Reuse & Permissions

It is not necessary to obtain permission to reuse this article or its components as it is available under the terms of the Creative Commons Attribution 4.0 International license. This license permits unrestricted use, distribution, and reproduction in any medium, provided attribution to the author(s) and the published article's title, journal citation, and DOI are maintained. Please note that some figures may have been included with permission from other third parties. It is your responsibility to obtain the proper permission from the rights holder directly for these figures.

Export citation

Export citation

Choose format for download:

Download Citation
  • Open Access

Electromagnetic modeling and science reach of DMRadio-m3

A. AlShirawi1, V. Ankel1,2, C. Bartram2,3, J. Begin4, C. Bell1,2, J. N. Benabou5,6, L. Brouwer7, S. Chaudhuri4, H.-M. Cho2,3 et al. (DMRadio Collaboration)

H.-M. Cho2,3, J. Corbin1,2, W. Craddock3, S. Cuadra10, A. Droster9,*, J. Echevers9, J. W. Foster8,†, J. T. Fry10, P. W. Graham1, R. Henning11,12, K. D. Irwin1,2,3, F. Kadribasic1,2, Y. Kahn13, A. Keller9, R. Kolevatov4, S. Kuenstner1,2, A. Kunder1,2, N. Kurita3, A. F. Leder9,14, D. Li2,3, N. Otto4, J. L. Ouellet10, K. M. W. Pappas10, A. Phipps15, N. M. Rapidis1,2,‡, B. R. Safdi5,6, C. P. Salemi1,2,3, M. Simanovskaia1,2, J. Singh1,2, P. Stark1,2,3, E. C. van Assendelft1,2, K. van Bibber9, K. Wells1, J. Wiedemann4, L. Winslow10, W. J. Wisniewski3, D. Wright2,16, A. K. Yi2,3, and B. A. Young17 (DMRadio Collaboration)

  • *Contact author: adroster@berkeley.edu
  • †Contact author: jwfoster@mit.edu
  • ‡Contact author: rapidis@stanford.edu

Phys. Rev. D 112, 052001 – Published 2 September, 2025

DOI: https://doi.org/10.1103/bwgd-kxsb

Abstract

DMRadio-m3 is an experimental search for dark matter axions. It uses a solenoidal dc magnetic field to convert an axion dark-matter signal to an ac electromagnetic response in a coaxial copper pickup. The current induced by this axion signal is measured by dc SQUIDs. DMRadio-m3 is designed to be sensitive to Kim-Shifman-Vainshtein-Zakharov (KSVZ) and Dine-Fischler-Srednicki-Zhitnisky (DFSZ) QCD axion models in the 10–200 MHz (41  neV/c2–0.83  μeV/c2) range, and to axions with gaγγ=gaγγ,DFSZ(30  MHz)=1.87×10−17  GeV−1 over 5–30 MHz as an extended goal. In this work, we present the electromagnetic modeling of the response of the experiment to an axion signal over the full frequency range of DMRadio-m3, which extends from the low-frequency, lumped-element limit to a regime where the axion Compton wavelength is only a factor of 2 larger than the detector size. With these results, we determine the live time and sensitivity of the experiment. The primary science goal of sensitivity to DFSZ axions across 30–200 MHz can be achieved with a 3σ live scan time of 2.9 years.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (78)

  1. R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38, 1440 (1977).
  2. R. D. Peccei and H. R. Quinn, Phys. Rev. D 16, 1791 (1977).
  3. S. Weinberg, Phys. Rev. Lett. 40, 223 (1978).
  4. F. Wilczek, Phys. Rev. Lett. 40, 279 (1978).
  5. L. F. Abbott and P. Sikivie, Phys. Lett. 120B, 133 (1983).
  6. J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. 120B, 127 (1983).
  7. M. Dine and W. Fischler, Phys. Lett. 120B, 137 (1983).
  8. S. Borsanyi et al., Nature (London) 539, 69 (2016).
  9. M. Tegmark, A. Aguirre, M. J. Rees, and F. Wilczek, Phys. Rev. D 73, 023505 (2006).
  10. M. P. Hertzberg, M. Tegmark, and F. Wilczek, Phys. Rev. D 78, 083507 (2008).
  11. R. T. Co, F. D’Eramo, and L. J. Hall, Phys. Rev. D 94, 075001 (2016).
  12. P. W. Graham and A. Scherlis, Phys. Rev. D 98, 035017 (2018).
  13. F. Takahashi, W. Yin, and A. H. Guth, Phys. Rev. D 98, 015042 (2018).
  14. L. Di Luzio et al., Phys. Rep. 870, 1 (2020).
  15. M. B. Wise, H. Georgi, and S. L. Glashow, Phys. Rev. Lett. 47, 402 (1981).
  16. G. Ballesteros, J. Redondo, A. Ringwald, and C. Tamarit, J. Cosmol. Astropart. Phys. 08 (2017) 001.
  17. A. Ernst, A. Ringwald, and C. Tamarit, J. High Energy Phys. 02 (2018) 103.
  18. L. Di Luzio, A. Ringwald, and C. Tamarit, Phys. Rev. D 98, 095011 (2018).
  19. A. Ernst et al., Proc. Sci. CORFU2018 (2019) 054 [arXiv:1811.11860].
  20. P. Fileviez Pérez, C. Murgui, and A. D. Plascencia, J. High Energy Phys. 11 (2019) 093.
  21. P. Fileviez Pérez, C. Murgui, and A. D. Plascencia, J. High Energy Phys. 01 (2020) 091.
  22. P. Svrcek and E. Witten, J. High Energy Phys. 06 (2006) 051.
  23. M. B. Green and J. H. Schwarz, Phys. Lett. 149B, 117 (1984).
  24. J. P. Conlon, J. High Energy Phys. 05 (2006) 078.
  25. B. Acharya, K. Bobkov, and P. Kumar, J. High Energy Phys. 11 (2010) 105.
  26. A. Ringwald, J. Phys. Conf. Ser. 485, 012013 (2014).
  27. M. Cicoli, M. Goodsell, and A. Ringwald, J. High Energy Phys. 10 (2012) 146.
  28. J. Halverson, C. Long, B. Nelson, and G. Salinas, Phys. Rev. D 100, 106010 (2019).
  29. E. Witten, Phys. Lett. 149B, 351 (1984).
  30. M. Tegmark, A. Aguirre, M. J. Rees, and F. Wilczek, Phys. Rev. D 73, 023505 (2006).
  31. P. Sikivie, Phys. Rev. Lett. 51, 1415 (1983); 52, 695(E) (1984).
  32. P. F. de Salas and A. Widmark, Rep. Prog. Phys. 84, 104901 (2021).
  33. C. Bartram et al. (ADMX Collaboration), Phys. Rev. Lett. 127, 261803 (2021).
  34. K. M. Backes et al. (HAYSTAC Collaboration), Nature (London) 590, 238 (2021).
  35. A. K. Yi et al., Phys. Rev. Lett. 130, 071002 (2023).
  36. B. Cabrera and S. Thomas, Workshop Axions 2010 (University of Florida, Gainesville, 2008).
  37. P. Sikivie, N. Sullivan, and D. B. Tanner, Phys. Rev. Lett. 112, 131301 (2014).
  38. N. Crisosto, P. Sikivie, N. S. Sullivan, D. B. Tanner, J. Yang, and G. Rybka, Phys. Rev. Lett. 124, 241101 (2020).
  39. J. L. Ouellet et al., Phys. Rev. Lett. 122, 121802 (2019).
  40. J. L. Ouellet et al., Phys. Rev. D 99, 052012 (2019).
  41. C. P. Salemi et al., Phys. Rev. Lett. 127, 081801 (2021).
  42. Y. Kahn, B. R. Safdi, and J. Thaler, Phys. Rev. Lett. 117, 141801 (2016).
  43. A. V. Gramolin, D. Aybas, D. Johnson, J. Adam, and A. O. Sushkov, Nat. Phys. 17, 79 (2021).
  44. N. M. Rapidis (DMRadio Collaboration), SciPost Phys. Proc. 12, 036 (2023).
  45. A. Phipps et al., in Microwave Cavities and Detectors for Axion Research, edited by G. Carosi and G. Rybka (Springer International Publishing, Cham, 2020), pp. 139–145.
  46. J. Benabou, J. W. Foster, Y. Kahn, B. R. Safdi, and C. P. Salemi, Phys. Rev. D 108, 035009 (2023).
  47. D. Budker, P. W. Graham, M. Ledbetter, S. Rajendran, and A. O. Sushkov, Phys. Rev. X 4, 021030 (2014).
  48. Z. Bogorad, A. Hook, Y. Kahn, and Y. Soreq, Phys. Rev. Lett. 123, 021801 (2019).
  49. L. Brouwer et al. (DMRadio Collaboration), Phys. Rev. D 106, 103008 (2022).
  50. S. Chaudhuri et al., arXiv:1803.01627.
  51. M. Dine, W. Fischler, and M. Srednicki, Phys. Lett. 104B, 199 (1981).
  52. A. Zhitnitsky, Sov. J. Nucl. Phys. 31, 260 (1980).
  53. J. E. Kim, Phys. Rev. Lett. 43, 103 (1979).
  54. M. A. Shifman, A. I. Vainshtein, and V. I. Zakharov, Nucl. Phys. B166, 493 (1980).
  55. D. M. Pozar, Microwave Engineering (John Wiley & Sons, New York, 2011).
  56. comsol AB and comsol multiphysics.
  57. T. Braine et al. (ADMX Collaboration), Phys. Rev. Lett. 124, 101303 (2020).
  58. B. M. Brubaker et al., Phys. Rev. Lett. 118, 061302 (2017).
  59. N. M. Rapidis, S. M. Lewis, and K. A. van Bibber, Rev. Sci. Instrum. 90, 024706 (2019).
  60. J. Herzog-Arbeitman, M. Lisanti, P. Madau, and L. Necib, Phys. Rev. Lett. 120, 041102 (2018).
  61. L. Brouwer et al. (DMRadio Collaboration), Phys. Rev. D 106, 112003 (2022).
  62. V. Ankel et al., arXiv:2504.20398.
  63. A. AlShirawi et al., 10.5281/zenodo.15149989 (2025).
  64. C. Bartram et al. (ADMX Collaboration), Phys. Rev. D 103, 032002 (2021).
  65. ADMX Collaboration (private communication).
  66. D. A. Palken et al., Phys. Rev. D 101, 123011 (2020).
  67. J. D. Jackson, Classical Electrodynamics, 3rd ed. (Wiley, New York, NY, 1999).
  68. A. Pippard, Adv. Electron. Electron Phys. 6, 1 (1954).
  69. A. Cahill et al., in 7th International Particle Accelerator Conference (JACoW, Geneva, Switzerland, 2016).
  70. H. Peng et al., Nucl. Instrum. Methods Phys. Res., Sect. A 444, 569 (2000).
  71. R. Finger and A. Kerr, Int. J. Infrared Millimeter Waves 29, 924 (2008).
  72. M. Simanovskaia, A. Droster, H. Jackson, I. Urdinaran, and K. van Bibber, Rev. Sci. Instrum. 92, 033305 (2021).
  73. H. Yoon, M. Ahn, B. Yang, Y. Lee, D. Kim, H. Park, B. Min, and J. Yoo, Phys. Rev. D 106, 092007 (2022).
  74. M. Benz, J. Appl. Phys. 40, 2003 (1969).
  75. F. R. Fickett, eConf C 720919, 539 (1972).
  76. M. Kohler, Ann. Phys. (Berlin) 424, 211 (1938).
  77. J. T. Rogers, S. De Panfilis, A. C. Melissinos, B. E. Moskowitz, Y. K. Semertzidis, W. U. Wuensch, H. J. Halama, A. G. Prodell, W. B. Fowler, and F. A. Nezrick, Appl. Phys. Lett. 52, 2266 (1988).
  78. S. Ahn et al., J. Instrum. 12, P10023 (2017).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation