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001     617437
005     20250115142343.0
024 7 _ |a Egge:2023cos
|2 INSPIRETeX
024 7 _ |a inspire:2725450
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024 7 _ |a arXiv:2311.13359
|2 arXiv
024 7 _ |a 10.3204/PUBDB-2024-06788
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037 _ _ |a PUBDB-2024-06788
041 _ _ |a English
082 _ _ |a 530
088 _ _ |a arXiv:2311.13359
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088 _ _ |a FERMILAB-PUB-24-0399-PPD
|2 Fermilab
100 1 _ |a Egge
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245 _ _ |a Experimental determination of axion signal power of dish antennas and dielectric haloscopes using the reciprocity approach
260 _ _ |c 2024
336 7 _ |a Preprint
|b preprint
|m preprint
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336 7 _ |a WORKING_PAPER
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336 7 _ |a Electronic Article
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336 7 _ |a preprint
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336 7 _ |a ARTICLE
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336 7 _ |a Output Types/Working Paper
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500 _ _ |a JCAP04(2024)005. v2, updated to match journal version, 18 pages, 10 figures
520 _ _ |a The reciprocity approach is a powerful method to determine the expected signal power of axion haloscopes in a model-independent way. Especially for open and broadband setups like the MADMAX dielectric haloscope the sensitivity to the axion field is difficult to calibrate since they do not allow discrete eigenmode analysis and are optically too large to fully simulate. The central idea of the reciprocity approach is to measure a reflection-induced test field in the setup instead of trying to simulate the axion-induced field. In this article, the reciprocity approach is used to determine the expected signal power of a dish antenna and a minimal dielectric haloscope directly from measurements. The results match expectations from simulation but also include important systematic effects that are too difficult to simulate. In particular, the effect of antenna standing waves and higher order mode perturbations can be quantified for the first time in a dielectric haloscope.
536 _ _ |a 611 - Fundamental Particles and Forces (POF4-611)
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536 _ _ |a DFG project G:(GEPRIS)390833306 - EXC 2121: Quantum Universe (390833306)
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588 _ _ |a Dataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
650 _ 7 |a dielectric
|2 INSPIRE
650 _ 7 |a axion: dark matter
|2 INSPIRE
650 _ 7 |a dark matter: detector
|2 INSPIRE
650 _ 7 |a resonance: cavity
|2 INSPIRE
650 _ 7 |a current: density
|2 INSPIRE
650 _ 7 |a reflection
|2 INSPIRE
650 _ 7 |a frequency
|2 INSPIRE
650 _ 7 |a perturbation
|2 INSPIRE
650 _ 7 |a calibration
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650 _ 7 |a sensitivity
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650 _ 7 |a higher-order
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650 _ 7 |a MADMAX
|2 INSPIRE
650 _ 7 |a experimental methods
|2 INSPIRE
650 _ 7 |a experimental results
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650 _ 7 |a dark matter detectors
|2 autogen
650 _ 7 |a dark matter experiments
|2 autogen
693 _ _ |0 EXP:(DE-H253)MADMAX-20210101
|5 EXP:(DE-H253)MADMAX-20210101
|e MAgnetized Disc and Mirror Axion eXperiment
|x 0
700 1 _ |a Ekmedžić, M.
|b 1
700 1 _ |a Gardikiotis, A.
|0 0000-0002-4435-2695
|b 2
700 1 _ |a Garutti, E.
|b 3
700 1 _ |a Heyminck, S.
|b 4
700 1 _ |a Kasemann, C.
|b 5
700 1 _ |a Knirck, S.
|0 0000-0002-5714-4545
|b 6
700 1 _ |a Kramer, M.
|b 7
700 1 _ |a Krieger, C.
|b 8
700 1 _ |a Leppla-Weber, D.
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700 1 _ |a Martens, S.
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700 1 _ |a Öz, E.
|0 0000-0003-2621-4990
|b 11
700 1 _ |a Salama, N.
|b 12
700 1 _ |a Schmidt, A.
|0 0000-0003-2711-8984
|b 13
700 1 _ |a Wang, H.
|b 14
700 1 _ |a Wieching, G.
|b 15
856 4 _ |y OpenAccess
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910 1 _ |a Deutsches Elektronen-Synchrotron
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910 1 _ |a External Institute
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913 1 _ |a DE-HGF
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914 1 _ |y 2024
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915 _ _ |a Creative Commons Attribution CC BY 4.0
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915 _ _ |a Published
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920 1 _ |0 I:(DE-H253)UNI_EXP-20120731
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920 1 _ |0 I:(DE-H253)RWTH-20140517
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920 1 _ |0 I:(DE-H253)UBonn-20140228
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980 _ _ |a I:(DE-H253)UNI_EXP-20120731
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980 1 _ |a FullTexts

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