Samantha M. Lewis, Dillon T. Goulart, Mirelys Carcana Barbosa, Alexander F. Leder, Aarav M. Sindhwad, Isabella Urdinaran, Karl van Bibber
{"title":"A tunable photonic band gap resonator for axion dark matter searches","authors":"Samantha M. Lewis, Dillon T. Goulart, Mirelys Carcana Barbosa, Alexander F. Leder, Aarav M. Sindhwad, Isabella Urdinaran, Karl van Bibber","doi":"arxiv-2408.03861","DOIUrl":null,"url":null,"abstract":"Axions are a well-motivated dark matter candidate particle. Haloscopes aim to\ndetect axions in the galactic halo by measuring the photon signal resulting\nfrom axions interacting with a strong magnetic field. Existing haloscopes are\nprimarily targeting axion masses which produce microwave-range photons and rely\non microwave resonators to enhance the signal power. Only a limited subset of\nresonator modes are useful for this process, and current cylindrical-style\ncavities suffer from mode mixing and crowding from other fundamental modes. The\nmajority of these modes can be eliminated by using photonic band gap (PBG)\nresonators. The band gap behavior of these structures allows for a resonator\nwith mode selectivity based on frequency. We present results from the first\ntunable PBG resonator, a proof-of-concept design with a footprint compatible\nwith axion haloscopes. We have thoroughly characterized the tuning range of two\nversions of the structure and report the successful confinement of the\noperating TM$_{010}$ mode and the elimination of all TE modes within the tuning\nrange.","PeriodicalId":501374,"journal":{"name":"arXiv - PHYS - Instrumentation and Detectors","volume":"57 1","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-08-07","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"arXiv - PHYS - Instrumentation and Detectors","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/arxiv-2408.03861","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
Axions are a well-motivated dark matter candidate particle. Haloscopes aim to
detect axions in the galactic halo by measuring the photon signal resulting
from axions interacting with a strong magnetic field. Existing haloscopes are
primarily targeting axion masses which produce microwave-range photons and rely
on microwave resonators to enhance the signal power. Only a limited subset of
resonator modes are useful for this process, and current cylindrical-style
cavities suffer from mode mixing and crowding from other fundamental modes. The
majority of these modes can be eliminated by using photonic band gap (PBG)
resonators. The band gap behavior of these structures allows for a resonator
with mode selectivity based on frequency. We present results from the first
tunable PBG resonator, a proof-of-concept design with a footprint compatible
with axion haloscopes. We have thoroughly characterized the tuning range of two
versions of the structure and report the successful confinement of the
operating TM$_{010}$ mode and the elimination of all TE modes within the tuning
range.