to unfold singlet-doublet dark matter in the presence of non-standard cosmology
• Structure Formation with Two Periods of Inflation: Beyond PLaIn $\Lambda$CDM
• Rapid onset of the 21-cm signal suggests a preferred mass range for dark matter particle
• Non-Halo Structures and their Effects on Gravitational Lensing
• Probing the Warm Dark Matter with High-z Quasar Luminosity Function
• The low mass end of the neutral gas mass and velocity width functions of galaxies in $\Lambda$CDM
• Cosmological Constraints from Fourier Phase Statistics
• Cosmology of fermionic dark matter
• Constraining the non-gravitational scattering of baryons and dark matter with early cosmic structure formation
• Modified initial power spectrum and too big to fail problem
• Deep learning-driven likelihood-free parameter inference for 21-cm forest observations
• Black hole remnants are not too fast to be dark matter
• PAC in DESI. I. Galaxy Stellar Mass Function into the $10^6{\mathrm{M}}_{\odot }$ Frontier
• Non-linear power spectra of dark and luminous matter in halo model of structure formation
• Matter in the beam: Weak lensing, substructures and the temperature of dark matter
• Universal subhalo accretion in cold and warm dark matter cosmologies
• Constraining Warm Dark Matter with high-$z$ supernova lensing
• Cosmic Birefringence from Neutrino and Dark Matter Asymmetries
• Implications of multi-axion dark matter on structure formation
• ARTEMIS emulator: exploring the effect of cosmology and galaxy formation physics on Milky Way-mass haloes and their satellites
• Time evolution of gaps in stellar streams in axisymmetric Stäckel potentials
• Small-scale clumping of dark matter and the mean free path of ionizing photons at $z=6$
• Probing the nature of Dark Matter through the metal enrichment of the intergalactic medium
• A Stochastic Theory of the Hierarchical Clustering II. Halo progenitor mass function and large-scale bias
• Anisotropic strong lensing as a probe of dark matter self-interactions
• Impact of a Warm Dark Matter late-time velocity dispersion on large-scale structures
• The Properties of Satellite Galaxies in External Systems. I. Morphology and Structural Parameters
• Theoretical Overview on the Flavor Issues of Massive Neutrinos
• Extended Stellar Components of Galaxies & the Nature of Dark Matter
• Secular evolution of galaxies and galaxy clusters in decaying dark matter cosmology
• Constraints on non-thermal Dark Matter from Planck lensing extraction
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• Anticipating the XRISM search for the decay of resonantly produced sterile neutrino dark matter
• Euclid preparation. Sensitivity to non-standard particle dark matter model
• t-channel dark matter at the LHC -- a whitepaper
• Large-Scale Structure Topology in Non-Standard Cosmologies: Impact of Dark Sector Physics
• Faster than SAM: An empirical model for the tidal evolution of dark matter substructure around strong gravitational lenses
• Warm Hawking Relics From Primordial Black Hole Domination
• A solution to the S8 tension through neutrino-dark matter interactions
• Testing black holes in a perfect fluid dark matter environment using quasinormal modes
• Self-Interacting Dark Matter in Cosmology: accurate numerical implementation and observational constraints
• Analytic approach to astrometric perturbations of critical curves by substructures
• Gravitational waves from binary black holes as probes of the structure formation history
• Testing $\Lambda$CDM With Dwarf Galaxy Morphology
• EDEN: Exploring Disks Embedded in N-body simulations of Milky-Way-mass halos from Symphony
• Trial by FIRE: Probing the dark matter density profile of dwarf galaxies with GraphNPE
• Hollow cores in Warm Dark Matter halos from the Vlasov-Poisson equation
• COZMIC. III. Cosmological Zoom-in Simulations of Self-interacting Dark Matter with Suppressed Initial Conditions
• Forecasts for Warm Dark Matter from Photometric Galaxy Surveys
• Neutrino masses in the minimal gauged $(B-L)$ supersymmetry
• N-body simulations of structure formation in thermal inflation cosmologies
• Constraining warm dark matter power spectrum using the cross-correlation of HI 21 cm signal and the Lyman-$\alpha$ forest
• Analytic Fluid Approximation for Warm Dark Matter
• Constraining Ultra Light Dark Matter with the Galactic Nuclear Star Cluster
• Inhomogenous Primordial Baryon Distributions on Sub-Galactic Scales: High-z Galaxy Formation with WDM
• Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063
• Signatures of reionization feedback in the near-infrared background
• Warm Dark Matter versus Bumpy Power Spectra
• Signatures of Bulk Neutrinos in the Early Universe
• Dark Energy, scalar-curvature couplings and a critical acceleration scale
• The Hierarchical Structure of Galactic Haloes: Classification and characterisation with Halo-OPTICS
• Return of the Lepton Number: Sterile Neutrino Dark Matter Production and the Revival of the Shi-Fuller Mechanism
• The influence of baryons on low-mass haloes
• Possible modification to standard cosmological model to resolve tension with Hubble constant values
• Bound Dark Matter (BDM) towards solving the Small Scale Structure Problem
• Cosmological Signatures of Dark Sector Physics: The Evolution of Haloes and Spin Alignment
• Warm and Cold Dark Matter in Bouncing Universe
• The Epoch of Reionization in Warm Dark Matter Scenarios
• Warm dark matter model with a few keV mass is bad for the too-big-to-fail problem
• The Dark Side of the Universe
• KMTNet Nearby Galaxy Survey: Overview and a Survey Description
• Cored DARKexp systems with finite size: numerical results
• Fingerprint matching of beyond-WIMP dark matter: neural network approach
• Signatures of Compact Halos of Sterile-Neutrino Dark Matter
• The north-south asymmetry of the ALFALFA HI velocity width function
• Clues to the nature of dark matter from first galaxies
• Measurement of Substructure from the Kinematics of the GD-1 Stellar Stream
• Galaxy formation with wave/fuzzy dark matter: The core-halo structure and the solitonic imprint
• nuMSM and its experimental tests
• Nuclear star clusters as probes of dark matter halos: the case of the Sagittarius Dwarf Spheroidal Galaxy
• Mass accretion rates and multi-scale halo environment in cold and warm dark matter cosmologies
• Sommerfeld enhancement of invisible dark matter annihilation in galaxies and galaxy clusters
• Anisotropies in the Motions and Positions of the Galactic Globular Clusters
• Effects of Cosmic Strings on Free Streaming
• Structure Formation with Warm White Noise: Effects of Finite Number Density and Velocity Dispersion in Particle and Wave Dark Matter
• Observing the very low-surface brightness dwarfs in a deep field in the VIRGO cluster: constraints on Dark Matter scenarios
• Inferring the density and membership of stellar streams with flexible models: The GD-1 stream in Gaia Data Release 3
• The Possible Equation Of State Of Dark Matter in Low Surface Brightness Galaxies
• Properties of subhalos in the interacting dark matter scenario
• Analytical warm dark matter power spectrum on small scales
• The cusp-halo relation
• DESI forecast for Dark Matter-Neutrino interactions using EFTofLSS
• Testing extensions to LCDM on small scales with forthcoming cosmic shear surveys
• Enhanced Small-Scale Structure in the Cosmic Dark Ages
• Neutrino and Collider Implications of a Left-Right Extended Zee Model
• FIMP Dark Matter in bulk viscous non-standard cosmologies
• From Large Telescopes to the MUltiplexed Survey Telescope (MUST)
• Supermassive Black Holes and Galaxy Formation
• Subhalos are Anisotropically Distributed and Aligned with the Smooth Matter Distribution of Their Host Halos
• Warm Dark Matter from Higher-Dimensional Gauge Theories
• Non-thermal warm dark matter limits from small-scale structure
• Using dust to constrain dark matter models
• Unveiling the nature and fate of the almost-dark cloud AGC 226178 through HI mapping
• Degeneracy between warm and coupled cold dark matter: A clarifying note
• Quantum Statistical Effects on Warm Dark Matter and the Mass Constraint from the Cosmic Structure at Small Scales
• The Upper Bound of the Second Higgs Boson Mass in Minimal Gauge Mediation with the Gravitino Warm Dark Matter
• Ultra-light dark matter with non-canonical kinetics reopening the mass window
• Cosmology of Single Species Hidden Dark Matter
• Implications for the missing low-mass galaxies (satellites) problem from cosmic shear
• Confronting global 21-cm signal with ${\mathbb{Z}}_3$ symmetric dark matter models
• The Milky Way's total satellite population and constraining the mass of the warm dark matter particle
• Distinguishing thermal histories of dark matter from structure formation
• Revisiting PBH accretion, evaporation and their cosmological consequences
• Constraints on dark matter models from the stellar cores observed in ultra-faint dwarf galaxies: Self-interacting dark matter
• Semi-Analytic Modeling of Dark Matter Subhalo Encounters with Thin Stellar Streams: Statistical Predictions for GD-1-like Streams in CDM
• Velocity-dependent self-interacting dark matter from thermal freeze-out and tests in direct detections
• Exploring Ultralight Scalar Assistance in Sterile Neutrino Dark Matter: Cold Spectrum and Unusual X/Gamma-ray Signatures
• Chameleon Gravity as an Alternative to Dark Matter
• On Dark Matter As A Geometric Effect in the Galactic Halo
• JERALD: high-fidelity dark matter, stellar mass and neutral hydrogen maps from fast N-body simulations
• New model of density distribution for fermionic dark matter halos
• Observational constraints on phenomenological emergent dark energy and barotropic dark matter characterized by a constant equation of state parameter
• Is it possible to unify three kinds of Dark Matters into a Kaluza-Klein Neutrino?
• Modified Cosmology or Modified Galaxy Astrophysics is Driving the z>6 JWST Results? CMB Experiments can discover the Origin in the Near Future
• 21 cm Cosmology Sensitivity to Small-Scale Structure: Warm vs Neutrino-Interacting Dark Matter
• Helium reionization in the presence of self-annihilating clumpy dark matter
• Weak lensing of bright standard sirens: prospects for ${\sigma }_8$
• Super-resolution simulation of the Fuzzy Dark Matter cosmological model
• The APOSTLE simulations: Rotation curves derived from synthetic 21-cm observations
• A neutrino model fit to the CMB power spectrum
• Cross Section Calculations in Theories of Self-Interacting Dark Matter
• Analytical modeling of the one-dimensional power spectrum of 21-cm forest based on a halo model method
• Tidal adaptive softening and artificial fragmentation in cosmological simulations
• Measuring the Dark Matter Self-Interaction Cross-Section with Deep Compact Clustering for Robust Machine Learning Inference
• New leaves of the tree: percolation analysis for cosmic web with discrete points
• Probing power spectrum enhancement at small scales with the SKA
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Constraining the shape of Milky Way satellites with distance gradients
• Modeling dark matter as self-bound quantum liquid droplets
• What can the outskirts of galaxies tell us about dark matter?
• Modeling Solitonic Cores, Stabilization of Bar, and Suppression of Bar Dissolution in DDO 168 via GPP Formalism: A Detailed Analysis of Bose--Einstein Condensate/Fuzzy Dark Matter Halo Structure and Bar Dynamics in the Dwarf Galaxy DDO 168
• Non-Standard Structure Formation Scenarios
• Warm, not Fuzzy: Generalized Ultralight Dark Matter Limits from Milky Way Satellites
• LSST Strong Lensing Systems Dark Matter Sensitivity Analysis with Neural Ratio Estimators
• Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
• CASCO: Cosmological and AStrophysical parameters from Cosmological simulations and Observations IV. Testing warm dark matter cosmologies with galaxy scaling relations: A joint simulation-observation study using DREAMS simulations
• Constraints on the velocity dispersion of Dark Matter from Cosmology and new bounds on scattering from the Cosmic Dawn
• Comparison of simulations and semi-analytical model for WDM subhalo mass functions
• Probing the warm dark matter mass with [C II] intensity mapping
• Dwarf stellar haloes: a powerful probe of small-scale galaxy formation and the nature of dark matter
• Fuzzy dark matter dynamical friction: stalling of globular clusters induced by dynamical heatings
• Overview of the ESCAPE Dark Matter Test Science Project for Astronomers
• Kolmogorov complexity in the Milky Way and its reduction with warm dark matter
• Non-halo structures and their effects on gravitationally lensed galaxies