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A first look on 3D effects in open axion haloscopes
Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany..
Hamburg Univ, D-22761 Hamburg, Germany..
KTH, Centres, Nordic Institute for Theoretical Physics NORDITA. Stockholm Univ, Oskar Klein Ctr Cosmoparticle Phys, Dept Phys, S-10691 Stockholm, Sweden.;Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden..
Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany.;Univ Zaragoza, E-50009 Zaragoza, Spain..
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2019 (English)In: Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, E-ISSN 1475-7516, no 8, article id 026Article in journal (Refereed) Published
Abstract [en]

We explore finite size 3D effects in open axion haloscopes such as a dish antenna, a dielectric disk and a minimal dielectric haloscope consisting of a mirror and one dielectric disk. Particularly dielectric haloscopes are a promising new method for detecting dark matter axions in the mass range above 40 mu eV. By using two specialized independent approaches - based on finite element methods and Fourier optics - we compute the electromagnetic fields in these settings expected in the presence of an axion dark matter field. This allows us to study diffraction and near field effects for realistically sized experimental setups in contrast to earlier idealized 1D studies with infinitely extended mirrors and disks. We also study axion velocity effects and disk tiling. Diffraction effects are found to become less relevant towards larger axion masses and for the larger disk radii for example aimed at in full size dielectric haloscopes such as MADMAX. The insights of our study not only provide a foundation for a realistic modelling of open axion dark matter search experiments in general, they are in particular also the first results taking into account 3D effects for dielectric haloscopes.

Place, publisher, year, edition, pages
IOP PUBLISHING LTD , 2019. no 8, article id 026
Keywords [en]
axions, dark matter simulations, dark matter detectors, dark matter experiments
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-257821DOI: 10.1088/1475-7516/2019/08/026ISI: 000482013000006Scopus ID: 2-s2.0-85072100132OAI: oai:DiVA.org:kth-257821DiVA, id: diva2:1348970
Note

QC 20190906

Available from: 2019-09-06 Created: 2019-09-06 Last updated: 2019-10-04Bibliographically approved

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