Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey

Cosmology and Nongalactic Astrophysics (astro-ph.CO) astro-ph.GA FOS: Physical sciences hep-ph Astrophysics - Astrophysics of Galaxies 01 natural sciences High Energy Physics - Phenomenology High Energy Physics - Phenomenology (hep-ph) 13. Climate action Astrophysics of Galaxies (astro-ph.GA) 0103 physical sciences astro-ph.CO Astrophysics - Cosmology and Nongalactic Astrophysics
DOI: 10.48550/arxiv.1903.03263 Publication Date: 2019-01-01
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.<br/>5 pages + references; Submitted to the Astro2020 call for science white papers<br/>
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