Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey
Authors: Neelima Sehgal, Ho Nam Nguyen, Joel Meyers, Moritz Munchmeyer, Tony Mroczkowski, Luca Di Mascolo, Eric Baxter, Francis-Yan Cyr-Racine, Mathew Madhavacheril, Benjamin Beringue, Gil Holder, Daisuke Nagai, Simon Dicker, Cora Dvorkin, Simone Ferraro, George M. Fuller, Vera Gluscevic, Dongwon Han, Bhuvnesh Jain, Bradley Johnson, Pamela Klaassen, Daan Meerburg, Pavel Motloch, David N. Spergel, Alexander van Engelen, Peter Adshead, Robert Armstrong, Carlo Baccigalupi, Darcy Barron, Kaustuv Basu, Bradford Benson, Florian Beutler, J. Richard Bond, Julian Borrill, Erminia Calabrese, Omar Darwish, S. Lucas Denny, Kelly A. Douglass, Tom Essinger-Hileman, Simon Foreman, David Frayer, Martina Gerbino, Satya Gontcho A Gontcho, Evan B. Grohs, Nikhel Gupta, J. Colin Hill, Christopher M. Hirata, Selim Hotinli, Matthew C. Johnson, Marc Kamionkowski, Ely D. Kovetz, Erwin T. Lau, Michele Liguori, Toshiya Namikawa, Laura Newburgh, Bruce Partridge, Francesco Piacentni, Benjamin Rose, Graziano Rossi, Benjamin Saliwanchik, Emmanuel Schaan, Huanyuan Shan, Sara Simon, Anže Slosar, Eric R. Switzer, Hy Trac, Weishuang Xu, Matias Zaldarriaga, Michael Zemcov
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.
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