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Sensitivity of a closed dielectric haloscope to axion dark matter

Fuente: arXiv

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Hauptverfasser:	Ivanov, A., Leppla-Weber, D., Garcia, B. Ary dos Santos, Bergermann, D., Byun, H., Caldwell, A., Dabhi, V., Diaconu, C., Diehl, J., Dvali, G., Döbrich, B., Egge, J., Garutti, E., Heyminck, S., Houdy, T., Hubaut, F., Jochum, J., Kazemipour, A., Kermaidic, Y., Knirck, S., Kramer, M., Kreikemeyer-Lorenzo, D., Krieger, C., Lee, C., Li, X., Lindner, A., Majorovits, B., Maldonado, J., Martini, A., Miyazaki, A., Öz, E., Pralavorio, P., Raffelt, G., Redondo, J., Ringwald, A., Schaffran, J., Schmidt, A., Stankewitz, L., Steffen, F., Strandhagen, C., Usherov, I., Wang, H., Wieching, G.
Format:	Preprint
Veröffentlicht:	2026
Schlagworte:	Instrumentation and Methods for Astrophysics High Energy Physics - Experiment
Online-Zugang:	Acceder al recurso
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_version_	1866912944614277120
author	Ivanov, A. Leppla-Weber, D. Garcia, B. Ary dos Santos Bergermann, D. Byun, H. Caldwell, A. Dabhi, V. Diaconu, C. Diehl, J. Dvali, G. Döbrich, B. Egge, J. Garutti, E. Heyminck, S. Houdy, T. Hubaut, F. Jochum, J. Kazemipour, A. Kermaidic, Y. Knirck, S. Kramer, M. Kreikemeyer-Lorenzo, D. Krieger, C. Lee, C. Li, X. Lindner, A. Majorovits, B. Maldonado, J. Martini, A. Miyazaki, A. Öz, E. Pralavorio, P. Raffelt, G. Redondo, J. Ringwald, A. Schaffran, J. Schmidt, A. Stankewitz, L. Steffen, F. Strandhagen, C. Usherov, I. Wang, H. Wieching, G.
author_facet	Ivanov, A. Leppla-Weber, D. Garcia, B. Ary dos Santos Bergermann, D. Byun, H. Caldwell, A. Dabhi, V. Diaconu, C. Diehl, J. Dvali, G. Döbrich, B. Egge, J. Garutti, E. Heyminck, S. Houdy, T. Hubaut, F. Jochum, J. Kazemipour, A. Kermaidic, Y. Knirck, S. Kramer, M. Kreikemeyer-Lorenzo, D. Krieger, C. Lee, C. Li, X. Lindner, A. Majorovits, B. Maldonado, J. Martini, A. Miyazaki, A. Öz, E. Pralavorio, P. Raffelt, G. Redondo, J. Ringwald, A. Schaffran, J. Schmidt, A. Stankewitz, L. Steffen, F. Strandhagen, C. Usherov, I. Wang, H. Wieching, G.
contents	We present a method to determine the sensitivity of a closed dielectric haloscope to axion dark matter. Dielectric haloscopes aim to probe the theoretically well-motivated axion mass range of ~26 $\mathrmμ$eV to ~500 $\mathrmμ$eV by utilizing a stack of dielectric disks and a mirror to enhance the axion-photon conversion within an external magnetic field. Their conversion volume is nearly axion-mass independent, thereby favoring large-scale designs to increase sensitivity. The large volume causes simulations to be computationally expensive and time-consuming. This paper presents a simple model that can be used to determine the sensitivity of the experiment with minimal computational resources. The model is able to describe the electromagnetic response of a closed dielectric haloscope, accounting for realistic geometric imperfections, as well as the noise introduced by the receiver system. It is applied to data taken with a MAgnetized Disk and Mirror Axion Experiment (MADMAX) prototype within the 1.6 T Morpurgo magnet at CERN. This work underpins the first axion dark matter search using a dielectric haloscope and provides the foundation for future dark matter searches with MADMAX.
format	Preprint
id	arxiv_https___arxiv_org_abs_2603_05006
institution	arXiv
publishDate	2026
record_format	arxiv
spellingShingle	Sensitivity of a closed dielectric haloscope to axion dark matter Ivanov, A. Leppla-Weber, D. Garcia, B. Ary dos Santos Bergermann, D. Byun, H. Caldwell, A. Dabhi, V. Diaconu, C. Diehl, J. Dvali, G. Döbrich, B. Egge, J. Garutti, E. Heyminck, S. Houdy, T. Hubaut, F. Jochum, J. Kazemipour, A. Kermaidic, Y. Knirck, S. Kramer, M. Kreikemeyer-Lorenzo, D. Krieger, C. Lee, C. Li, X. Lindner, A. Majorovits, B. Maldonado, J. Martini, A. Miyazaki, A. Öz, E. Pralavorio, P. Raffelt, G. Redondo, J. Ringwald, A. Schaffran, J. Schmidt, A. Stankewitz, L. Steffen, F. Strandhagen, C. Usherov, I. Wang, H. Wieching, G. Instrumentation and Methods for Astrophysics High Energy Physics - Experiment We present a method to determine the sensitivity of a closed dielectric haloscope to axion dark matter. Dielectric haloscopes aim to probe the theoretically well-motivated axion mass range of ~26 $\mathrmμ$eV to ~500 $\mathrmμ$eV by utilizing a stack of dielectric disks and a mirror to enhance the axion-photon conversion within an external magnetic field. Their conversion volume is nearly axion-mass independent, thereby favoring large-scale designs to increase sensitivity. The large volume causes simulations to be computationally expensive and time-consuming. This paper presents a simple model that can be used to determine the sensitivity of the experiment with minimal computational resources. The model is able to describe the electromagnetic response of a closed dielectric haloscope, accounting for realistic geometric imperfections, as well as the noise introduced by the receiver system. It is applied to data taken with a MAgnetized Disk and Mirror Axion Experiment (MADMAX) prototype within the 1.6 T Morpurgo magnet at CERN. This work underpins the first axion dark matter search using a dielectric haloscope and provides the foundation for future dark matter searches with MADMAX.
title	Sensitivity of a closed dielectric haloscope to axion dark matter
topic	Instrumentation and Methods for Astrophysics High Energy Physics - Experiment
url	https://arxiv.org/abs/2603.05006