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Searching for dark matter with plasma haloscopes

Authors :
Millar, Alexander J.
Anlage, Steven M.
Balafendiev, Rustam
Belov, Pavel
van Bibber, Karl
Conrad, Jan
Demarteau, Marcel
Droster, Alexander
Dunne, Katherine
Gallo Rosso, Andrea
Gudmundsson, Jon E.
Jackson, Heather
Kaur, Gagandeep
Klaesson, Tove
Kowitt, Nolan
Lawson, Matthew
Leder, Alexander
Miyazaki, Akira
Morampudi, Sid
V. Peiris, Hiranya
Røising, Henrik S.
Singh, Gaganpreet
Sun, Dajie
Thomas, Jacob H.
Wilczek, Frank
Withington, Stafford
Wooten, Mackenzie
Dilling, Jens
Febbraro, Michael
Knirck, Stefan
Marvinney, Claire
Millar, Alexander J.
Anlage, Steven M.
Balafendiev, Rustam
Belov, Pavel
van Bibber, Karl
Conrad, Jan
Demarteau, Marcel
Droster, Alexander
Dunne, Katherine
Gallo Rosso, Andrea
Gudmundsson, Jon E.
Jackson, Heather
Kaur, Gagandeep
Klaesson, Tove
Kowitt, Nolan
Lawson, Matthew
Leder, Alexander
Miyazaki, Akira
Morampudi, Sid
V. Peiris, Hiranya
Røising, Henrik S.
Singh, Gaganpreet
Sun, Dajie
Thomas, Jacob H.
Wilczek, Frank
Withington, Stafford
Wooten, Mackenzie
Dilling, Jens
Febbraro, Michael
Knirck, Stefan
Marvinney, Claire
Publication Year :
2023

Abstract

We summarize the recent progress of the Axion Longitudinal Plasma Haloscope (ALPHA) Consortium, a new experimental collaboration to build a plasma haloscope to search for axions and dark photons. The plasma haloscope is a novel method for the detection of the resonant conversion of light dark matter to photons. ALPHA will be sensitive to QCD axions over almost a decade of parameter space, potentially discovering dark matter and resolving the strong CP problem. Unlike traditional cavity haloscopes, which are generally limited in volume by the Compton wavelength of the dark matter, plasma haloscopes use a wire metamaterial to create a tuneable artificial plasma frequency, decoupling the wavelength of light from the Compton wavelength and allowing for much stronger signals. We develop the theoretical foundations of plasma haloscopes and discuss recent experimental progress. Finally, we outline a baseline design for ALPHA and show that a full-scale experiment could discover QCD axions over almost a decade of parameter space.

Details

Database :
OAIster
Notes :
application/pdf, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1387018208
Document Type :
Electronic Resource
Full Text :
https://doi.org/10.1103.PhysRevD.107.055013