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 (25)

• The hierarchical formation of the brightest cluster galaxies
• Too big to fail? The puzzling darkness of massive Milky Way subhaloes
• Cats and Dogs, Hair and A Hero: A Quintet of New Milky Way Companions
• The redshift dependence of the structure of massive LCDM 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
• Stellar Feedback in Dwarf Galaxy Formation
• Assembly bias in the clustering of dark matter haloes
• The halo mass function from the dark ages through the present day
• 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
• Halo assembly bias and its effects on galaxy clustering
• Cosmological puzzle resolved by stellar feedback in high redshift galaxies
• A blueprint for detecting supersymmetric dark matter in the Galactic halo
• Galaxy growth in the concordance $\Lambda$CDM cosmology
• Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
• 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
• 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
• The Dark Matter Annihilation Signal from Galactic Substructure: Predictions for GLAST
• The fine-grained phase-space structure of Cold Dark Matter halos
• The origin of failed subhaloes and the common mass scale of the Milky Way satellite galaxies
• Dark Matter Caustics
• 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 (138)

• Large-scale dark matter simulations
• 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 Cosmic Ballet II: Spin alignment of galaxies and haloes with large-scale filaments in the EAGLE simulation
• Faint dwarfs as a test of DM models: WDM vs. CDM
• The Three Hundred Project: Backsplash galaxies in simulations of clusters
• The phase space density of fermionic dark matter haloes
• The failures of the standard model of cosmology require a new paradigm
• 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
• New Roads to the Small-Scale Universe: Measurements of the Clustering of Matter with the High-Redshift UV Galaxy Luminosity Function
• Caught in the cosmic web: Environmental effect on halo concentrations, shape, and spin
• The Search for Dark Matter
• The halo mass function and filaments in full cosmological simulations with fuzzy dark matter
• Building a Predictive Model of Galaxy Formation - I: Phenomenological Model Constrained to the $z=0$ Stellar Mass Function
• SIBELIUS-DARK: a galaxy catalogue of the Local Volume from a constrained realisation simulation
• Subhaloes gone Notts: Spin across subhaloes and finders
• Deadly dark matter cusps vs faint and extended star clusters: Eridanus II and Andromeda XXV
• The tangential velocity excess of the Milky Way satellites
• The phase-space structure of tidally stripped halos
• 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
• 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
• Hadronic and hadron-like physics of Dark Matter
• Tidal Stripping in the Adiabatic Limit
• Coherent and incoherent structures in fuzzy dark matter halos
• Probing massless and massive gravitons via entanglement in a warped extra dimension
• Testing strong lensing subhalo detection with a cosmological simulation
• Selection of massive evolved galaxies at $3\le z\le 4.5$ in the CANDELS fields
• Flattened structures of dwarf satellites around massive host galaxies in the MATLAS low-to-moderate density fields
• Testing the Prediction of Fuzzy Dark Matter Theory in the Milky Way Center
• The Three Hundred Project: Substructure in hydrodynamical and dark matter simulations of galaxy groups around clusters
• Search for Bosonic Super-WIMP Interactions with the XENON100 Experiment
• Cosmological tests of modified gravity: constraints on $F(R)$ theories from the galaxy clustering ratio
• Radial velocities and stellar population properties of 56 MATLAS dwarf galaxies observed with MUSE
• Baryonic effects on the detectability of annihilation radiation from dark matter subhaloes around the Milky Way
• The Three Hundred project: galaxy cluster mergers and their impact on the stellar component of brightest cluster galaxies
• The stellar halo in Local Group Hestia simulations III. Chemical abundance relations for accreted and in-situ stars
• Testing the Relationship Between Bursty Star Formation and Size Fluctuations of Local Dwarf Galaxies
• Constraining interacting dark energy models with the halo concentration-mass relation
• Emergent gravity in galaxies and in the Solar System
• A dynamical system representation of generalized Rastall gravity
• Modelling the accretion and feedback of supermassive black hole binaries in gas-rich galaxy mergers
• The Three Hundred project: Galaxy groups do not survive cluster infall
• Hydrodynamical structure formation in Milgromian cosmology
• Multi-Epoch Machine Learning 1: Unravelling Nature vs Nurture for Galaxy Formation
• Gravitational collapse in the Schrödinger-Poisson system
• Ejection of supermassive black holes and implications for merger rates in fuzzy dark matter haloes
• Evolution of subhalo orbits in a smoothly-growing host halo potential
• 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
• 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
• Micro galaxies in LCDM
• 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
• Star forming filaments in warm dark matter models
• Properties and observables of massive galaxies in self-interacting dark matter cosmologies
• Culminating the peak CUSP to descry the dark side of halos
• Cosmological Probes for Supersymmetry
• Mitigating Foreground Bias to the CMB Lensing Power Spectrum for a CMB-HD Survey
• Dark Matter in Fractional Gravity I: Astrophysical Tests on Galactic Scales
• Robust Clustering of the Local Milky Way Stellar Kinematic Substructures with Gaia eDR3
• Shan--Chen interacting vacuum cosmology
• Tracking the orbit of unresolved subhalos for semi-analytic models
• Universal scaling laws and density slope for dark matter haloes
• 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
• Fingerprints of Anomalous Primordial Universe on the Abundance of Large Scale Structures
• Connecting the Cosmic Star Formation Rate with the Local Star Formation
• The interacting vacuum and tensions: a comparison of theoretical models
• RABBITS -- II. The impact of AGN feedback on coalescing supermassive black holes in disc and elliptical galaxy mergers
• Dark matter halo mass functions and density profiles from mass and energy cascade
• The Subaru HSC weak lensing mass-observable scaling relations of spectroscopic galaxy groups from the GAMA survey
• Determining Satellite Infall Times Using Machine Learning
• Hα Dots: Direct-Method Metal Abundances of Low-Luminosity Star-Forming Systems
• Velocity-dependent annihilation radiation from dark matter subhalos in cosmological simulations
• Hidden from view: Coupled Dark Sector Physics and Small Scales
• Maximum entropy distributions of dark matter in $\Lambda$CDM cosmology
• How do baryonic effects on the cosmic matter distribution vary with scale and local density environment?
• Assessing Mass Loss and Stellar-to-Halo Mass Ratio of Satellite Galaxies: A Galaxy-Galaxy Lensing Approach Utilizing DECaLS DR8 Data
• The proper motion of stars in dwarf galaxies: distinguishing central density cusps from cores
• Correlations of Dark Matter, Gas and Stellar Profiles in Dark Matter Halos
• Discovery of a Rare Group of Dwarf Galaxies in the Local Universe
• Probing modified Newtonian dynamics with hypervelocity stars
• A Primer on Dark Matter
• Numerical convergence of pre-initial conditions on dark matter halo properties
• SCONCE: A cosmic web finder for spherical and conic geometries
• The feasibility of constraining DM interactions with high-redshift observations by JWST
• MultiCAM: A multivariable framework for connecting the mass accretion history of haloes with their properties
• The Galaxy Halo Connection in Modified Gravity Cosmologies: Environment Dependence of Galaxy Luminosity function
• Made-To-Measure Models of Self-Similar Triaxial Halos with Steep Inner Density Gradients
• Galaxy pairs in The Three Hundred simulations: a study on the performance of observational pair-finding techniques
• Influence of dark matter on the structure of strange quark stars in one-fluid model
• Search for Dark Matter Annihilation to gamma-rays from SPT-SZ selected Galaxy Clusters
• Novel modulus stabilization mechanism in higher dimensional f(R) Gravity
• Galaxy pairs in The Three Hundred simulations II: studying bound ones and identifying them via machine learning
• Hollow cores in Warm Dark Matter halos from the Vlasov-Poisson equation
• Baryon effects on the dark matter halos constrained from strong gravitational lensing
• The influence of baryons on low-mass haloes
• Solving the puzzle of subhalo spins
• Uniqueness of dark matter magnetized static black hole spacetime
• The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
• 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
• From particles to orbits: precise dark matter density profiles using dynamical information
• Halo heating from fluctuating gas in a model dwarf
• The nature of the Eastern Extent in the outer halo of M31
• What is the right way to quench star formation in semi-analytic model of galaxy formation?
• Galaxies OBserved as Low-luminosity Identified Nebulae (GOBLIN): a catalog of 43,000 high-probability dwarf galaxy candidates in the UNIONS survey
• Charge transport in chiral solids as a possible tool in search of dark matter signals
• The Formation of M101-alike Galaxies in the Cold Dark Matter Model
• Halo concentration strengthens dark matter constraints in galaxy-galaxy strong lensing analyses
• Simulating gravitational motion, gas dynamics, and structure in the cosmos
• Comparison of HMG and flat rotation velocities inferred from galaxy-galaxy weak lensing
• CWTHF: Identifying Dark Matter Halos with Continuous Wavelet Transform
• Measuring the Stellar-to-Halo Mass Relation at $\sim 10^{10}$ Solar masses, using forthcoming space-based imaging of galaxy-galaxy strong lenses
• Galaxy-galaxy strong lens perturbations: line-of-sight haloes versus lens subhaloes
• Thermodynamics of self-gravitating fermions as a robust theory for dark matter halos: Stability analysis applied to the Milky Way
• Abundance and phase-space distribution of subhalos in cosmological N-body simulations: testing numerical convergence and correction methods
• The impact of cosmic filaments on the abundance of satellite galaxies
• Investigation of mass substructure in gravitational lens system SDP.81 with ALMA long-baseline observations
• Impact of baryons on the population of Galactic subhalos and implications for dark matter searches
• Timing Mass of the Local Group
• On a critical acceleration scale of dark matter in Lambda-CDM and dynamical dark energy
• Properties of the Lower Segment of M31's North West Stream
• The effects of self-interacting dark matter on the stripping of galaxies that fall into clusters
• Correlation between Outlying Halo Abundance and Host Halo Properties
• Prediction of Individual Halo Concentrations Across Cosmic Time Using Neural Networks
• Overview of the ESCAPE Dark Matter Test Science Project for Astronomers
• Non-halo structures and their effects on gravitationally lensed galaxies
• 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
• Void probability function in the Quijote simulations
• 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