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CMB-HD: An Ultra-Deep, High-Resolution Millimeter-Wave Survey Over Half the Sky

Authors :
Sehgal, Neelima
Aiola, Simone
Akrami, Yashar
Basu, Kaustuv
Boylan-Kolchin, Michael
Bryan, Sean
Clesse, Sebastien
Cyr-Racine, Francis-Yan
Di Mascolo, Luca
Dicker, Simon
Essinger-Hileman, Thomas
Ferraro, Simone
Fuller, George M.
Han, Dongwon
Hasselfield, Mathew
Holder, Gil
Jain, Bhuvnesh
Johnson, Bradley
Johnson, Matthew
Klaassen, Pamela
Madhavacheril, Mathew
Mauskopf, Philip
Meerburg, Daan
Meyers, Joel
Mroczkowski, Tony
Munchmeyer, Moritz
Naess, Sigurd
Nagai, Daisuke
Namikawa, Toshiya
Newburgh, Laura
Nguyen, Ho Nam
Niemack, Michael
Oppenheimer, Benjamin D.
Pierpaoli, Elena
Schaan, Emmanuel
Slosar, Anze
Spergel, David
Switzer, Eric
van Engelen, Alexander
Wollack, Edward
Source :
Bulletin of the American Astronomical Society, Vol. 51, Issue 7, id. 6 (2019)
Publication Year :
2019

Abstract

A millimeter-wave survey over half the sky, that spans frequencies in the range of 30 to 350 GHz, and that is both an order of magnitude deeper and of higher-resolution than currently funded surveys would yield an enormous gain in understanding of both fundamental physics and astrophysics. By providing such a deep, high-resolution millimeter-wave survey (about 0.5 uK-arcmin noise and 15 arcsecond resolution at 150 GHz), CMB-HD will enable major advances. It will allow 1) the use of gravitational lensing of the primordial microwave background to map the distribution of matter on small scales (k~10/hMpc), which probes dark matter particle properties. It will also allow 2) measurements of the thermal and kinetic Sunyaev-Zel'dovich effects on small scales to map the gas density and gas pressure profiles of halos over a wide field, which probes galaxy evolution and cluster astrophysics. In addition, CMB-HD would allow us to cross critical thresholds in fundamental physics: 3) ruling out or detecting any new, light (< 0.1eV), thermal particles, which could potentially be the dark matter, and 4) testing a wide class of multi-field models that could explain an epoch of inflation in the early Universe. Such a survey would also 5) monitor the transient sky by mapping the full observing region every few days, which opens a new window on gamma-ray bursts, novae, fast radio bursts, and variable active galactic nuclei. Moreover, CMB-HD would 6) provide a census of planets, dwarf planets, and asteroids in the outer Solar System, and 7) enable the detection of exo-Oort clouds around other solar systems, shedding light on planet formation. CMB-HD will deliver this survey in 5 years of observing half the sky, using two new 30-meter-class off-axis cross-Dragone telescopes to be located at Cerro Toco in the Atacama Desert. The telescopes will field about 2.4 million detectors (600,000 pixels) in total.<br />Comment: APC White Paper for the Astro2020 Decadal, with updated proposing team

Details

Database :
arXiv
Journal :
Bulletin of the American Astronomical Society, Vol. 51, Issue 7, id. 6 (2019)
Publication Type :
Report
Accession number :
edsarx.1906.10134
Document Type :
Working Paper