Search for axion dark matter with the QUAX-LNF tunable haloscope

被引：0
|
作者：
Rettaroli, A. [1 ]
Alesini, D. [1 ]
Babusci, D. [1 ]
Braggio, C. [2 ,3 ]
Carugno, G. [2 ]
DAgostino, D. [4 ,5 ]
DElia, A. [1 ]
Di Gioacchino, D. [1 ]
Di Vora, R. [6 ]
Falferi, P. [7 ,8 ]
Gambardella, U. [4 ,5 ]
Gardikiotis, A. [2 ]
Gatti, C. [1 ]
Ligi, C. [1 ]
Lombardi, A. [3 ]
Maccarrone, G. [1 ]
Ortolan, A. [6 ]
Ruoso, G. [6 ]
Tocci, S. [1 ]
Vidali, G. [1 ,9 ]
机构：
[1] Ist Nazl Fis Nucl, Lab Nazl Frascati, Rome, Italy
[2] Ist Nazl Fis Nucl, Sez Padova, Padua, Italy
[3] Dipartimento Fis & Astron, Padua, Italy
[4] Dipartimento Fis ER Caianiello, Salerno, Italy
[5] Ist Nazl Fis Nucl, Sez Napoli, Naples, Italy
[6] Ist Nazl Fis Nucl, Lab Nazl Legnaro, Padua, Italy
[7] CNR Fdn Bruno Kessler, Ist Foton & Nanotecnol, I-38123 Povo, Trento, Italy
[8] Ist Nazl Fis Nucl, TIFPA, Povo, Trento, Italy
[9] Univ Roma La Sapienza, Dipartimento Fis, Rome, Italy
来源：
PHYSICAL REVIEW D | 2024年 / 110卷 / 02期
关键词：
CP CONSERVATION; INVARIANCE;
D O I：
10.1103/PhysRevD.110.022008
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We report the first experimental results obtained with the new haloscope of the QUAX experiment located at Laboratori Nazionali di Frascati of INFN (LNF). The haloscope is composed of a OFHC Cu resonant cavity cooled down to about 30 mK and immersed in a magnetic field of 8 T. The cavity frequency was varied in a 6 MHz range between 8.831496 and 8.83803 GHz. This corresponds to a previously unprobed mass range between 36.52413 and 36.5511 mu eV. We don't observe any excess in the power spectrum and set limits on the axion-photon coupling in this mass range down to g a gamma gamma < 0.882 x 10 - 13 GeV-1 - 1 with the confidence level set to 90%.
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页数：10
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