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

Adjusting optical cavity birefringence with wavelength tunable laser for axion searches

Hinata Takidera1, Hiroki Fujimoto1, Yuka Oshima1, Satoru Takano1,2, Kentaro Komori1,3, Tomohiro Fujita4,3,5, Ippei Obata5,6, Masaki Ando1,3, and Yuta Michimura3,5

Phys. Rev. D 112, 063048 – Published 24 September, 2025

DOI: https://doi.org/10.1103/5pw8-zxmc

Abstract

Axions have attracted attention as promising candidates for dark matter (DM). Although axions have been intensively searched for, they have not been observed yet. Recently, novel experiments to search for axion DM have been proposed that use optical cavities to amplify polarization rotation of laser light induced by the axion-photon interaction. One such experiment employs a ring cavity composed of four mirrors. However, its sensitivity to the axion-photon coupling gaγ in the low axion mass region is limited due to a reflection phase difference between s- and p-polarizations. In this paper, we propose a new method to improve the sensitivity using zero phase shift mirrors and a wavelength tunable laser. Moreover, the laser makes it easier to scan the high axion mass region by tuning the reflection phase difference between s- and p-polarizations. We experimentally confirmed that the phase difference generated upon reflection on a zero phase shift mirror satisfied the requirement of 8.6×10−3  deg, which corresponds to the half width at half maximum (HWHM) of the cavity for p-polarization with the mirror fixed on a folded cavity and a wavelength tunable laser.

View figure in article

Physics Subject Headings (PhySH)

Article Text

References (58)

  1. J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. 120B, 127 (1983).
  2. L. Abbott and P. Sikivie, Phys. Lett. 120B, 133 (1983).
  3. M. Dine and W. Fischler, Phys. Lett. 120B, 137 (1983).
  4. R. D. Peccei and H. R. Quinn, Phys. Rev. Lett. 38, 1440 (1977).
  5. P. Svrcek and E. Witten, J. High Energy Phys. 06 (2006) 051.
  6. A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. March-Russell, Phys. Rev. D 81, 123530 (2010).
  7. P. Sikivie, Phys. Rev. Lett. 51, 1415 (1983).
  8. S. Asztalos, E. Daw, H. Peng, L. J. Rosenberg, C. Hagmann, D. Kinion, W. Stoeffl, K. van Bibber, P. Sikivie, N. S. Sullivan, D. B. Tanner, F. Nezrick, M. S. Turner, D. M. Moltz, J. Powell et al., Phys. Rev. D 64, 092003 (2001).
  9. S. J. Asztalos, G. Carosi, C. Hagmann, D. Kinion, K. van Bibber, M. Hotz, L. J. Rosenberg, G. Rybka, J. Hoskins, J. Hwang, P. Sikivie, D. B. Tanner, R. Bradley, and J. Clarke, Phys. Rev. Lett. 104, 041301 (2010).
  10. N. Du, N. Force, R. Khatiwada, E. Lentz, R. Ottens, L. J. Rosenberg, G. Rybka, G. Carosi, N. Woollett, D. Bowring, A. S. Chou, A. Sonnenschein, W. Wester, C. Boutan, N. S. Oblath et al. (ADMX Collaboration), Phys. Rev. Lett. 120, 151301 (2018).
  11. T. Braine, R. Cervantes, N. Crisosto, N. Du, S. Kimes, L. J. Rosenberg, G. Rybka, J. Yang, D. Bowring, A. S. Chou, R. Khatiwada, A. Sonnenschein, W. Wester, G. Carosi, N. Woollett et al. (ADMX Collaboration), Phys. Rev. Lett. 124, 101303 (2020).
  12. C. Bartram, T. Braine, E. Burns, R. Cervantes, N. Crisosto, N. Du, H. Korandla, G. Leum, P. Mohapatra, T. Nitta, L. J. Rosenberg, G. Rybka, J. Yang, J. Clarke, I. Siddiqi et al. (ADMX Collaboration), Phys. Rev. Lett. 127, 261803 (2021).
  13. N. Crisosto, P. Sikivie, N. S. Sullivan, D. B. Tanner, J. Yang, and G. Rybka, Phys. Rev. Lett. 124, 241101 (2020).
  14. D. M. Lazarus, G. C. Smith, R. Cameron, A. C. Melissinos, G. Ruoso, Y. K. Semertzidis, and F. A. Nezrick, Phys. Rev. Lett. 69, 2333 (1992).
  15. S. Moriyama, M. Minowa, T. Namba, Y. Inoue, Y. Takasu, and A. Yamamoto, Phys. Lett. B 434, 147 (1998).
  16. Y. Inoue, Y. Akimoto, R. Ohta, T. Mizumoto, A. Yamamoto, and M. Minowa, Phys. Lett. B 668, 93 (2008).
  17. V. Anastassopoulos, S. Aune, K. Barth, A. Belov, H. Bräuninger, G. Cantatore, J. M. Carmona, J. F. Castel, S. A. Cetin, F. Christensen, J. I. Collar, T. Dafni, M. Davenport, T. A. Decker, A. Dermenev et al. (CAST Collaboration), Nat. Phys. 13, 584 (2017).
  18. K. Altenmüller, V. Anastassopoulos, S. Arguedas-Cuendis, S. Aune, J. Baier, K. Barth, H. Bräuninger, G. Cantatore, F. Caspers, J. F. Castel, S. A. Çetin, F. Christensen, C. Cogollos, T. Dafni, M. Davenport et al. (CAST Collaboration), Phys. Rev. Lett. 133, 221005 (2024).
  19. K. Van Bibber, N. R. Dagdeviren, S. E. Koonin, A. K. Kerman, and H. N. Nelson, Phys. Rev. Lett. 59, 759 (1987).
  20. A. A. Anselm, Phys. Rev. D 37, 2001 (1988).
  21. K. Ehret, M. Frede, S. Ghazaryan, M. Hildebrandt, E.-A. Knabbe, D. Kracht, A. Lindner, J. List, T. Meier, N. Meyer, D. Notz, J. Redondo, A. Ringwald, G. Wiedemann, and B. Willke, Nucl. Instrum. Methods Phys. Res., Sect. A 612, 83 (2009).
  22. K. Ehret, M. Frede, S. Ghazaryan, M. Hildebrandt, E.-A. Knabbe, D. Kracht, A. Lindner, J. List, T. Meier, N. Meyer, D. Notz, J. Redondo, A. Ringwald, G. Wiedemann, and B. Willke, Phys. Lett. B 689, 149 (2010).
  23. R. Ballou, G. Deferne, M. Finger, M. Finger, L. Flekova, J. Hosek, S. Kunc, K. Macuchova, K. A. Meissner, P. Pugnat, M. Schott, A. Siemko, M. Slunecka, M. Sulc, C. Weinsheimer et al. (OSQAR Collaboration), Phys. Rev. D 92, 092002 (2015).
  24. F. D. Valle, A. Ejlli, U. Gastaldi, G. Messineo, E. Milotti, R. Pengo, G. Ruoso, and G. Zavattini, Eur. Phys. J. C 76 (2016).
  25. Y. Kahn, B. R. Safdi, and J. Thaler, Phys. Rev. Lett. 117, 141801 (2016).
  26. C. P. Salemi, J. W. Foster, J. L. Ouellet, A. Gavin, K. M. W. Pappas, S. Cheng, K. A. Richardson, R. Henning, Y. Kahn, R. Nguyen, N. L. Rodd, B. R. Safdi, and L. Winslow, Phys. Rev. Lett. 127, 081801 (2021).
  27. A. V. Gramolin, D. Aybas, D. Johnson, J. Adam, and A. O. Sushkov, Nat. Phys. 17, 79 (2021).
  28. J. W. Brockway, E. D. Carlson, and G. G. Raffelt, Phys. Lett. B 383, 439 (1996).
  29. A. Payez, C. Evoli, T. Fischer, M. Giannotti, A. Mirizzi, and A. Ringwald, J. Cosmol. Astropart. Phys. 02 (2015) 006.
  30. M. D. Marsh, H. R. Russell, A. C. Fabian, B. R. McNamara, P. Nulsen, and C. S. Reynolds, J. Cosmol. Astropart. Phys. 12 (2017) 036.
  31. C. S. Reynolds, M. C. D. Marsh, H. R. Russell, A. C. Fabian, R. Smith, F. Tombesi, and S. Veilleux, Astrophys. J. 890, 59 (2020).
  32. J. Sisk-Reynés, J. H. Matthews, C. S. Reynolds, H. R. Russell, R. N. Smith, and M. C. D. Marsh, Mon. Not. R. Astron. Soc. 510, 1264 (2021).
  33. D. Noordhuis, A. Prabhu, S. J. Witte, A. Y. Chen, F. Cruz, and C. Weniger, Phys. Rev. Lett. 131, 111004 (2023).
  34. M. Escudero, C. K. Pooni, M. Fairbairn, D. Blas, X. Du, and D. J. E. Marsh, Phys. Rev. D 109, 043018 (2024).
  35. S. Goldstein, F. McCarthy, C. Mondino, J. C. Hill, J. Huang, and M. C. Johnson, Phys. Rev. Lett. 134, 081001 (2025).
  36. J. N. Benabou, C. Dessert, K. C. Patra, T. G. Brink, W. Zheng, A. V. Filippenko, and B. R. Safdi, arXiv:2504.12377.
  37. O. Ning and B. R. Safdi, Phys. Rev. Lett. 134, 171003 (2025).
  38. I. A. Sulai, S. Kalia, A. Arza, I. M. Bloch, E. C. Muñoz, C. Fabian, M. A. Fedderke, M. Forseth, B. Garthwaite, P. W. Graham, W. Griffith, E. Helgren, K. Hermanson, A. Interiano-Alvarado, B. Karki et al., Phys. Rev. D 108, 096026 (2023).
  39. A. Arza, M. A. Fedderke, P. W. Graham, D. F. Jackson Kimball, and S. Kalia, Phys. Rev. D 105, 095007 (2022).
  40. M. Friel, J. W. Gjerloev, S. Kalia, and A. Zamora, Phys. Rev. D 110, 115036 (2024).
  41. A. Nishizawa, A. Taruya, and Y. Himemoto, arXiv:2504.07559.
  42. W. DeRocco and A. Hook, Phys. Rev. D 98, 035021 (2018).
  43. K. Nagano, T. Fujita, Y. Michimura, and I. Obata, Phys. Rev. Lett. 123, 111301 (2019).
  44. K. Nagano, H. Nakatsuka, S. Morisaki, T. Fujita, Y. Michimura, and I. Obata, Phys. Rev. D 104, 062008 (2021).
  45. J. Heinze, A. Gill, A. Dmitriev, J. c. v. Smetana, T. Yan, V. Boyer, D. Martynov, and M. Evans, Phys. Rev. Lett. 132, 191002 (2024).
  46. H. Liu, B. D. Elwood, M. Evans, and J. Thaler, Phys. Rev. D 100, 023548 (2019).
  47. S. Pandey, E. D. Hall, and M. Evans, Phys. Rev. Lett. 133, 111003 (2024).
  48. I. Obata, T. Fujita, and Y. Michimura, Phys. Rev. Lett. 121, 161301 (2018).
  49. Y. Oshima, H. Fujimoto, J. Kume, S. Morisaki, K. Nagano, T. Fujita, I. Obata, A. Nishizawa, Y. Michimura, and M. Ando, Phys. Rev. D 108, 072005 (2023).
  50. D. Martynov and H. Miao, Phys. Rev. D 101, 095034 (2020).
  51. H. Fujimoto, Y. Oshima, M. Ando, T. Fujita, Y. Michimura, K. Nagano, and I. Obata, J. Phys. Conf. Ser. 2156, 012182 (2021).
  52. G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005).
  53. M. Weber and W. de Boer, Astron. Astrophys. 509, A25 (2010).
  54. R. Catena and P. Ullio, J. Cosmol. Astropart. Phys. 08 (2010) 004.
  55. D. Budker, P. W. Graham, M. Ledbetter, S. Rajendran, and A. O. Sushkov, Phys. Rev. X 4, 021030 (2014).
  56. P. Zorabedian and W. R. Trutna, Opt. Lett. 13, 826 (1988).
  57. X. Baillard, A. Gauguet, S. Bize, P. Lemonde, P. Laurent, A. Clairon, and P. Rosenbusch, Opt. Commun. 266, 609 (2006).
  58. R. W. P. Drever, J. L. Hall, F. V. Kowalski, J. Hough, G. M. Ford, A. J. Munley, and H. Ward, Appl. Phys. B 31, 97 (1983).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation