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000617437 0247_ $$2arXiv$$aarXiv:2311.13359
000617437 0247_ $$2datacite_doi$$a10.3204/PUBDB-2024-06788
000617437 037__ $$aPUBDB-2024-06788
000617437 041__ $$aEnglish
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000617437 088__ $$2arXiv$$aarXiv:2311.13359
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000617437 1001_ $$0P:(DE-HGF)0$$aEgge$$b0$$eCorresponding author
000617437 245__ $$aExperimental determination of axion signal power of dish antennas and dielectric haloscopes using the reciprocity approach
000617437 260__ $$c2024
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000617437 500__ $$aJCAP04(2024)005. v2, updated to match journal version, 18 pages, 10 figures
000617437 520__ $$aThe 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.
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000617437 650_7 $$2INSPIRE$$adielectric
000617437 650_7 $$2INSPIRE$$aaxion: dark matter
000617437 650_7 $$2INSPIRE$$adark matter: detector
000617437 650_7 $$2INSPIRE$$aresonance: cavity
000617437 650_7 $$2INSPIRE$$acurrent: density
000617437 650_7 $$2INSPIRE$$areflection
000617437 650_7 $$2INSPIRE$$afrequency
000617437 650_7 $$2INSPIRE$$aperturbation
000617437 650_7 $$2INSPIRE$$acalibration
000617437 650_7 $$2INSPIRE$$asensitivity
000617437 650_7 $$2INSPIRE$$ahigher-order
000617437 650_7 $$2INSPIRE$$aMADMAX
000617437 650_7 $$2INSPIRE$$aexperimental methods
000617437 650_7 $$2INSPIRE$$aexperimental results
000617437 650_7 $$2autogen$$adark matter detectors
000617437 650_7 $$2autogen$$adark matter experiments
000617437 693__ $$0EXP:(DE-H253)MADMAX-20210101$$5EXP:(DE-H253)MADMAX-20210101$$eMAgnetized Disc and Mirror Axion eXperiment$$x0
000617437 7001_ $$aEkmedžić, M.$$b1
000617437 7001_ $$00000-0002-4435-2695$$aGardikiotis, A.$$b2
000617437 7001_ $$aGarutti, E.$$b3
000617437 7001_ $$aHeyminck, S.$$b4
000617437 7001_ $$aKasemann, C.$$b5
000617437 7001_ $$00000-0002-5714-4545$$aKnirck, S.$$b6
000617437 7001_ $$aKramer, M.$$b7
000617437 7001_ $$aKrieger, C.$$b8
000617437 7001_ $$0P:(DE-H253)PIP1088832$$aLeppla-Weber, D.$$b9$$udesy
000617437 7001_ $$aMartens, S.$$b10
000617437 7001_ $$00000-0003-2621-4990$$aÖz, E.$$b11
000617437 7001_ $$aSalama, N.$$b12
000617437 7001_ $$00000-0003-2711-8984$$aSchmidt, A.$$b13
000617437 7001_ $$aWang, H.$$b14
000617437 7001_ $$aWieching, G.$$b15
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000617437 9141_ $$y2024
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000617437 9201_ $$0I:(DE-H253)UNI_EXP-20120731$$kUNI/EXP$$lUni Hamburg / Experimentalphysik$$x0
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000617437 9201_ $$0I:(DE-H253)UBonn-20140228$$kUBonn$$lUniversität Bonn$$x3
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