Dark matter and cosmic structure

Abstract

We review the current standard model for the evolution of cosmic structure, tracing its development over the last forty years and focusing specifically on the role played by numerical simulations and on aspects related to the nature of dark matter.

Invited review in Annalen der Physik - www.ann-phys.org

References in corpus (157)

• Measurements of Omega and Lambda from 42 High-Redshift Supernovae
• A Universal Density Profile from Hierarchical Clustering
• The Structure of Cold Dark Matter Halos
• Simulating the joint evolution of quasars, galaxies and their large-scale distribution
• The many lives of active galactic nuclei: cooling flows, black holes and the luminosities and colours of galaxies
• Dark Matter Substructure in Galactic Halos
• Where are the missing galactic satellites?
• Populating a cluster of galaxies - I. Results at z=0
• A Flat Universe from High-Resolution Maps of the Cosmic Microwave Background Radiation
• The broken hierarchy of galaxy formation
• The 2dF Galaxy Redshift Survey: Spectra and redshifts
• Cosmological SPH simulations: A hybrid multi-phase model for star formation
• The Formation of Galactic Disks
• Observational evidence for self-interacting cold dark matter
• Stable clustering, the halo model and nonlinear cosmological power spectra
• Halo Models of Large Scale Structure
• The Aquarius Project: the subhalos of galactic halos
• Toward a halo mass function for precision cosmology: the limits of universality
• Ellipsoidal collapse and an improved model for the number and spatial distribution of dark matter haloes
• Mass function of dark matter halos
• The hierarchical formation of the brightest cluster galaxies
• An analytic model for the spatial clustering of dark matter haloes
• Too big to fail? The puzzling darkness of massive Milky Way subhaloes
• MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on angular scales of 10 arcminutes to 5 degrees
• From dwarf spheroidals to cDs: Simulating the galaxy population in a LCDM cosmology
• How Filaments are Woven into the Cosmic Web
• Analytic model for galaxy and dark matter clustering
• The Inner Structure of LambdaCDM Halos III: Universality and Asymptotic Slopes
• At the heart of the matter: the origin of bulgeless dwarf galaxies and Dark Matter cores
• The Inner Structure of LambdaCDM Halos I: A Numerical Convergence Study
• Halo occupation numbers and galaxy bias
• Clustering of Galaxies in a Hierarchical Universe: I. Methods and Results at z=0
• Response of dark matter halos to condensation of baryons: cosmological simulations and improved adiabatic contraction model
• Resolving Cosmic Structure Formation with the Millennium-II Simulation
• Reionization and the abundance of galactic satellites
• The physics driving the cosmic star formation history
• The Diversity and Similarity of Simulated Cold Dark Matter Halos
• Triaxial Modeling of Halo Density Profiles with High-resolution N-body Simulations
• A Recipe for Galaxy Formation Shaun Cole
• How supernova feedback turns dark matter cusps into cores
• Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions
• The large-scale structure of the Universe
• The statistics of LCDM Halo Concentrations
• Merger rates in hierarchical models of galaxy formation. II: Comparison with N-body simulations
• Accurate masses for dispersion-supported galaxies
• A Universal Mass Profile for Dwarf Spheroidal Galaxies?
• The subhalo populations of LCDM dark haloes
• The role of sterile neutrinos in cosmology and astrophysics
• The Merger Rates and Mass Assembly Histories of Dark Matter Haloes in the Two Millennium Simulations
• The Structure of Dark Matter Haloes in Hierarchical Clustering Models
• The Cores of Dwarf Galaxy Halos
• Direct Detection of CDM Substructure
• The Shape of Dark Matter Halos: Dependence on Mass, Redshift, Radius, and Formation
• Formation and evolution of galaxy dark matter halos and their substructure
• The Dependence of Halo Clustering on Halo Formation History, Concentration, and Occupation
• Evolution of structure in cold dark matter universes
• Precision Determination of the Mass Function of Dark Matter Halos
• Observation of muon neutrino disappearance with the MINOS detectors and the NuMI neutrino beam
• Dark Matter Halos within Clusters
• Evidence for substructure in lens galaxies?
• The redshift dependence of the structure of massive LCDM halos
• A novel determination of the local dark matter density
• The Nature of Galaxy Bias and Clustering
• Accurate universal models for the mass accretion histories and concentrations of dark matter halos
• The spin and shape of dark matter haloes in the Millennium simulation of a LambdaCDM universe
• The Observed properties of Dark Matter on small spatial scales
• The Power Spectrum Dependence of Dark Matter Halo Concentrations
• The effects of galaxy formation on the matter power spectrum: A challenge for precision cosmology
• Can Photoionization Squelching Resolve the Sub-structure Crisis?
• The dark and baryonic matter content of low surface brightness disk galaxies
• Haloes gone MAD: The Halo-Finder Comparison Project
• Mass loss from dwarf spheroidal galaxies: the origins of shallow dark matter cores and exponential surface brightness profiles
• The haloes of bright satellite galaxies in a warm dark matter universe
• Quantifying the heart of darkness with GHALO - a multi-billion particle simulation of our galactic halo
• The Effects of Photoionization on Galaxy Formation - II: Satellites in the Local Group
• A Map of the Universe
• Gravitational detection of a low-mass dark satellite at cosmological distance
• The Linear Theory Power Spectrum from the Lyman-alpha Forest in the Sloan Digital Sky Survey
• A New Milky Way Companion: Unusual Globular Cluster or Extreme Dwarf Satellite?
• Compound gravitational lensing as a probe of dark matter substructure within galaxy halos
• Internal and External Alignment of the Shapes and Angular Momenta of LCDM Halos
• Stellar Feedback in Dwarf Galaxy Formation
• The halo mass function from the dark ages through the present day
• Assembly bias in the clustering of dark matter haloes
• The observed ionization rate of the intergalactic medium and the ionizing emissivity at z >5: Evidence for a photon starved and extended epoch of reionization
• Galaxy Evolution in Cosmological Simulations With Outflows I: Stellar Masses and Star Formation Rates
• Halo assembly bias and its effects on galaxy clustering
• Hierarchical galaxy formation and substructure in the Galaxy's stellar halo
• The Phase-Space Density Profiles of Cold Dark Matter Halos
• GALICS I: A hybrid N-body semi-analytic model of hierarchical galaxy formation
• Galaxies in LCDM with Halo Abundance Matching: luminosity-velocity relation, baryonic mass-velocity relation, velocity function and clustering
• Detection of a Dark Substructure through Gravitational Imaging
• Discovery of an Unusual Dwarf Galaxy in the Outskirts of the Milky Way
• Galaxy Formation and Large-Scale Bias
• Cosmological puzzle resolved by stellar feedback in high redshift galaxies
• The Milky Way's satellite population in a LambdaCDM universe
• The Origin of Disks and Spheroids in Simulated Galaxies
• Weakly Self-Interacting Dark Matter and the Structure of Dark Halos
• A blueprint for detecting supersymmetric dark matter in the Galactic halo
• Cores in warm dark matter haloes: a Catch 22 problem
• Galaxies-Intergalactic Medium Interaction Calculation --I. Galaxy formation as a function of large-scale environment
• Mass and Redshift Dependence of Dark Halo Structure
• Masses for the Local Group and the Milky Way
• Galaxy growth in the concordance $\Lambda$CDM cosmology
• The effect of neutrinos on the matter distribution as probed by the Intergalactic Medium
• Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
• Statistics of Physical Properties of Dark Matter Clusters
• A Pair of Bootes: A New Milky Way Satellite
• Semi-analytical model of galaxy formation with high-resolution N-body simulations
• How cold is cold dark matter? Small scales constraints from the flux power spectrum of the high-redshift Lyman-alpha forest
• A universal density slope - velocity anisotropy relation for relaxed structures
• Luminosity function and radial distribution of Milky Way Satellites in a LCDM Universe
• Maximum Feedback and Dark Matter Profiles of Dwarf Galaxies
• Shapes and Alignments of Galaxy Cluster Halos
• Halo Cores and Phase Space Densities: Observational Constraints on Dark Matter Physics and Structure Formation
• The velocity function in the local environment from LCDM and LWDM constrained simulations
• The dependence of dark halo clustering on the formation epoch and the concentration parameter
• How universal are the density profiles of dark halos?
• The velocity width function of galaxies from the 40% ALFALFA survey: shedding light on the cold dark matter overabundance problem
• The Dark Matter Annihilation Signal from Galactic Substructure: Predictions for GLAST
• Assembly History and Structure of Galactic Cold Dark Matter Halos
• Dwarf spheroidal galaxy kinematics and spiral galaxy scaling laws
• The Shapes and Alignments of Dark Matter Halos
• One simulation to fit them all - changing the background parameters of a cosmological N-body simulation
• Dark matter response to galaxy formation
• Kinematics of Milky Way Satellites in a Lambda Cold Dark Matter Universe
• On the Baryon Fractions in Clusters and Groups of Galaxies
• Assembly bias and the dynamical structure of dark matter halos
• The Dark Matter Distribution in Abell 383: Evidence for a Shallow Density Cusp from Improved Lensing, Stellar Kinematic and X-ray Data
• Connection between Newtonian simulations and general relativity
• Prospects of detecting gamma-ray emission from galaxy clusters: cosmic rays and dark matter annihilations
• Galaxy formation using halo merger histories taken from N-body simulations
• Early structure in LCDM
• The fine-grained phase-space structure of Cold Dark Matter halos
• Streams and caustics: the fine-grained structure of LCDM haloes
• The Dependence of the Occupation of Galaxies on the Halo Formation Time
• Cosmological and astrophysical constraints from the Lyman-alpha forest flux probability distribution function
• The origin of failed subhaloes and the common mass scale of the Milky Way satellite galaxies
• Are mergers responsible for universal halo properties?
• On the Effects of Line-of-Sight Structures on Lensing Flux-ratio Anomalies in a LCDM Universe
• The angular momentum of cold dark matter haloes with and without baryons
• Galaxy Groups in the 2dFGRS: the number density of groups
• Accurate determination of the Lagrangian bias for the dark matter halos
• Quantifying the Cosmic Web I: The large-scale halo ellipticity-ellipticity and ellipticity-direction correlations
• Spin flips I: Evolution of the angular momentum orientation of Milky Way-mass dark matter haloes
• Dark-Halo Cusp: Asymptotic Convergence
• Galaxy Clustering Topology in the Sloan Digital Sky Survey Main Galaxy Sample: a Test for Galaxy Formation Models
• On the Origin of the Inner Structure of Halos
• Substructure Lensing: Effects of Galaxies, Globular Clusters & Satellite Streams
• Theoretical dark matter halo density profile
• Bound and unbound substructures in Galaxy-scale Dark Matter haloes
• Satellite galaxies in hydrodynamical simulations of Milky Way sized galaxies
• Dark Matter Caustics
• Abundances, masses, and weak-lensing mass profiles of galaxy clusters as a function of richness and luminosity in LambdaCDM cosmologies
• Particle Annihilation in Cold Dark Matter Micropancakes
• A group-galaxy cross-correlation function analysis in zCOSMOS
• Sterile neutrinos in cosmology and how to find them in the lab

Cited by in corpus (283)

• Small-Scale Challenges to the $\Lambda$CDM Paradigm
• A History of Dark Matter
• The Connection between Galaxies and their Dark Matter Halos
• Theoretical Challenges in Galaxy Formation
• WIMP dark matter candidates and searches - current status and future prospects
• A New Era in the Quest for Dark Matter
• The properties of warm dark matter haloes
• Direct Detection of WIMP Dark Matter: Concepts and Status
• EMERGE - An empirical model for the formation of galaxies since $z\sim 10$
• Streams, substructures and the early history of the Milky Way
• Sterile Neutrino Dark Matter
• Secular Evolution in Disk Galaxies
• Cosmological and Solar System Consequences of f(R,T) Gravity Models
• f(R,T) Cosmological Models in Phase Space
• The flattening of the concentration-mass relation towards low halo masses and its implications for the annihilation signal boost
• The Mass Profile and Accretion History of Cold Dark Matter Halos
• Structure Finding in Cosmological Simulations: The State of Affairs
• The impact of galaxy formation on the total mass, mass profile and abundance of haloes
• Large-scale dark matter simulations
• Constraining the WDM Particle Mass with Milky Way Satellites
• Using the Milky Way satellites to study interactions between cold dark matter and radiation
• From galactic bars to the Hubble tension: weighing up the astrophysical evidence for Milgromian gravity
• ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume
• The COpernicus COmplexio: Statistical Properties of Warm Dark Matter Haloes
• The total satellite population of the Milky Way
• Baryonic impact on the dark matter distribution in Milky Way-size galaxies and their satellites
• Jeans Analysis for Dwarf Spheroidal Galaxies in Wave Dark Matter
• Sensitivity Projections for Dark Matter Searches with the Fermi Large Area Telescope
• Structure formation in large-volume cosmological simulations of fuzzy dark matter: Impact of the non-linear dynamics
• Testing the Strong Equivalence Principle: Detection of the External Field Effect in Rotationally Supported Galaxies
• The metallicity bimodality of globular cluster systems: a test of galaxy assembly and of the evolution of the galaxy mass-metallicity relation
• Low-mass halo perturbations in strong gravitational lenses at redshift z$\sim$0.5 are consistent with CDM
• The Cosmic Ballet: spin and shape alignments of haloes in the cosmic web
• Black Hole and Galaxy Coevolution from Continuity Equation and Abundance Matching
• The effect of baryons on redshift space distortions and cosmic density and velocity fields in the EAGLE simulation
• The Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• The Copernicus Complexio: a high-resolution view of the small-scale Universe
• Fundamental Particle Structure in the Cosmological Dark Matter
• Faint dwarfs as a test of DM models: WDM vs. CDM
• The Three Hundred Project: Backsplash galaxies in simulations of clusters
• The asymptotic tidal remnants of cold dark matter subhalos
• The phase space density of fermionic dark matter haloes
• No cores in dark matter-dominated dwarf galaxies with bursty star formation histories
• The failures of the standard model of cosmology require a new paradigm
• An adaptively refined phase-space element method for cosmological simulations and collisionless dynamics
• Constraints on the identity of the dark matter from strong gravitational lenses
• Substructure and galaxy formation in the Copernicus Complexio warm dark matter simulations
• Density profiles of ultracompact minihalos: Implications for constraining the primordial power spectrum
• Axion-like Relics: New Constraints from Old Comagnetometer Data
• Are ultracompact minihalos really ultracompact?
• Enhanced tidal stripping of satellites in the galactic halo from dark matter self-interactions
• The impact of baryonic discs on the shapes and profiles of self-interacting dark matter halos
• Conserved actions, maximum entropy and dark matter halos
• Cosmological evolution of a complex scalar field with repulsive or attractive self-interaction
• LoCuSS: Pre-processing in galaxy groups falling into massive galaxy clusters at z=0.2
• A general explanation on the correlation of dark matter halo spin with the large scale environment
• Numerical resolution limits on subhalo abundance matching
• Resonant Sterile Neutrino Dark Matter in the Local and High-z Universe
• Dynamical models for the Sculptor dwarf spheroidal in a Lambda CDM universe
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• WIMP searches with gamma rays in the Fermi era: challenges, methods and results
• An observer's guide to the (Local Group) dwarf galaxies: predictions for their own dwarf satellite populations
• The Main Sequences of Starforming Galaxies and Active Galactic Nuclei at High Redshift
• A model for AGN variability on multiple timescales
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• Sterile neutrino Dark Matter production from scalar decay in a thermal bath
• TheHaloMod: An online calculator for the halo model
• CosmicGrowth Simulations---Cosmological simulations for structure growth studies
• Glueball scattering cross section in lattice SU(2) Yang-Mills theory
• From cusps to cores: a stochastic model
• The impact of the phase-space density on the indirect detection of dark matter
• Terrestrial and Martian Heat Flow Limits on Dark Matter
• The contribution of N-rich stars to the Galactic stellar halo using APOGEE red giants
• The Search for Dark Matter
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Implications of hydrodynamical simulations for the interpretation of direct dark matter searches
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• Compact bifluid hybrid stars: Hadronic Matter mixed with self-interacting fermionic Asymmetric Dark Matter
• Dark Atoms and Puzzles of Dark Matter Searches
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• On Ellipsoidal Collapse and Primordial Black-Hole Formation
• Warm FIRE: Simulating Galaxy Formation with Resonant Sterile Neutrino Dark Matter
• The effect of fluctuating fuzzy axion haloes on stellar dynamics: a stochastic model
• Subhaloes gone Notts: Spin across subhaloes and finders
• The velocity anisotropy of the Milky Way satellite system
• Cold or Warm? Constraining Dark Matter with Primeval Galaxies and Cosmic Reionization after Planck
• Dark Matter in the Local Universe
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• The phase-space structure of tidally stripped halos
• On the Quantum-To-Classical Transition for Ekpyrotic Perturbations
• Measuring subhalo mass in redMaPPer clusters with CFHT Stripe 82 Survey
• The tangential velocity excess of the Milky Way satellites
• Pre-processing, group accretion and the orbital trajectories of associated subhaloes
• A Comparative Analysis of the Chemical Compositions of Gaia-Enceladus/Sausage and Milky Way Satellites using APOGEE
• Searches for sterile neutrinos and axionlike particles from the Galactic halo with eROSITA
• Warm Dark Matter in B-L Inverse Seesaw
• Hadronic and hadron-like physics of Dark Matter
• LCDM halo substructure properties revealed with high resolution and large volume cosmological simulations
• A new direction for dark matter research: intermediate mass compact halo objects
• Inferring high redshift large-scale structure dynamics from the Lyman-alpha forest
• Ab initio nuclear response functions for dark matter searches
• Tidal Stripping in the Adiabatic Limit
• Probing massless and massive gravitons via entanglement in a warped extra dimension
• Coherent and incoherent structures in fuzzy dark matter halos
• Scalarons mimicking Dark Matter in the Hu-Sawicki model of f(R) gravity
• The Phase Space Structure of Dark Matter Halos
• Testing strong lensing subhalo detection with a cosmological simulation
• Cosmological consequences and statefinder diagnosis of a non-interacting generalized Chaplygin gas in $f(R,T)$ gravity
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Simulating the Complexity of the Dark Matter Sheet I: Numerical Algorithms
• Cosmic CARNage I: on the calibration of galaxy formation models
• Constraining the inner density slope of massive galaxy clusters
• Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
• Constraining warm dark matter with 21 cm line fluctuations due to minihalos
• Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
• The twisted dark matter halo of the Milky Way
• Testing the Prediction of Fuzzy Dark Matter Theory in the Milky Way Center
• The abundance of dwarf galaxies around low-mass giants in the Local Volume
• The optimal gravitational softening length for cosmological N-body simulations
• Testing MONDian Dark Matter with Galactic Rotation Curves
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
• Radial velocities and stellar population properties of 56 MATLAS dwarf galaxies observed with MUSE
• Revealing modified gravity signal in matter and halo hierarchical clustering
• The galaxy population in cold and warm dark matter cosmologies
• Cosmological tests of modified gravity: constraints on $F(R)$ theories from the galaxy clustering ratio
• Search for Bosonic Super-WIMP Interactions with the XENON100 Experiment
• Exploring properties of long-lived particles in inelastic dark matter models at Belle II
• Gravitationally Bound Bose Condensates with Rotation
• The bivariate gas-stellar mass distributions and the mass functions of early- and late-type galaxies at $z\sim 0$
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• An alternative method to generate pre-initial conditions for cosmological $N$-body simulations
• The segregation of baryons and dark matter during halo assembly
• Constraining interacting dark energy models with the halo concentration-mass relation
• Challenges for Lambda-CDM and MOND
• A Deeper Look at DES Dwarf Galaxy Candidates: Grus I and Indus II
• Is the Universe Simpler than LCDM?
• Emergent gravity in galaxies and in the Solar System
• The Three Hundred project: Galaxy groups do not survive cluster infall
• The Second Nucleus of NGC 7727: Direct Evidence for the Formation and Evolution of an Ultracompact Dwarf Galaxy
• A dynamical system representation of generalized Rastall gravity
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• Subhaloes gone Notts: the clustering properties of subhaloes
• The Schrödinger-Poisson method for Large-Scale Structure
• Hydrodynamical structure formation in Milgromian cosmology
• Observation of the new emission line at ~3.5 keV in X-ray spectra of galaxies and galaxy clusters
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Fixing a Rigorous Formalism for the Accurate Analytic Derivation of Halo Properties
• Singlet-Doublet Dirac Dark Matter and Neutrino Masses
• Impact of dark matter models on the EoR 21-cm signal bispectrum
• Ejection of supermassive black holes and implications for merger rates in fuzzy dark matter haloes
• Gravitational collapse in the Schrödinger-Poisson system
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• Cosmic structures from a mathematical perspective 1. Dark matter halo mass density profiles
• Deflection angle, quasinormal modes and optical properties of a de Sitter black hole in $f(\mathcal{T},\mathcal{B})$ gravity
• Thermal production of cold "hot dark matter" around eV
• Tidal Stripping and Post-Merger Relaxation of Dark Matter Halos: Causes and Consequences of Mass Loss
• Warm Dark Haloes Accretion Histories and their Gravitational Signatures
• Shedding light on low-mass subhalo survival and annihilation luminosity with numerical simulations
• Simulating the LOcal Web (SLOW) II: Properties of local galaxy clusters
• Impact of substructure on local dark matter searches
• Determination of the abundance of cosmic matter via the cell count moments of the galaxy distribution (1)
• Micro galaxies in LCDM
• Two interacting current model of holographic Dirac fluid in graphene
• Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. IV. High Precision Constraints on the Evolution of Stellar-Halo Mass Relation at Redshift $z<0.7$
• High Precision Calculations of the Higgs Boson Mass
• Chemo-dynamical simulations of dwarf galaxy evolution
• Star forming filaments in warm dark matter models
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Mass assembly history and infall time of the Fornax dwarf spheroidal galaxy
• Transient Weak-Lensing by Cosmological Dark Matter Microhaloes
• Cosmological Probes for Supersymmetry
• Culminating the peak CUSP to descry the dark side of halos
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• Constraints on the Sommerfeld-enhanced dark matter annihilation from the gamma rays of subhalos and dwarf galaxies
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Cosmic Voids in Evolving Dark Sector Cosmologies: the High Redshift Universe
• Universal scaling laws and density slope for dark matter haloes
• Shan--Chen interacting vacuum cosmology
• Tracking the orbit of unresolved subhalos for semi-analytic models
• A Stochastic Theory of the Hierarchical Clustering I. Halo Mass Function
• The Tessellation-Level-Tree: characterising the nested hierarchy of density peaks and their spatial distribution in cosmological N-body simulations
• Circular polarization of cosmic photons due to their interactions with Sterile neutrino dark matter
• Gravitational Collapse of Baryonic and Dark matter
• Probes for Dark Matter Physics
• Testing Modified Dark Matter with Galaxy Clusters: Does Dark Matter know about the Cosmological Constant?
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Tip of the red giant branch distance to the nearby dwarf galaxy [TT2009] 25 in the NGC 891 group
• Big Bounce Genesis and Possible Experimental Tests -- A Brief Review
• Statistical ensembles of virialized halo matter density profiles
• MaNGA DynPop -- IV. Stacked total density profile of galaxy groups and clusters from combining dynamical models of integral-field stellar kinematics and galaxy-galaxy lensing
• The interacting vacuum and tensions: a comparison of theoretical models
• Dark matter halo mass functions and density profiles from mass and energy cascade
• Thermal Fluctuations of Dark Matter in Bouncing Cosmology
• Hα Dots: Direct-Method Metal Abundances of Low-Luminosity Star-Forming Systems
• Determining Satellite Infall Times Using Machine Learning
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• Condensation of Galactic Cold Dark Matter
• The Last Journey. II. SMACC -- Subhalo Mass-loss Analysis using Core Catalogs
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
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• Dark matter reflection of particle symmetry
• A Dwarf Disrupting -- Andromeda XXVII and the North West Stream
• On the Apparent Power Law in CDM Halo Pseudo Phase Space Density Profiles
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• Discovery of a Rare Group of Dwarf Galaxies in the Local Universe
• SCONCE: A cosmic web finder for spherical and conic geometries
• Enhanced spectrum of primordial perturbations, galaxy formation and small scale structure
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• Numerical convergence of pre-initial conditions on dark matter halo properties
• A Primer on Dark Matter
• Can the periodic spectral modulations of the 236 SETI candidate Sloan Survey stars be due to Dark Matter effects?
• Probing modified Newtonian dynamics with hypervelocity stars
• Made-To-Measure Models of Self-Similar Triaxial Halos with Steep Inner Density Gradients
• Dwarf Galaxies as Cosmological Probes
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• Hollow cores in Warm Dark Matter halos from the Vlasov-Poisson equation
• Novel modulus stabilization mechanism in higher dimensional f(R) Gravity
• Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
• Influence of dark matter on the structure of strange quark stars in one-fluid model
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Globular clusters vs dark matter haloes in strong lensing observations
• The influence of baryons on low-mass haloes
• A forward-modelling method to infer the dark matter particle mass from strong gravitational lenses
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• Ether and Relativity
• Explaining Dark Matter and Neutrino Mass in the light of TYPE-II Seesaw Model
• Unified dark matter: constraints from galaxies and clusters
• Solving the puzzle of subhalo spins
• Uniqueness of dark matter magnetized static black hole spacetime
• The nature of the Eastern Extent in the outer halo of M31
• Halo heating from fluctuating gas in a model dwarf
• Caught in the cosmic web: environmental effects on subhalo abundance and internal density profiles
• A dense dark matter core of the subhalo in the strong lensing system JVAS B1938+666
• Properties of subhalos in the interacting dark matter scenario
• From particles to orbits: precise dark matter density profiles using dynamical information
• The Dark Matter Contribution to Galactic Diffuse Gamma Ray Emission
• Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
• Search for dark matter in compact hydrogen clouds
• Charge transport in chiral solids as a possible tool in search of dark matter signals
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Partitioning the Galactic Halo with Gaussian Mixture Models
• Minimal parameterizations for modified gravity
• HIKER: a halo-finding method based on kernel-shift algorithm
• Milky Way globular cluster dynamics: are they preferentially co-rotating?
• A Model For Intergalactic Filaments and Galaxy Formation During the First Gigayear
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Timing Mass of the Local Group
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Impact of baryons on the population of Galactic subhalos and implications for dark matter searches
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• The impact of cosmic filaments on the abundance of satellite galaxies
• Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Thermodynamics of self-gravitating fermions as a robust theory for dark matter halos: Stability analysis applied to the Milky Way
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Assembly History and Internal Structure of Cluster Cold Dark Matter Haloes
• Merging Galaxy Clusters and the Search for New Physics of Dark Matter: A Review
• Two fluid CFL strange quark stars with scalar dark matter: critical mass and mass gap implications
• RR Lyrae stars in the newly discovered ultra-faint dwarf galaxy Centaurus I
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• Non-halo structures and their effects on gravitationally lensed galaxies
• Void probability function in the Quijote simulations
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Properties of the Lower Segment of M31's North West Stream
• Overview of the ESCAPE Dark Matter Test Science Project for Astronomers