Details

Autor(en) / Beteiligte

• Bartram, C
• Braine, T
• Burns, E
• Cervantes, R
• Crisosto, N
• Du, N
• Korandla, H
• Leum, G
• Mohapatra, P
• Nitta, T
• Rosenberg, L J
• Rybka, G
• Yang, J
• Clarke, John
• Siddiqi, I
• Agrawal, A
• Dixit, A V
• Awida, M H
• Chou, A S
• Hollister, M
• Knirck, S
• Sonnenschein, A
• Wester, W
• Gleason, J R
• Hipp, A T
• Jois, S
• Sikivie, P
• Sullivan, N S
• Tanner, D B
• Lentz, E
• Khatiwada, R
• Carosi, G
• Robertson, N
• Woollett, N
• Duffy, L D
• Boutan, C
• Jones, M
• LaRoque, B H
• Oblath, N S
• Taubman, M S
• Daw, E J
• Perry, M G
• Buckley, J H
• Gaikwad, C
• Hoffman, J
• Murch, K W
• Goryachev, M
• McAllister, B T
• Quiskamp, A
• Thomson, C
• Tobar, M E

Titel

Search for Invisible Axion Dark Matter in the 3.3-4.2  μeV Mass Range

Ist Teil von

• Physical review letters, 2021-12, Vol.127 (26), p.261803-261803, Article 261803

Ort / Verlag

United States: American Physical Society

Erscheinungsjahr

2021

Link zum Volltext

Quelle

American Physical Society Journals

Beschreibungen/Notizen

• We report the results from a haloscope search for axion dark matter in the 3.3-4.2  μeV mass range. This search excludes the axion-photon coupling predicted by one of the benchmark models of "invisible" axion dark matter, the Kim-Shifman-Vainshtein-Zakharov model. This sensitivity is achieved using a large-volume cavity, a superconducting magnet, an ultra low noise Josephson parametric amplifier, and sub-Kelvin temperatures. The validity of our detection procedure is ensured by injecting and detecting blind synthetic axion signals.