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; 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

doi:10.48550/arXiv.1903.03263

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, Mathew Madhavacheril, Benjamin Beringue, Gil Holder, Daisuke Nagai, Simon Dicker, Cora Dvorkin, Simone Ferraro, George M. Fuller, Vera Gluscevic, Dongwon Han, Bhuvnesh Jain, Bradley JohnsonPamela 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

Research output: Working paper › Preprint › Academic

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.

Original language	English
DOIs	https://doi.org/10.48550/arXiv.1903.03263
Publication status	Submitted - 8-Mar-2019
Externally published	Yes

Keywords

astro-ph.CO
astro-ph.GA
hep-ph

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Sehgal, N., Nguyen, H. N., Meyers, J., Munchmeyer, M., Mroczkowski, T., Mascolo, L. D., Baxter, E., Cyr-Racine, F.-Y., Madhavacheril, M., Beringue, B., Holder, G., Nagai, D., Dicker, S., Dvorkin, C., Ferraro, S., Fuller, G. M., Gluscevic, V., Han, D., Jain, B., ... Zemcov, M. (2019). Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey. https://doi.org/10.48550/arXiv.1903.03263

@techreport{e8f24d4ced344e968f831dbe052360d3,

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

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. ",

keywords = "astro-ph.CO, astro-ph.GA, hep-ph",

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

note = "5 pages + references; Submitted to the Astro2020 call for science white papers",

year = "2019",

month = mar,

day = "8",

doi = "10.48550/arXiv.1903.03263",

language = "English",

type = "WorkingPaper",

}

Sehgal, N, Nguyen, HN, Meyers, J, Munchmeyer, M, Mroczkowski, T, Mascolo, LD, Baxter, E, Cyr-Racine, F-Y, Madhavacheril, M, Beringue, B, Holder, G, Nagai, D, Dicker, S, Dvorkin, C, Ferraro, S, Fuller, GM, Gluscevic, V, Han, D, Jain, B, Johnson, B, Klaassen, P, Meerburg, D, Motloch, P, Spergel, DN, Engelen, AV, Adshead, P, Armstrong, R, Baccigalupi, C, Barron, D, Basu, K, Benson, B, Beutler, F, Bond, JR, Borrill, J, Calabrese, E, Darwish, O, Denny, SL, Douglass, KA, Essinger-Hileman, T, Foreman, S, Frayer, D, Gerbino, M, Gontcho, SGA, Grohs, EB, Gupta, N, Hill, JC, Hirata, CM, Hotinli, S, Johnson, MC, Kamionkowski, M, Kovetz, ED, Lau, ET, Liguori, M, Namikawa, T, Newburgh, L, Partridge, B, Piacentni, F, Rose, B, Rossi, G, Saliwanchik, B, Schaan, E, Shan, H, Simon, S, Slosar, A, Switzer, ER, Trac, H, Xu, W, Zaldarriaga, M & Zemcov, M 2019 'Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey'. https://doi.org/10.48550/arXiv.1903.03263

TY - UNPB

T1 - Science from an Ultra-Deep, High-Resolution Millimeter-Wave Survey

AU - Sehgal, Neelima

AU - Nguyen, Ho Nam

AU - Meyers, Joel

AU - Munchmeyer, Moritz

AU - Mroczkowski, Tony

AU - Mascolo, Luca Di

AU - Baxter, Eric

AU - Cyr-Racine, Francis-Yan

AU - Madhavacheril, Mathew

AU - Beringue, Benjamin

AU - Holder, Gil

AU - Nagai, Daisuke

AU - Dicker, Simon

AU - Dvorkin, Cora

AU - Ferraro, Simone

AU - Fuller, George M.

AU - Gluscevic, Vera

AU - Han, Dongwon

AU - Jain, Bhuvnesh

AU - Johnson, Bradley

AU - Klaassen, Pamela

AU - Meerburg, Daan

AU - Motloch, Pavel

AU - Spergel, David N.

AU - Engelen, Alexander van

AU - Adshead, Peter

AU - Armstrong, Robert

AU - Baccigalupi, Carlo

AU - Barron, Darcy

AU - Basu, Kaustuv

AU - Benson, Bradford

AU - Beutler, Florian

AU - Bond, J. Richard

AU - Borrill, Julian

AU - Calabrese, Erminia

AU - Darwish, Omar

AU - Denny, S. Lucas

AU - Douglass, Kelly A.

AU - Essinger-Hileman, Tom

AU - Foreman, Simon

AU - Frayer, David

AU - Gerbino, Martina

AU - Gontcho, Satya Gontcho A

AU - Grohs, Evan B.

AU - Gupta, Nikhel

AU - Hill, J. Colin

AU - Hirata, Christopher M.

AU - Hotinli, Selim

AU - Johnson, Matthew C.

AU - Kamionkowski, Marc

AU - Kovetz, Ely D.

AU - Lau, Erwin T.

AU - Liguori, Michele

AU - Namikawa, Toshiya

AU - Newburgh, Laura

AU - Partridge, Bruce

AU - Piacentni, Francesco

AU - Rose, Benjamin

AU - Rossi, Graziano

AU - Saliwanchik, Benjamin

AU - Schaan, Emmanuel

AU - Shan, Huanyuan

AU - Simon, Sara

AU - Slosar, Anže

AU - Switzer, Eric R.

AU - Trac, Hy

AU - Xu, Weishuang

AU - Zaldarriaga, Matias

AU - Zemcov, Michael

N1 - 5 pages + references; Submitted to the Astro2020 call for science white papers

PY - 2019/3/8

Y1 - 2019/3/8

N2 - 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.

AB - 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.

KW - astro-ph.CO

KW - astro-ph.GA

KW - hep-ph

U2 - 10.48550/arXiv.1903.03263

DO - 10.48550/arXiv.1903.03263

M3 - Preprint

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

ER -

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

Abstract

Keywords

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