Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey
arXiv:1903.03263
Abstract
Opening up a new window of millimeter-wave observations that span frequency bands in the range of 30 to 500 GHz, survey half the sky, and are both an order of magnitude deeper (about 0.5 uK-arcmin) and of higher-resolution (about 10 arcseconds) than currently funded surveys would yield an enormous gain in understanding of both fundamental physics and astrophysics. In particular, such a survey would allow for major advances in measuring the distribution of dark matter and gas on small-scales, and yield needed insight on 1.) dark matter particle properties, 2.) the evolution of gas and galaxies, 3.) new light particle species, 4.) the epoch of inflation, and 5.) the census of bodies orbiting in the outer Solar System.
arXiv comment5 pages + references; Submitted to the Astro2020 call for science white papers
References in corpus (72)
- A direct empirical proof of the existence of dark matter
- Observational evidence for self-interacting cold dark matter
- Cold and Fuzzy Dark Matter
- Ultralight scalars as cosmological dark matter
- Dark Matter Self-interactions and Small Scale Structure
- Cosmic Structure as the Quantum Interference of a Coherent Dark Wave
- Constraining Warm Dark Matter candidates including sterile neutrinos and light gravitinos with WMAP and the Lyman-alpha forest
- Warm Dark Matter as a solution to the small scale crisis: new constraints from high redshift Lyman-alpha forest data
- Direct Detection of CDM Substructure
- Subhaloes in Self-Interacting Galactic Dark Matter Haloes
- Dark Matter Halos as Particle Colliders: A Unified Solution to Small-Scale Structure Puzzles from Dwarfs to Clusters
- New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman- forest data
- The unexpected diversity of dwarf galaxy rotation curves
- Late time Cosmological Phase Transition and Galactic Halo as Bose-liquid
- The Lyman-alpha Forest in the Cold Dark Matter Model
- Substructure and halo density profiles in a Warm Dark Matter Cosmology
- Gravitational detection of a low-mass dark satellite at cosmological distance
- Fluid Dark Matter
- Repulsive Dark Matter
- CMB-S4 Science Book, First Edition
- Core Formation in Dwarf Halos with Self Interacting Dark Matter: No Fine-Tuning Necessary
- Detection of a Dark Substructure through Gravitational Imaging
- Constraining Dark Matter-Baryon Scattering with Linear Cosmology
- The Cosmology of Atomic Dark Matter
- How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves
- ETHOS - An Effective Theory of Structure Formation: Dark matter physics as a possible explanation of the small-scale CDM problems
- ETHOS - An Effective Theory of Structure Formation: From dark particle physics to the matter distribution of the Universe
- The Power Spectrum of Mass Fluctuations Measured from the Lyman-alpha Forest at Redshift z=2.5
- Lyman-alpha Forests cool Warm Dark Matter
- Inference of the Cold Dark Matter substructure mass function at z=0.2 using strong gravitational lenses
- Dark Matter from an ultra-light pseudo-Goldsone-boson
- Quantifying baryon effects on the matter power spectrum and the weak lensing shear correlation
- Probing sub-GeV Dark Matter-Baryon Scattering with Cosmological Observables
- The chosen few: the low mass halos that host faint galaxies
- A New Target for Cosmic Axion Searches
- Constraints on scattering of keV--TeV dark matter with protons in the early Universe
- A Critical Assessment of CMB Limits on Dark Matter-Baryon Scattering: New Treatment of the Relative Bulk Velocity
- Kinematics and chemistry of recently discovered Reticulum 2 and Horologium 1 dwarf galaxies
- Interacting Dark Matter disguised as Warm Dark Matter
- Evidence for the kinematic Sunyaev-Zeľdovich effect with ACTPol and velocity reconstruction from BOSS
- All about baryons: revisiting SIDM predictions at small halo masses
- Low-mass halo perturbations in strong gravitational lenses at redshift z0.5 are consistent with CDM
- Mass Accretion and its Effects on the Self-Similarity of Gas Profiles in the Outskirts of Galaxy Clusters
- Properties of Dark Subhaloes from Gaps in Tidal Streams
- Measuring the power spectrum of dark matter substructure using strong gravitational lensing
- Constraining local non-Gaussianities with kSZ tomography
- First Cosmological Constraint on the Effective Theory of Dark Matter-Proton Interactions
- Dark matter-radiation interactions: the impact on dark matter haloes
- Quantifying dwarf satellites through gravitational imaging: the case of SDSS J120602.09+514229.5
- Reconstruction of the remote dipole and quadrupole fields from the kinetic Sunyaev Zel'dovich and polarized Sunyaev Zel'dovich effects
- Effects of sub-mm and radio point sources on the recovery of Sunyaev-Zeldovich galaxy cluster parameters
- Future constraints on halo thermodynamics from combined Sunyaev-Zel'dovich measurements
- Constraints on Warm Dark Matter models from high-redshift long gamma-ray bursts
- Constraints on the small-scale power spectrum of density fluctuations from high-redshift gamma-ray bursts
- Recovery of the Shape of the Mass Power Spectrum from the Lyman-alpha Forest
- On the Power Spectrum of Dark Matter Substructure in Strong Gravitational Lenses
- Gravitational Lensing and the Power Spectrum of Dark Matter Substructure: Insights from the ETHOS N-body Simulations
- The inner mass power spectrum of galaxies using strong gravitational lensing: beyond linear approximation
- Probing the small-scale structure in strongly lensed systems via transdimensional inference
- Discovery and Physical Characterization of a Large Scattered Disk Object at 92 AU
- Beyond subhalos: Probing the collective effect of the Universe's small-scale structure with gravitational lensing
- Systematic errors in the measurement of neutrino masses due to baryonic feedback processes: Prospects for stage IV lensing surveys
- Wandering in the Lyman-alpha Forest: A Study of Dark Matter-Dark Radiation Interactions
- Measuring the Small-Scale Matter Power Spectrum with High-Resolution CMB Lensing
- Disentangling Dark Physics with Cosmic Microwave Background Experiments
- The Effects of Rayleigh Scattering on the CMB and Cosmic Structure
- Dark Matter Superfluidity
- Quantifying the power spectrum of small-scale structure in semi-analytic galaxies
- Constrained Cluster Parameters from Sunyaev-Zel'dovich Observations
- KSZ tomography and the bispectrum
- Tidal Debris as a Dark Matter Probe
- Gravitational Imaging of CDM Substructure