The large-scale structure of the Universe
arXiv:astro-ph/0604561 · doi:10.1038/nature04805
Abstract
Research over the past 25 years has led to the view that the rich tapestry of present-day cosmic structure arose during the first instants of creation, where weak ripples were imposed on the otherwise uniform and rapidly expanding primordial soup. Over 14 billion years of evolution, these ripples have been amplified to enormous proportions by gravitational forces, producing ever-growing concentrations of dark matter in which ordinary gases cool, condense and fragment to make galaxies. This process can be faithfully mimicked in large computer simulations, and tested by a variety of observations that probe the history of the Universe starting from just 400,000 yr after the Big Bang.
Invited review to Nature (27 April 2006 issue), Early Universe Supplement, 34 pages, 6 figures (partially size reduced)
References in corpus (2)
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- Evolution of matter and galaxy clustering in cosmological hydrodynamical simulations
- Continuous Filament Network of the Local Universe
- STRRINGS: STReams in Residual Images of Nearby GalaxieS
- Growth rate of matter perturbations as a probe of large-scale magnetism
- Combined dark matter search towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS
- The Schrdinger-Poisson equations as the large-N limit of the Newtonian N-body system: applications to the large scale dark matter dynamics
- Dark Matter Substructure or Source Model Systematics? A Case Study of Cluster Lens Abell S1063
- HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
- The KALEIDOSCOPE survey : A new strong and weak gravitational lensing view of the massive galaxy cluster MACS J1423.8+2404
- The bias from hydrodynamic simulations: mapping baryon physics onto dark matter fields
- The viability of low-mass subhaloes as targets for gamma-ray dark matter searches
- Relating the HI Gas Structure of Spiral Disks to Passing Satellites
- Identifying clustering at high redshift through actively star-forming galaxies
- Dark Coincidences: Small-Scale Solutions with Refracted Gravity and MOND
- Self-interacting Dark Matter with Scalar Dilepton Mediator
- Gibbs Point Process Model for Young Star Clusters in M33
- Bayesian analysis of cosmic structures
- On the accuracy of the high redshift cluster luminosity function
- Numerical Simulations of the Dark Universe: State of the Art and the Next Decade
- Dissecting Cosmological Filaments at High Redshifts: Emergence of Spaghetti-type Flow Inside DM Haloes
- Power-law solutions for TeVeS
- Scatter in the star formation rate-halo mass relation: secondary bias and its impact on line-intensity mapping
- GalaxyGenius: Mock galaxy image generator for various telescopes from hydrodynamical simulations
- Gravitational Lensing of Dark Energy Models and CDM Using Observational data in Loop Quantum Cosmology
- Dynamics of Coulombic and Gravitational Periodic Systems
- DARKSKIES: A suite of super-sampled zoom-in simulations of galaxy clusters with self-interacting dark matter
- MUSE observations of the blue compact dwarf galaxy Haro 14. Data analysis and first results on morphology and stellar populations
- The nature of the Eastern Extent in the outer halo of M31
- ALMA detects molecular gas in the halo of the powerful radio galaxy TXS 0828+193
- Application of Physics-Informed Neural Networks in Removing Telescope Beam Effects
- On the cosmological viability of the Hu-Sawicki type modified induced gravity
- Revisiting Puffy Dark Matter with Novel Insights: Partial Wave Analysis
- Thermal evolution of dark matter and gravitational-wave production in the early universe from a symplectic glueball model
- Distinguishing thermal histories of dark matter from structure formation
- Metamorphosis of dwarf halo density profile under dark matter decays
- Statistics of the Planck CMB signal in direction of gamma-ray bursts from the BATSE and BeppoSAX catalogs
- Luminosity Bias (II): The Cosmic Web of the First Stars
- Dark Matter searches in Dwarf Galaxies with the Southern Wide-field Gamma-ray Observatory
- Disentanglement of the chemodynamical assembly: mapping the Milky Way disks
- Pearls on a string: Dark and bright galaxies on a strikingly straight and narrow filament
- Symmetry and Conserved Quantities in -Gravity: Mei vs. Noether Approaches
- Gamma Rays from Annihilations at the Galactic Center in a Physical Dark Matter Distribution
- Euclid preparation: TBD. Cosmic Dawn Survey: evolution of the galaxy stellar mass function across 0.2<z<6.5 measured over 10 square degrees
- Asymmetry at Low Surface Brightness as an Indicator of Environmental Processes in the Fornax Cluster
- The relation of galaxies and dark matter haloes to the filamentary cosmic web
- Stability of HDE model with sign-changeable interaction in Brans-Dicke theory
- Plasma processes at the scales of galaxies and clusters of galaxies
- Under an Iron Sky: On the Entropy at the Start of the Universe
- Structure Formation independent of Cold Dark Matter
- Revisiting Agegraphic Dark Energy in Brans-Dicke Cosmology
- The Evolution of the Hubble Sequence: morpho-kinematics of distant galaxies
- Impact of the large-scale cosmic web on the X-ray emitting circumgalactic medium
- A Hydro-Particle-Mesh Code for Efficient and Rapid Simulations of the Intracluster Medium
- Combined LOFAR-uGMRT analysis of the diffuse radio emission in the massive clusters Abell 773 and Abell 1351
- Estimating the mass of galactic components using machine learning algorithms
- Refracted Gravity Solutions from Small to Large Scales
- Using Strong Lensing to Detect Subhalos with Steep Inner Density Profiles
- Unequal-mass mergers of dark matter haloes with rare and frequent self-interactions
- Excess of diffuse gamma-ray emission detected from the galaxy cluster Abell 119 from 14-year Fermi-LAT Data
- The Extended Zel'dovich Mass Functions of Clusters and Isolated Clusters in the Presence of Primordial Non-Gaussianity
- Properties of the Lower Segment of M31's North West Stream
- Formation of Population III Stars in a flat FLRW Universe
- Stellar populations -- the next ten years
- Structure-wide dark matter density depletion induced by local degeneracies
- Probing Dark Matter with Strong Gravitational Lensing through an Effective Density Slope
- A LOFAR-uGMRT spectral index study of distant radio halos
- Quintessence reconstruction of interacting HDE in a non-flat universe
- Some properties of doubly-degenerate stars
- Fenomenología de modelos supersimétricos: partículas y materia oscura
- CDM, DGP and extended phantom-like cosmologies
- Spikes in the SED and Ripples in the Outskirts of Galaxies
- Structure Formation with Dark Magnetohydrodynamics
- Explosions in the Empty: A Survey of Transients in Local Void Galaxies
- Signatures of Extended Dark Energy Parametrisations in Structure Formation under Background Constraints
- Multiverse effects on the CMB angular correlation function in the framework of NCG
- A group of merging galaxies falling onto Abell 2142
- Tidal adaptive softening and artificial fragmentation in cosmological simulations
- Clumpy Starburst in a Local Dwarf Galaxy, NGC 1522
- Fast Baryonic Field Painting for Sunyaev-Zel'dovich Analyses: Transfer Function vs. Hybrid Effective Field Theory
- Mode and Ridge Estimation in Euclidean and Directional Product Spaces: A Mean Shift Approach
- Non-halo structures and their effects on gravitationally lensed galaxies
- Dark Energy Survey Year 3 results: Cosmology with peaks using an emulator approach
- The intergalactic medium in the cosmic web
- Revisiting the two-body problem in Yukawa gravity and in a gravitational extension of the Buckingham potential
- A new mechanism for dark matter generation from an interacting cosmological constant
- Mesoscopic Energy Ranking Constraints in the IllustrisTNG Simulations
- rrlfe: Software for Generating and Applying Metallicity Calibrations for RR Lyrae Variable Stars Across a Wide Range of Phases and Temperatures