The Milky Way, Coming into Focus: Precision Astrometry Probes its Evolution, and its Dark Matter
arXiv:2106.13284 · doi:10.1016/j.ppnp.2021.103904
Abstract
The growing trove of precision astrometric observations from the Gaia space telescope and other surveys is revealing the structure and dynamics of the Milky Way in ever more exquisite detail. We summarize the current status of our understanding of the structure and the characteristics of the Milky Way, and we review the emerging picture: the Milky Way is evolving through interactions with the massive satellite galaxies that stud its volume, with evidence pointing to a cataclysmic past. It is also woven with stellar streams, and observations of streams, satellites, and field stars offer new constraints on its dark matter, both on its spatial distribution and its fundamental nature. The recent years have brought much focus to the study of dwarf galaxies found within our Galaxy's halo and their internal matter distributions. In this review, we focus on the predictions of the cold dark matter paradigm at small mass scales through precision astrometric measurements, and we summarize the modern consensus on the extent to which small-scale probes are consistent with this paradigm. We note the discovery prospects of these studies, and also how they intertwine with probes of the dynamics and evolution of the Milky Way in various and distinct ways.
87 pages, LaTeX, 25 figures; to be published by: Progress in Particle and Nuclear Physics, in 2021; references, corrections added in proof
References in corpus (73)
- The Gaia mission
- Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties
- Ultralight scalars as cosmological dark matter
- Dark Matter Candidates from Particle Physics and Methods of Detection
- Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds
- The Milky Way's Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars
- The Effective Field Theory of Cosmological Large Scale Structures
- Are the Magellanic Clouds on their First Passage about the Milky Way?
- Massloss of galaxies due to a UV-background
- Beasts of the Southern Wild: Discovery of nine Ultra Faint satellites in the vicinity of the Magellanic Clouds
- Evidence for Two Early Accretion Events That Built the Milky Way Stellar Halo
- The Local Dark Matter Density
- The accretion origin of the Milky Way's stellar halo
- Hundreds of Milky Way Satellites? Luminosity Bias in the Satellite Luminosity Function
- Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
- Disruption of Dark Matter Substructure: Fact or Fiction?
- Non-relativistic effective theory of dark matter direct detection
- Dark Matter Substructure in Numerical Simulations: A Tale of Discreteness Noise, Runaway Instabilities, and Artificial Disruption
- Single-electron and single-photon sensitivity with a silicon Skipper CCD
- Cluster Lenses
- "Skinny Milky Way, Please", says Sagittarius
- Rings and Radial Waves in the Disk of the Milky Way
- A Compendium of Distances to Molecular Clouds in the Star Formation Handbook
- The Vertical Structure of the Outer Milky Way HI Disk
- A critical look at cosmological perturbation theory techniques
- Phase-space structure in the local dark matter distribution and its signature in direct detection experiments
- A First Constraint on the Thick Disk Scale Length: Differential Radial Abundances in K Giants at Galactocentric Radii 4, 8, and 12 kpc
- Detection of sub-MeV Dark Matter with Three-Dimensional Dirac Materials
- Bent by baryons: the low mass galaxy-halo relation
- Globular Cluster Streams as Galactic High-Precision Scales - The Poster Child Palomar 5
- Improved GRAVITY astrometric accuracy from modeling of optical aberrations
- Dark matter in the Milky Way, II. the HI gas distribution as a tracer of the gravitational potential
- The shape of the inner Milky Way halo from observations of the Pal 5 and GD-1 stellar streams
- An excess of small-scale gravitational lenses observed in galaxy clusters
- The end of the MACHO era- revisited: new limits on MACHO masses from halo wide binaries
- Making dark matter out of light: freeze-in from plasma effects
- The Fall of a Giant. Chemical evolution of Enceladus, alias the Gaia Sausage
- Diamond Detectors for Direct Detection of Sub-GeV Dark Matter
- An intuitive 3D map of the Galactic warp's precession traced by classical Cepheids
- Orbits of Massive Satellite Galaxies: I. A Close Look at the Large Magellanic Cloud and a New Orbital History for M33
- Shaken and Stirred: The Milky Way's Dark Substructures
- M31 Transverse Velocity and Local Group Mass from Satellite Kinematics
- All-Sky Dynamical Response of the Galactic Halo to the Large Magellanic Cloud
- A Magellanic Origin for the Warp of the Galaxy
- Galactic Warps Induced By Cosmic Infall
- Pulsar Timing Probes of Primordial Black Holes and Subhalos
- Halo-to-Halo Similarity and Scatter in the Velocity Distribution of Dark Matter
- Too Many, Too Few, or Just Right? The Predicted Number and Distribution of Milky Way Dwarf Galaxies
- Extended stellar systems in the solar neighborhood - II. Discovery of a nearby 120° stellar stream in Gaia DR2
- Gaps in globular cluster streams: giant molecular clouds can cause them too
- Milky Way Mass and Potential Recovery Using Tidal Streams in a Realistic Halo
- Dipping Our Toes in the Water: First Models of GD-1 as a Stream
- Nuclear Structure of Bound States of Asymmetric Dark Matter
- The tidal evolution of dark matter substructure -- I. Subhalo density profiles
- The dynamics of tidal tails from massive satellites
- Action-space clustering of tidal streams to infer the Galactic potential
- Strategies for Determining the Nature of Dark Matter
- The coherent motion of Cen A dwarf satellite galaxies remains a challenge for CDM cosmology
- Inferring the gravitational potential of the Milky Way with a few precisely measured stars
- Dark Matter Direct Search Rates in Simulations of the Milky Way and Sagittarius Stream
- Draco, a flawless dwarf galaxy
- Galactoseismology and the Local Density of Dark Matter
- Probing the Local Velocity Distribution of WIMP Dark Matter with Directional Detectors
- Dependence of Dark Matter - Electron Scattering on the Galactic Dark Matter Velocity Distribution
- Cooling in a Dissipative Dark Sector
- Milky Way Tomography with K and M Dwarf Stars: the Vertical Structure of the Galactic Disk
- Dynamical model of the Milky Way using APOGEE and Gaia data
- Phase-space correlation in stellar streams of the Milky Way halo: The clash of Kshir and GD-1
- Primordial Black Holes as Dark Matter: Constraints From Compact Ultra-Faint Dwarfs
- Reconstructing the three-dimensional local dark matter velocity distribution
- Observing Dark Matter via the Gyromagnetic Faraday Effect
- Asymmetric Mean Metallicity Distribution of the Milky Way's Disk
- Axial Asymmetry Studies in Gaia Data Release 2 Yield the Pattern Speed of the Galactic Bar
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- The Return of the Templates: Revisiting the Galactic Center Excess with Multi-Messenger Observations
- Neutron Stars with Baryon Number Violation, Probing Dark Sectors
- Forecasts for Galaxy Formation and Dark Matter Constraints from Dwarf Galaxy Surveys
- Milky Way-est: Cosmological Zoom-in Simulations with Large Magellanic Cloud and Gaia-Sausage-Enceladus Analogs
- Astrometric Gravitational-Wave Detection via Stellar Interferometry
- Directional Detection of Dark Matter Using Solid-State Quantum Sensing
- Probing Dark Sectors with Neutron Stars
- Two-point correlation function studies for the Milky Way: discovery of spatial clustering from disk excitations and substructure
- A Wave-Corrected Assessment of the Local Midplane
- Using two point correlation functions to understand the assembly histories of Milky Way-like galaxies
- Newtonian Gravity and Galaxy Rotation Curves: An Axisymmetric Green's Function Perspective