Axion Dark Matter

Axion Dark Matter

Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white paper summarizes axion phenomenology and outlines n...

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Veröffentlicht in:arXiv.org 2023-03
Hauptverfasser: Adams, C B, Aggarwal, N, Agrawal, A, Bartram, C, Bekker, H, Belov, P, Berggren, K K, Boutan, C, Bowring, D, Budker, D, Caldwell, A, Cervantes, R, Chakrabarty, S S, Chou, A, Co, R T, Conrad, J, Croon, D, D'Agnolo, R T, Demarteau, M, DePorzio, N, L Di Luzio, Diaz-Morcillo, A, Dona, K, Droster, A, Dunne, K, Döbrich, B, Essig, R, Foster, J W, Fry, J T, A Gallo Rosso, García Barceló, J M, Irastorza, I G, Gardner, S, Ghosh, S, Giaccone, B, Giannotti, M, Grin, D, Grote, H, Awida, M H, Hoof, S, Hoshino, G, Irsic, V, Jackson, H, Jackson Kimball, D F, Jaeckel, J, Jakovcic, K, Jewell, M J, Khatiwada, R, Knirck, S, Kovachy, T, Krueger, P, Kuenstner, S E, Kurinsky, N A, Leane, R K, Leder, A F, Lee, C, Lehnert, K W, Liu, J, Majorovits, B, Millar, A J, Miller, D W, Mitchell, J, Nagaitsev, S, Noroozian, O, Oblath, N S, Ouellet, J L, Peiris, H V, Perez, K, Phipps, A, Pivovaroff, M J, Quílez, P, Rapidis, N M, Robles, V H, Rudolph, J, Rybka, G, Safdari, M, Safdi, B R, Shu, J, Singh, J, Singh, S, Sinha, K, Sinnis, J T, Smith, M S, Snow, W M, Sokolov, A V, Sushkov, A O, Tait, T M P, Takhistov, V, Temples, D J, Thomas, J H, Tobar, M E, Vandegar, M, Vogel, J K, Wang, Z, Wickenbrock, A, Winslow, L, Wooten, M, Young, B A, F Yu, Zhou, K
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Astronomical models
Cosmology
Dark matter
Magnets
Phenomenology
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creator Adams, C B
Aggarwal, N
Agrawal, A
Bartram, C
Bekker, H
Belov, P
Berggren, K K
Boutan, C
Bowring, D
Budker, D
Caldwell, A
Cervantes, R
Chakrabarty, S S
Chou, A
Co, R T
Conrad, J
Croon, D
D'Agnolo, R T
Demarteau, M
DePorzio, N
L Di Luzio
Diaz-Morcillo, A
Dona, K
Droster, A
Dunne, K
Döbrich, B
Essig, R
Foster, J W
Fry, J T
A Gallo Rosso
García Barceló, J M
Irastorza, I G
Gardner, S
Ghosh, S
Giaccone, B
Giannotti, M
Grin, D
Grote, H
Awida, M H
Hoof, S
Hoshino, G
Irsic, V
Jackson, H
Jackson Kimball, D F
Jaeckel, J
Jakovcic, K
Jewell, M J
Khatiwada, R
Knirck, S
Kovachy, T
Krueger, P
Kuenstner, S E
Kurinsky, N A
Leane, R K
Leder, A F
Lee, C
Lehnert, K W
Liu, J
Majorovits, B
Millar, A J
Miller, D W
Mitchell, J
Nagaitsev, S
Noroozian, O
Oblath, N S
Ouellet, J L
Peiris, H V
Perez, K
Phipps, A
Pivovaroff, M J
Quílez, P
Rapidis, N M
Robles, V H
Rudolph, J
Rybka, G
Safdari, M
Safdi, B R
Shu, J
Singh, J
Singh, S
Sinha, K
Sinnis, J T
Smith, M S
Snow, W M
Sokolov, A V
Sushkov, A O
Tait, T M P
Takhistov, V
Temples, D J
Thomas, J H
Tobar, M E
Vandegar, M
Vogel, J K
Wang, Z
Wickenbrock, A
Winslow, L
Wooten, M
Young, B A
F Yu
Zhou, K
description Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white paper summarizes axion phenomenology and outlines next-generation laboratory experiments proposed to detect axion dark matter. There are vibrant synergies with astrophysical searches and advances in instrumentation including quantum-enabled readout, high-Q resonators and cavities and large high-field magnets. This white paper outlines a clear roadmap to discovery, and shows that the US is well-positioned to be at the forefront of the search for axion dark matter in the coming decade.
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They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white paper summarizes axion phenomenology and outlines next-generation laboratory experiments proposed to detect axion dark matter. There are vibrant synergies with astrophysical searches and advances in instrumentation including quantum-enabled readout, high-Q resonators and cavities and large high-field magnets. 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20230329</creationdate><title>Axion Dark Matter</title><author>Adams, C B ; Aggarwal, N ; Agrawal, A ; Bartram, C ; Bekker, H ; Belov, P ; Berggren, K K ; Boutan, C ; Bowring, D ; Budker, D ; Caldwell, A ; Cervantes, R ; Chakrabarty, S S ; Chou, A ; Co, R T ; Conrad, J ; Croon, D ; D'Agnolo, R T ; Demarteau, M ; DePorzio, N ; L Di Luzio ; Diaz-Morcillo, A ; Dona, K ; Droster, A ; Dunne, K ; Döbrich, B ; Essig, R ; Foster, J W ; Fry, J T ; A Gallo Rosso ; García Barceló, J M ; Irastorza, I G ; Gardner, S ; Ghosh, S ; Giaccone, B ; Giannotti, M ; Grin, D ; Grote, H ; Awida, M H ; Hoof, S ; Hoshino, G ; Irsic, V ; Jackson, H ; Jackson Kimball, D F ; Jaeckel, J ; Jakovcic, K ; Jewell, M J ; Khatiwada, R ; Knirck, S ; Kovachy, T ; Krueger, P ; Kuenstner, S E ; Kurinsky, N A ; Leane, R K ; Leder, A F ; Lee, C ; Lehnert, K W ; Liu, J ; Majorovits, B ; Millar, A J ; Miller, D W ; Mitchell, J ; Nagaitsev, S ; Noroozian, O ; Oblath, N S ; Ouellet, J L ; Peiris, H V ; Perez, K ; Phipps, A ; Pivovaroff, M J ; Quílez, P ; Rapidis, N M ; Robles, V H ; Rudolph, J ; Rybka, G ; Safdari, M ; Safdi, B R ; Shu, J ; Singh, J ; Singh, S ; Sinha, K ; Sinnis, J T ; Smith, M S ; Snow, W M ; Sokolov, A V ; Sushkov, A O ; Tait, T M P ; Takhistov, V ; Temples, D J ; Thomas, J H ; Tobar, M E ; Vandegar, M ; Vogel, J K ; Wang, Z ; Wickenbrock, A ; Winslow, L ; Wooten, M ; Young, B A ; F Yu ; Zhou, K</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_26445920293</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Astronomical models</topic><topic>Cosmology</topic><topic>Dark matter</topic><topic>Magnets</topic><topic>Phenomenology</topic><toplevel>online_resources</toplevel><creatorcontrib>Adams, C B</creatorcontrib><creatorcontrib>Aggarwal, N</creatorcontrib><creatorcontrib>Agrawal, A</creatorcontrib><creatorcontrib>Bartram, C</creatorcontrib><creatorcontrib>Bekker, H</creatorcontrib><creatorcontrib>Belov, P</creatorcontrib><creatorcontrib>Berggren, K K</creatorcontrib><creatorcontrib>Boutan, C</creatorcontrib><creatorcontrib>Bowring, D</creatorcontrib><creatorcontrib>Budker, D</creatorcontrib><creatorcontrib>Caldwell, A</creatorcontrib><creatorcontrib>Cervantes, R</creatorcontrib><creatorcontrib>Chakrabarty, S S</creatorcontrib><creatorcontrib>Chou, 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D</creatorcontrib><creatorcontrib>Grote, H</creatorcontrib><creatorcontrib>Awida, M H</creatorcontrib><creatorcontrib>Hoof, S</creatorcontrib><creatorcontrib>Hoshino, G</creatorcontrib><creatorcontrib>Irsic, V</creatorcontrib><creatorcontrib>Jackson, H</creatorcontrib><creatorcontrib>Jackson Kimball, D F</creatorcontrib><creatorcontrib>Jaeckel, J</creatorcontrib><creatorcontrib>Jakovcic, K</creatorcontrib><creatorcontrib>Jewell, M J</creatorcontrib><creatorcontrib>Khatiwada, R</creatorcontrib><creatorcontrib>Knirck, S</creatorcontrib><creatorcontrib>Kovachy, T</creatorcontrib><creatorcontrib>Krueger, P</creatorcontrib><creatorcontrib>Kuenstner, S E</creatorcontrib><creatorcontrib>Kurinsky, N A</creatorcontrib><creatorcontrib>Leane, R K</creatorcontrib><creatorcontrib>Leder, A F</creatorcontrib><creatorcontrib>Lee, C</creatorcontrib><creatorcontrib>Lehnert, K W</creatorcontrib><creatorcontrib>Liu, J</creatorcontrib><creatorcontrib>Majorovits, B</creatorcontrib><creatorcontrib>Millar, A J</creatorcontrib><creatorcontrib>Miller, D W</creatorcontrib><creatorcontrib>Mitchell, J</creatorcontrib><creatorcontrib>Nagaitsev, S</creatorcontrib><creatorcontrib>Noroozian, O</creatorcontrib><creatorcontrib>Oblath, N S</creatorcontrib><creatorcontrib>Ouellet, J L</creatorcontrib><creatorcontrib>Peiris, H V</creatorcontrib><creatorcontrib>Perez, K</creatorcontrib><creatorcontrib>Phipps, A</creatorcontrib><creatorcontrib>Pivovaroff, M J</creatorcontrib><creatorcontrib>Quílez, P</creatorcontrib><creatorcontrib>Rapidis, N M</creatorcontrib><creatorcontrib>Robles, V H</creatorcontrib><creatorcontrib>Rudolph, J</creatorcontrib><creatorcontrib>Rybka, G</creatorcontrib><creatorcontrib>Safdari, M</creatorcontrib><creatorcontrib>Safdi, B R</creatorcontrib><creatorcontrib>Shu, J</creatorcontrib><creatorcontrib>Singh, J</creatorcontrib><creatorcontrib>Singh, S</creatorcontrib><creatorcontrib>Sinha, K</creatorcontrib><creatorcontrib>Sinnis, J T</creatorcontrib><creatorcontrib>Smith, M S</creatorcontrib><creatorcontrib>Snow, W M</creatorcontrib><creatorcontrib>Sokolov, A V</creatorcontrib><creatorcontrib>Sushkov, A O</creatorcontrib><creatorcontrib>Tait, T M P</creatorcontrib><creatorcontrib>Takhistov, V</creatorcontrib><creatorcontrib>Temples, D J</creatorcontrib><creatorcontrib>Thomas, J H</creatorcontrib><creatorcontrib>Tobar, M E</creatorcontrib><creatorcontrib>Vandegar, M</creatorcontrib><creatorcontrib>Vogel, J K</creatorcontrib><creatorcontrib>Wang, Z</creatorcontrib><creatorcontrib>Wickenbrock, A</creatorcontrib><creatorcontrib>Winslow, L</creatorcontrib><creatorcontrib>Wooten, M</creatorcontrib><creatorcontrib>Young, B A</creatorcontrib><creatorcontrib>F Yu</creatorcontrib><creatorcontrib>Zhou, K</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science &amp; Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Access via ProQuest (Open Access)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Adams, C B</au><au>Aggarwal, N</au><au>Agrawal, A</au><au>Bartram, C</au><au>Bekker, H</au><au>Belov, P</au><au>Berggren, K K</au><au>Boutan, C</au><au>Bowring, D</au><au>Budker, D</au><au>Caldwell, A</au><au>Cervantes, R</au><au>Chakrabarty, S S</au><au>Chou, A</au><au>Co, R T</au><au>Conrad, J</au><au>Croon, D</au><au>D'Agnolo, R T</au><au>Demarteau, M</au><au>DePorzio, N</au><au>L Di Luzio</au><au>Diaz-Morcillo, A</au><au>Dona, K</au><au>Droster, A</au><au>Dunne, K</au><au>Döbrich, B</au><au>Essig, R</au><au>Foster, J W</au><au>Fry, J T</au><au>A Gallo Rosso</au><au>García Barceló, J M</au><au>Irastorza, I G</au><au>Gardner, S</au><au>Ghosh, S</au><au>Giaccone, B</au><au>Giannotti, M</au><au>Grin, D</au><au>Grote, H</au><au>Awida, M H</au><au>Hoof, S</au><au>Hoshino, G</au><au>Irsic, V</au><au>Jackson, H</au><au>Jackson Kimball, D F</au><au>Jaeckel, J</au><au>Jakovcic, K</au><au>Jewell, M J</au><au>Khatiwada, R</au><au>Knirck, S</au><au>Kovachy, T</au><au>Krueger, P</au><au>Kuenstner, S E</au><au>Kurinsky, N A</au><au>Leane, R K</au><au>Leder, A F</au><au>Lee, C</au><au>Lehnert, K W</au><au>Liu, J</au><au>Majorovits, B</au><au>Millar, A J</au><au>Miller, D W</au><au>Mitchell, J</au><au>Nagaitsev, S</au><au>Noroozian, O</au><au>Oblath, N S</au><au>Ouellet, J L</au><au>Peiris, H V</au><au>Perez, K</au><au>Phipps, A</au><au>Pivovaroff, M J</au><au>Quílez, P</au><au>Rapidis, N M</au><au>Robles, V H</au><au>Rudolph, J</au><au>Rybka, G</au><au>Safdari, M</au><au>Safdi, B R</au><au>Shu, J</au><au>Singh, J</au><au>Singh, S</au><au>Sinha, K</au><au>Sinnis, J T</au><au>Smith, M S</au><au>Snow, W M</au><au>Sokolov, A V</au><au>Sushkov, A O</au><au>Tait, T M P</au><au>Takhistov, V</au><au>Temples, D J</au><au>Thomas, J H</au><au>Tobar, M E</au><au>Vandegar, M</au><au>Vogel, J K</au><au>Wang, Z</au><au>Wickenbrock, A</au><au>Winslow, L</au><au>Wooten, M</au><au>Young, B A</au><au>F Yu</au><au>Zhou, K</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Axion Dark Matter</atitle><jtitle>arXiv.org</jtitle><date>2023-03-29</date><risdate>2023</risdate><eissn>2331-8422</eissn><abstract>Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This Snowmass white paper summarizes axion phenomenology and outlines next-generation laboratory experiments proposed to detect axion dark matter. There are vibrant synergies with astrophysical searches and advances in instrumentation including quantum-enabled readout, high-Q resonators and cavities and large high-field magnets. This white paper outlines a clear roadmap to discovery, and shows that the US is well-positioned to be at the forefront of the search for axion dark matter in the coming decade.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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subjects Astronomical models
Cosmology
Dark matter
Magnets
Phenomenology
title Axion Dark Matter
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