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  • Letter
  • Open Access

Horn-array haloscope for volume-efficient broadband axion searches

Junu Jeong1,*, Sungwoo Youn1,†, and Yannis K. Semertzidis1,2,‡

  • 1Center for Axion and Precision Physics Research (CAPP), Institute for Basic Science (IBS), Daejeon 34051, Republic of Korea
  • 2Department of Physics, Korea Advanced Institute of Science and Technology (KAIST), Daejeon 34141, Republic of Korea

  • *jwpc0120@ibs.re.kr
  • †swyoun@ibs.re.kr
  • ‡semertzidisy@gmail.com

Phys. Rev. D 108, L051101 – Published 1 September, 2023

DOI: https://doi.org/10.1103/PhysRevD.108.L051101

Abstract

The invisible axion is a hypothetical particle that arises from the Peccei-Quinn mechanism proposed to resolve the CP problem in quantum chromodynamics, and is considered one of the most favored candidates for cold dark matter. Dish antennas can provide a useful scheme for sensitive searches for dark matter axions. The conversion power through axion-photon couplings is proportional to the surface area of the metal plate, rather than the volume of the available magnetic field. To maximize the effect, we propose an advanced concept of haloscope that involves an array of horn antennas to increase the axion-induced photons and a reflector to focus them onto a photo sensor. Compared with other proposed schemes, this configuration can significantly improve the experimental sensitivity, especially in the terahertz region.

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References (46)

  1. R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38, 1440 (1977).
  2. S. Weinberg, Phys. Rev. Lett. 40, 223 (1978).
  3. F. Wilczek, Phys. Rev. Lett. 40, 279 (1978).
  4. J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. 120B, 127 (1983).
  5. L. F. Abbott and P. Sikivie, Phys. Lett. 120B, 133 (1983).
  6. M. Dine and W. Fischler, Phys. Lett. 120B, 137 (1983).
  7. J. E. Kim, Phys. Rev. Lett. 43, 103 (1979).
  8. M. A. Shifman, A. I. Vainshtein, and V. I. Zakharov, Nucl. Phys. B166, 493 (1980).
  9. A. P. Zhitnitsky, Yad. Fiz. 31, 497 (1980); Sov. J. Nucl. Phys. 31, 260 (1980).
  10. M. Dine, W. Fischler, and M. Srednicki, Phys. Lett. 104B, 199 (1981).
  11. S. DePanfilis, A. C. Melissinos, B. E. Moskowitz, J. T. Rogers, Y. K. Semertzidis, W. U. Wuensch, H. J. Halama, A. G. Prodell, W. B. Fowler, and F. A. Nezrick, Phys. Rev. Lett. 59, 839 (1987).
  12. C. Hagmann, P. Sikivie, N. S. Sullivan, and D. B. Tanner, Phys. Rev. D 42, 1297 (1990).
  13. S. J. Asztalos, Phys. Rev. Lett. 104, 041301 (2010); N. Du et al. (ADMX Collaboration), 120, 151301 (2018); C. Boutan et al. (ADMX Collaboration), 121, 261302 (2018); T. Braine et al. (ADMX Collaboration), 124, 101303 (2020); C. Bartram et al. (AMDX Collaboration), 127, 261803 (2021); Rev. Sci. Instrum. 94, 044703 (2023).
  14. S. Lee, S. Ahn, J. Choi, B.  R. Ko, and Y.  K. Semertzidis, Phys. Rev. Lett. 124, 101802 (2020); J. Jeong, S. Youn, S. Bae, J. Kim, T. Seong, J. E. Kim, and Y. K. Semertzidis, 125, 221302 (2020); O. Kwon et al., 126, 191802 (2021); Y. Lee, B. Yang, H. Yoon, M. Ahn, H. Park, B. Min, D. Kim, and J. Yoo, 128, 241805 (2022); A. K. Yi et al., 130, 071002 (2023); J. Kim et al., 130, 091602 (2023).
  15. L. Zhong et al. (HAYSTAC Collaboration), Phys. Rev. D 97, 092001 (2018); K. M. Backes et al. (HAYSTAC Collaboration), Nature (London) 590, 238 (2021); M. J. Jewell et al. (HAYSTAC Collaboration), Phys. Rev. D 107, 072007 (2023).
  16. C. M. Adair et al., Nat. Commun. 13, 6180 (2022).
  17. D. Alesini et al., Phys. Rev. D 99, 101101 (2019); 103, 102004 (2021); 106, 052007 (2022).
  18. A. Álvarez Melcón et al., J. High Energy Phys. 10 (2021) 075.
  19. B. T. McAllister, G. Flower, E. N. Ivanov, M. Goryachev, J. Bourhill, and M. E. Tobar, Phys. Dark Universe 18, 67 (2017); A. P. Quiskamp et al., Sci. Adv. 8, 27 (2022).
  20. T. Grenet et al., arXiv:2110.14406.
  21. H. Chang et al., Phys. Rev. Lett. 129, 111802 (2022).
  22. V. Anastassopoulos et al. (CAST Collaboration), Nat. Phys. 13, 584 (2017).
  23. P. Sikivie, Phys. Rev. D 32, 2988 (1985).
  24. D. Horns, J. Jaeckel, A. Lindner, A. Lobanov, J. Redondo, and A. Ringwald, J. Cosmol. Astropart. Phys. 04 (2013) 016; J. Jaeckel and J. Redondo, 11 (2013) 016; B. Döbrich et al., arXiv:1410.0200; J. Suzuki, T. Horie, Y. Inoue, and M. Minowa, J. Cosmol. Astropart. Phys. 09 (2015) 042; J. Jaeckel and S. Knirck, 01 (2016) 005;
  25. J. Liu et al. (BREAD Collaboration), Phys. Rev. Lett. 128, 131801 (2022).
  26. A. Caldwell, G. Dvali, B. Majorovits, A. Millar, G. Raffelt, J. Redondo, O. Reimann, F. Simon, and F. Steffen, Phys. Rev. Lett. 118, 091801 (2017).
  27. D. S. Kinion, Ph.D. thesis, UC Davis, 2001.
  28. J. Yang et al., Microwave Cavities and Detectors for Axion Research, Springer Proceedings in Physics (Springer, Cham, 2020).
  29. J. Jeong, S. Youn, S. Ahn, J. E. Kim, and Y. K. Semertzidis, Phys. Lett. B 777, 412 (2018).
  30. comsol multiphysics v. 5.2. www.comsol.com. COMSOL AB, Stockholm, Sweden.
  31. A. AlShirawi et al. (DMRadio Collaboration), arXiv:2302.14084.
  32. J. Jeong, Y. Kim, S. Bae, and S. Youn, J. Korean Phys. Soc. 83, 161 (2023).
  33. H. Eskandari, J. L. Albadalejo-Lijarcio, O. Zetterstrom, T. Tyc, and O. Quevedo-Teruel, Sci. Rep. 11, 14322 (2021).
  34. D. Wu et al., Proceedings of 2014 3rd APCAP (IEEE, 2014), p. 631, 10.1109/APCAP.2014.6992574.
  35. K. Konstantinidis et al., IEEE Trans. Terahertz Sci. Technol. 7, 572 (2017).
  36. Y. Amarasinghe, R. Mendis, R. Shrestha, H. Guerboukha, J. Taiber, Martin Koch, and D. M. Mittleman, Sci. Rep. 11, 5230 (2021).
  37. L. Wu et al., IEEE Antennas Wireless Propag. Lett. 19, 3 (2020).
  38. L. Wang et al., Proceedings of the 2016 2nd IEEE ICCC (IEEE, 2016), p. 1715, 10.1109/CompComm.2016.7924994.
  39. C. A. Fernandes, E. B. Lima, and J. R. Costa, IEEE Trans. Antennas Propag. 58, 3805 (2010); C. A. Fernandes, E. B. Lima, and J. R. Costa, Handbook of Antenna Technologies (Springer, Singapore, 2016).
  40. A. Suzuki et al., J. Low Temp. Phys. 193, 1048 (2018).
  41. M. L. Ridder, P. Khosropanah, R. A. Hijmering, T. Suzuki, M. P. Bruijn, H. F. C. Hoevers, J. R. Gao, and M. R. Zuiddam, J. Low Temp. Phys. 184, 60 (2016).
  42. D. J. Goldiea, A. V. Velichko, D. M. Glowacka, and S. Withington, J. Appl. Phys. 109, 084507 (2011).
  43. R. Kokkoniemi et al., Commun. Phys. 2, 124 (2019).
  44. G. H. Lee et al., Nature (London) 586, 42 (2020).
  45. F. Paolucci et al., J. Appl. Phys. 128, 194502 (2020).
  46. P. Hannan, IEEE Trans. Antennas Propag. 9, 140 (1961).

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