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%.

引用

页数：10

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