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

Fuente: arXiv

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Bibliographic Details
Main Authors:	Rettaroli, A., Alesini, D., Babusci, D., Braggio, C., Carugno, G., D'Agostino, D., D'Elia, A., Di Gioacchino, D., Di Vora, R., Falferi, P., Gambardella, U., Gardikiotis, A., Gatti, C., Iannone, G., Ligi, C., Lombardi, A., Maccarrone, G., Ortolan, A., Ruoso, G., Tocci, S., Vidali, G.
Format:	Preprint
Published:	2024
Subjects:	Instrumentation and Detectors Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment
Online Access:	Acceder al recurso
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author	Rettaroli, A. Alesini, D. Babusci, D. Braggio, C. Carugno, G. D'Agostino, D. D'Elia, A. Di Gioacchino, D. Di Vora, R. Falferi, P. Gambardella, U. Gardikiotis, A. Gatti, C. Iannone, G. Ligi, C. Lombardi, A. Maccarrone, G. Ortolan, A. Ruoso, G. Tocci, S. Vidali, G.
author_facet	Rettaroli, A. Alesini, D. Babusci, D. Braggio, C. Carugno, G. D'Agostino, D. D'Elia, A. Di Gioacchino, D. Di Vora, R. Falferi, P. Gambardella, U. Gardikiotis, A. Gatti, C. Iannone, G. Ligi, C. Lombardi, A. Maccarrone, G. Ortolan, A. Ruoso, G. Tocci, S. Vidali, G.
contents	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 $μ$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 $g_{aγγ} < 0.861 \times 10^{-13}$ GeV$^{-1}$ with the confidence level set at $90\%$.
format	Preprint
id	arxiv_https___arxiv_org_abs_2402_19063
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Search for Axion dark matter with the QUAX-LNF tunable haloscope Rettaroli, A. Alesini, D. Babusci, D. Braggio, C. Carugno, G. D'Agostino, D. D'Elia, A. Di Gioacchino, D. Di Vora, R. Falferi, P. Gambardella, U. Gardikiotis, A. Gatti, C. Iannone, G. Ligi, C. Lombardi, A. Maccarrone, G. Ortolan, A. Ruoso, G. Tocci, S. Vidali, G. Instrumentation and Detectors Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment 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 $μ$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 $g_{aγγ} < 0.861 \times 10^{-13}$ GeV$^{-1}$ with the confidence level set at $90\%$.
title	Search for Axion dark matter with the QUAX-LNF tunable haloscope
topic	Instrumentation and Detectors Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment
url	https://arxiv.org/abs/2402.19063