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

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arxiv 1903.03263 v1 pith:TBKXVXQY submitted 2019-03-08 astro-ph.CO astro-ph.GAhep-ph

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

Neelima Sehgal , Ho Nam Nguyen , Joel Meyers , Moritz Munchmeyer , Tony Mroczkowski , Luca Di Mascolo , Eric Baxter , Francis-Yan Cyr-Racine
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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 An\v{z}e Slosar Eric R. Switzer Hy Trac Weishuang Xu Matias Zaldarriaga Michael Zemcov
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classification astro-ph.CO astro-ph.GAhep-ph
keywords surveydarkmattermillimeter-waveparticleyieldadvancesallow
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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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Cited by 2 Pith papers

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    Self-interaction bounds from cosmology constrain ultralight dark matter couplings to neutrinos, electrons, and light quarks via unavoidable quantum loop corrections.

  2. The Atacama Large Aperture Submillimeter Telescope (AtLAST)

    astro-ph.IM 2019-07 unverdicted novelty 4.0

    Proposes the AtLAST 50m submm telescope concept with 1-degree field of view and advanced instruments to achieve transformative wide-field mapping of the sub-mm sky.