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Tunable rectangular resonant cavities for axion haloscopes

Ben T. McAllister1,2,*, Aaron P. Quiskamp2, and Michael E. Tobar2

  • 1ARC Centre of Excellence for Dark Matter Particle Physics, Swinburne University of Technology, John St, Hawthorn Victoria 3122, Australia
  • 2QDM Lab, Department of Physics, University of Western Australia, 35 Stirling Highway, Crawley, Western Australia 6009, Australia

  • *bmcallister@swin.edu.au

Phys. Rev. D 109, 015013 – Published 16 January, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.015013

Abstract

Axions are a compelling dark matter candidate, and one of the primary techniques employed to search for them is the axion haloscope, in which a resonant cavity is deployed inside a strong magnetic field so that some of the surrounding axions may convert into photons via the inverse Primakoff effect and become trapped inside the resonator. Resonant cavity design is critical to the sensitivity of a haloscope, and several geometries have been utilized and proposed. Here we consider a relatively simple concept—a rectangular resonant cavity with a tunable wall—and compare it to the standard tuning rod-type resonators employed in the field. We find that the rectangular cavities support similar modes to cylindrical tuning rod cavities, and have some advantages in terms of axion sensitivity and practicality, particularly when moving to higher frequencies which are of great and growing interest in the international axion dark matter community.

Physics Subject Headings (PhySH)

See Also

Exclusion of Axionlike-Particle Cogenesis Dark Matter in a Mass Window above 100μeV

Aaron Quiskamp, Ben T. McAllister, Paul Altin, Eugene N. Ivanov, Maxim Goryachev, and Michael E. Tobar
Phys. Rev. Lett. 132, 031601 (2024)

Article Text

References (46)

  1. V. C. Rubin and J. Ford, W. Kent, Rotation of the Andromeda Nebula from a spectroscopic survey of emission regions, Astrophys. J. 159, 379 (1970).
  2. C. L. Bennett, D. Larson, J. L. Weiland, N. Jarosik, G. Hinshaw, N. Odegard, K. Smith, R. Hill, B. Gold, M. Halpern et al., Nine-year Wilkinson microwave anisotropy probe (WMAP) observations: Final maps and results, Astrophys. J. Suppl. Ser. 208, 20 (2013).
  3. Planck Collaboration, Planck 2015 results—XIII. Cosmological parameters, Astron. Astrophys. 594, A13 (2016).
  4. R. D. Peccei and H. R. Quinn, CP conservation in the presence of pseudoparticles, Phys. Rev. Lett. 38, 1440 (1977).
  5. F. Wilczek, Problem of strong p and t invariance in the presence of instantons, Phys. Rev. Lett. 40, 279 (1978).
  6. J. Ipser and P. Sikivie, Can galactic halos be made of axions?, Phys. Rev. Lett. 50, 925 (1983).
  7. J. Preskill, M. B. Wise, and F. Wilczek, Cosmology of the invisible axion, Phys. Lett. 120B, 127 (1983).
  8. P. Sikivie, Experimental tests of the “invisible” axion, Phys. Rev. Lett. 51, 1415 (1983).
  9. P. Sikivie, Erratum: Experimental tests of the “invisible” axion, Phys. Rev. Lett. 52, 695(E) (1984).
  10. J. E. Kim, Weak-interaction singlet and strong CP invariance, Phys. Rev. Lett. 43, 103 (1979).
  11. A. R. Zhitnitsky, On possible suppression of the axion hadron interactions (in Russian), Sov. J. Nucl. Phys. 31, 260 (1980), https://www.osti.gov/biblio/7063072.
  12. M. Dine, W. Fischler, and M. Srednicki, A simple solution to the strong {CP} problem with a harmless axion, Phys. Lett. 104B, 199 (1981).
  13. M. Shifman, A. Vainshtein, and V. Zakharov, Can confinement ensure natural CP invariance of strong interactions?, Nucl. Phys. B166, 493 (1980).
  14. M. Dine and W. Fischler, The not-so-harmless axion, Phys. Lett. 120B, 137 (1983).
  15. D. Kim, J. Jeong, S. Youn, Y. Kim, and Y. K. Semertzidis, Revisiting the detection rate for axion haloscopes, J. Cosmol. Astropart. Phys. 03 (2020) 066.
  16. N. Du et al. (ADMX Collaboration), Search for invisible axion dark matter with the axion dark matter experiment, Phys. Rev. Lett. 120, 151301 (2018).
  17. T. Braine et al. (ADMX Collaboration), Extended search for the invisible axion with the axion dark matter experiment, Phys. Rev. Lett. 124, 101303 (2020).
  18. C. Bartram et al. (ADMX Collaboration), Axion dark matter experiment: Run 1b analysis details, Phys. Rev. D 103, 032002 (2021).
  19. C. Bartram et al. (ADMX Collaboration), Search for invisible axion dark matter in the 3.34.2μeV mass range, Phys. Rev. Lett. 127, 261803 (2021).
  20. A. K. Yi et al., Axion dark matter search around 4.55μeV with Dine-Fischler-Srednicki-Zhitnitskii sensitivity, Phys. Rev. Lett. 130, 071002 (2023).
  21. O. Kwon et al., First results from an axion haloscope at capp around 10.7μeV, Phys. Rev. Lett. 126, 191802 (2021).
  22. G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit, Unifying inflation with the axion, dark matter, baryogenesis, and the seesaw mechanism, Phys. Rev. Lett. 118, 071802 (2017).
  23. G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit, Several problems in particle physics and cosmology solved in one smash, Front. Astron. Space Sci. 6, 55 (2019).
  24. L. Zhong et al., Results from phase 1 of the haystac microwave cavity axion experiment, Phys. Rev. D 97, 092001 (2018).
  25. B. M. Brubaker, L. Zhong, S. K. Lamoreaux, K. W. Lehnert, and K. A. V. Bibber, Haystac axion search analysis procedure, Phys. Rev. D 96, 123008 (2017).
  26. A. Quiskamp, B. T. McAllister, P. Altin, E. N. Ivanov, M. Goryachev, and M. E. Tobar, Direct search for dark matter axions excluding alp cogenesis in the 63- to 67μev range with the organ experiment, Sci. Adv. 8, eabq3765 (2022).
  27. B. T. McAllister, G. Flower, E. N. Ivanov, M. Goryachev, J. Bourhill, and M. E. Tobar, The organ experiment: An axion haloscope above 15 GHz, Phys. Dark Universe 18, 67 (2017).
  28. I. Stern, A. A. Chisholm, J. Hoskins, P. Sikivie, N. S. Sullivan, D. B. Tanner, G. Carosi, and K. van Bibber, Cavity design for high-frequency axion dark matter detectors, Rev. Sci. Instrum. 86, 123305 (2015).
  29. J. Jeong, S. Youn, and J. E. Kim, Multiple-cell cavity design for high mass axion searches: An extended study, Nucl. Instrum. Methods Phys. Res., Sect. A 1053, 168327 (2023).
  30. R. Cervantes, G. Carosi, S. Kimes, C. Hanretty, B. H. LaRoque, G. Leum, P. Mohapatra, N. S. Oblath, R. Ottens, Y. Park, G. Rybka, J. Sinnis, and J. Yang, Admx-orpheus first search for 70μeV dark photon dark matter: Detailed design, operations, and analysis, Phys. Rev. D 106, 102002 (2022).
  31. A. P. Quiskamp, B. T. Mcallister, G. Rybka, and M. E. Tobar, Dielectric-boosted sensitivity to cylindrical azimuthally varying transverse-magnetic resonant modes in an axion haloscope, Phys. Rev. Appl. 14, 044051 (2020).
  32. A. Caldwell, G. Dvali, B. Majorovits, A. Millar, G. Raffelt, J. Redondo, O. Reimann, F. Simon, and F. Steffen (MADMAX Working Group), Dielectric haloscopes: A new way to detect axion dark matter, Phys. Rev. Lett. 118, 091801 (2017).
  33. B. T. McAllister, G. Flower, L. E. Tobar, and M. E. Tobar, Tunable supermode dielectric resonators for axion dark-matter haloscopes, Phys. Rev. Appl. 9, 014028 (2018).
  34. G. Carosi, Axion detection experiments, in pPC 2022: XV International Conference on Interconnections between Particle Physics & Cosmology (2022), https://indico.cern.ch/event/1126527/contributions/4811971/.
  35. S. Nam, B. Lee, C. Kwak, and J. Lee, Contactless tuning plunger and its application to k-band frequency-tunable cavity filter, IEEE Trans. Microwave Theory Tech. 67, 2713 (2019).
  36. B. Yassini, M. Yu, and B. Keats, A ka -band fully tunable cavity filter, IEEE Trans. Microwave Theory Tech. 60, 4002 (2012).
  37. B. Yassini, M. Yu, and B. Keats, A Ka-band planar TE011 mode cavity tunable filter using a mode-splitter ring, in 2012 IEEE/MTT-S International Microwave Symposium Digest, Montreal, QC, Canada, 2012 (IEEE, New York, 2012), pp. 1–3, https://ieeexplore.ieee.org/document/6259636.
  38. B. Yassini, M. Yu, D. Smith, and S. Kellett, A ku-band high-q tunable filter with stable tuning response, IEEE Trans. Microwave Theory Tech. 57, 2948 (2009).
  39. A. A. Melcón et al. (CAST Collaboration), First results of the CAST-RADES haloscope search for axions at 34.67μeV, J. High Energy Phys. 10 (2021) 075.
  40. J. M. García-Barceló, A. A. Melcón, A. Díaz-Morcillo, B. Gimeno, A. J. Lozano-Guerrero, J. Monzo-Cabrera, J. R. Navarro-Madrid, and P. Navarro, Methods and restrictions to increase the volume of resonant rectangular-section haloscopes for detecting dark matter axions, J. High Energy Phys. 08 (2023) 098.
  41. B. Aja, S. A. Cuendis, I. Arregui, E. Artal, R. Belén Barreiro, F. J. Casas, M. C. de Ory, A. Díaz-Morcillo, L. de la Fuente and J. D. Gallego et al., The canfranc axion detection experiment (CADEx): Search for axions at 90 GHz with kinetic inductance detectors, J. Cosmol. Astropart. Phys. 11 (2022) 044.
  42. I. Stern, G. Carosi, N. Sullivan, and D. Tanner, Avoided mode crossings in cylindrical microwave cavities, Phys. Rev. Appl. 12, 044016 (2019).
  43. C. Hagmann, P. Sikivie, N. S. Sullivan, and D. B. Tanner, Results from a search for cosmic axions, Phys. Rev. D 42, 1297 (1990).
  44. M. Bayindir, E. Cubukcu, I. Bulu, T. Tut, E. Ozbay, and C. M. Soukoulis, Photonic band gaps, defect characteristics, and waveguiding in two-dimensional disordered dielectric and metallic photonic crystals, Phys. Rev. B 64, 195113 (2001).
  45. J. Jeong, S. Youn, S. Bae, D. Kim, Y. Kim, and Y. K. Semertzidis, Analytical considerations for optimal axion haloscope design, J. Phys. G 49, 055201 (2022).
  46. A. P. Quiskamp, B. T. McAllister, P. Altin, E. N. Ivanov, M. Goryachev, and M. E. Tobar, Exclusion of axionlike-particle cogenesis dark matter in a mass window above 100μeV, Phys. Rev. Lett. 132, 031601 (2024).

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