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

Novel Constraints on Axions Produced in Pulsar Polar-Cap Cascades

Dion Noordhuis1,*,†, Anirudh Prabhu2,3,†, Samuel J. Witte1,†, Alexander Y. Chen4, Fábio Cruz5,6, and Christoph Weniger1

  • 1GRAPPA Institute, Institute for Theoretical Physics Amsterdam and Delta Institute for Theoretical Physics, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, Netherlands
  • 2Princeton Center for Theoretical Science, Princeton University, Princeton, New Jersey 08544, USA
  • 3Stanford Institute for Theoretical Physics, Stanford University, Stanford, California 94305, USA
  • 4Physics Department and McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri 63130, USA
  • 5GoLP/Instituto de Plasmas e Fusão Nuclear, Instituto Superior Técnico, Universidade de Lisboa, 1049-001 Lisboa, Portugal
  • 6Inductiva Research Labs, Rua da Prata 80, 1100-420 Lisboa, Portugal

  • *Corresponding author: d.noordhuis@uva.nl
  • †These authors contributed equally to this work.

Phys. Rev. Lett. 131, 111004 – Published 15 September, 2023

DOI: https://doi.org/10.1103/PhysRevLett.131.111004

Abstract

Axions can be copiously produced in localized regions of neutron star magnetospheres where the ambient plasma is unable to efficiently screen the induced electric field. As these axions stream away from the neutron star they can resonantly transition into photons, generating a large broadband contribution to the neutron star’s intrinsic radio flux. In this Letter, we develop a comprehensive end-to-end framework to model this process from the initial production of axions to the final detection of radio photons, and derive constraints on the axion-photon coupling, gaγγ, using observations of 27 nearby pulsars. We study the modeling uncertainty in the sourced axion spectrum by comparing predictions from 2.5 dimensional particle-in-cell simulations with those derived using a semianalytic model; these results show remarkable agreement, leading to constraints on the axion-photon coupling that typically differ by a factor of no more than ∼2. The limits presented here are the strongest to date for axion masses 10−8  eV≲ma≲10−5  eV, and crucially do not rely on the assumption that axions are dark matter.

View figure in article

Physics Subject Headings (PhySH)

Article Text

Supplemental Material

References (125)

  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. J. Preskill, M. B. Wise, and F. Wilczek, Phys. Lett. 120B, 127 (1983).
  6. L. Abbott and P. Sikivie, Phys. Lett. 120B, 133 (1983).
  7. M. Dine and W. Fischler, Phys. Lett. 120B, 137 (1983).
  8. N. Aghanim, Y. Akrami, M. Ashdown, J. Aumont, C. Baccigalupi, M. Ballardini, A. Banday, R. Barreiro, N. Bartolo et al. (P. Collaboration), Astron. Astrophys. 641, A6 (2020).
  9. P. Svrcek and E. Witten, J. High Energy Phys. 06 (2006) 051.
  10. A. Arvanitaki, S. Dimopoulos, S. Dubovsky, N. Kaloper, and J. March-Russell, Phys. Rev. D 81, 123530 (2010).
  11. P. Sikivie, Phys. Rev. Lett. 51, 1415 (1983).
  12. 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).
  13. C. Hagmann, P. Sikivie, N. S. Sullivan, and D. B. Tanner, Phys. Rev. D 42, 1297 (1990).
  14. C. Hagmann et al. (ADMX Collaboration), Phys. Rev. Lett. 80, 2043 (1998).
  15. S. J. Asztalos et al. (ADMX Collaboration), Phys. Rev. D 64, 092003 (2001).
  16. S. J. Asztalos et al. (ADMX Collaboration), Phys. Rev. Lett. 104, 041301 (2010).
  17. N. Du et al. (ADMX Collaboration), Phys. Rev. Lett. 120, 151301 (2018).
  18. T. Braine et al. (ADMX Collaboration), Phys. Rev. Lett. 124, 101303 (2020).
  19. R. Bradley, J. Clarke, D. Kinion, L. J. Rosenberg, K. van Bibber, S. Matsuki, M. Mück, and P. Sikivie, Rev. Mod. Phys. 75, 777 (2003).
  20. S. J. Asztalos et al., Phys. Rev. D 69, 011101(R) (2004).
  21. T. M. Shokair et al., Int. J. Mod. Phys. A 29, 1443004 (2014).
  22. B. M. Brubaker et al. (HAYSTAC Collaboration), Phys. Rev. Lett. 118, 061302 (2017).
  23. L. Zhong et al. (HAYSTAC Collaboration), Phys. Rev. D 97, 092001 (2018).
  24. K. M. Backes et al. (HAYSTAC Collaboration), Nature (London) 590, 238 (2021).
  25. B. T. McAllister, G. Flower, E. N. Ivanov, M. Goryachev, J. Bourhill, and M. E. Tobar, Phys. Dark Universe 18, 67 (2017).
  26. N. Crescini et al. (QUAX Collaboration), Phys. Rev. Lett. 124, 171801 (2020).
  27. J. Choi, S. Ahn, B. Ko, S. Lee, and Y. Semertzidis, Nucl. Instrum. Methods Phys. Res., Sect. A 1013, 165667 (2021).
  28. A. Caldwell, G. Dvali, B. Majorovits, A. Millar, G. Raffelt, J. Redondo, O. Reimann, F. Simon, and F. Steffen (MADMAX Working Group), Phys. Rev. Lett. 118, 091801 (2017).
  29. B. Majorovits et al. (MADMAX interest Group), J. Phys. Conf. Ser. 1342, 012098 (2020).
  30. M. Baryakhtar, J. Huang, and R. Lasenby, Phys. Rev. D 98, 035006 (2018).
  31. E. Arik et al. (CAST Collaboration), J. Cosmol. Astropart. Phys. 02 (2009) 008.
  32. M. Arik et al. (CAST Collaboration), Phys. Rev. D 92, 021101 (2015).
  33. V. Anastassopoulos et al. (CAST Collaboration), Nat. Phys. 13, 584 (2017).
  34. K. Van Bibber, N. R. Dagdeviren, S. E. Koonin, A. K. Kerman, and H. N. Nelson, Phys. Rev. Lett. 59, 759 (1987).
  35. R. Rabadán, A. Ringwald, and K. Sigurdson, Phys. Rev. Lett. 96, 110407 (2006).
  36. S. L. Adler, J. Gamboa, F. Méndez, and J. López-Sarrión, Ann. Phys. (Amsterdam) 323, 2851 (2008).
  37. D. Wouters and P. Brun, Astrophys. J. 772, 44 (2013).
  38. A. Abramowski et al. (H.E.S.S. Collaboration), Phys. Rev. D 88, 102003 (2013).
  39. A. Payez et al., J. Cosmol. Astropart. Phys. 02 (2015) 006.
  40. M. Ajello et al. (Fermi-LAT Collaboration), Phys. Rev. Lett. 116, 161101 (2016).
  41. M. Meyer, M. Giannotti, A. Mirizzi, J. Conrad, and M. A. Sánchez-Conde, Phys. Rev. Lett. 118, 011103 (2017).
  42. M. C. D. Marsh, H. R. Russell, A. C. Fabian, B. P. McNamara, P. Nulsen, and C. S. Reynolds, J. Cosmol. Astropart. Phys. 12 (2017) 036.
  43. 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).
  44. M. Xiao, K. M. Perez, M. Giannotti, O. Straniero, A. Mirizzi, B. W. Grefenstette, B. M. Roach, and M. Nynka, Phys. Rev. Lett. 126, 031101 (2021).
  45. H.-J. Li, J.-G. Guo, X.-J. Bi, S.-J. Lin, and P.-F. Yin, Phys. Rev. D 103, 083003 (2021).
  46. C. Dessert, J. W. Foster, and B. R. Safdi, Phys. Rev. Lett. 125, 261102 (2020).
  47. M. Meyer and T. Petrushevska, Phys. Rev. Lett. 124, 231101 (2020); 125, 119901(E) (2020).
  48. F. Calore, P. Carenza, C. Eckner, T. Fischer, M. Giannotti, J. Jaeckel, K. Kotake, T. Kuroda, A. Mirizzi, and F. Sivo, Phys. Rev. D 105, 063028 (2022).
  49. J. S. 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).
  50. J. W. Foster, Y. Kahn, O. Macias, Z. Sun, R. P. Eatough, V. I. Kondratiev, W. M. Peters, C. Weniger, and B. R. Safdi, Phys. Rev. Lett. 125, 171301 (2020).
  51. R. A. Battye, J. Darling, J. McDonald, and S. Srinivasan, Phys. Rev. D 105, L021305 (2022).
  52. J. W. Foster, S. J. Witte, M. Lawson, T. Linden, V. Gajjar, C. Weniger, and B. R. Safdi, Phys. Rev. Lett. 129, 251102 (2022).
  53. A. Caputo, C. P. n. Garay, and S. J. Witte, Phys. Rev. D 98, 083024 (2018); 99, 089901(E) (2019).
  54. A. Caputo, M. Regis, M. Taoso, and S. J. Witte, J. Cosmol. Astropart. Phys. 03 (2019) 027.
  55. O. Ghosh, J. Salvado, and J. Miralda-Escudé, arXiv:2008.02729.
  56. M. A. Buen-Abad, J. J. Fan, and C. Sun, Phys. Rev. D 105, 075006 (2022).
  57. Y. Sun, K. Schutz, A. Nambrath, C. Leung, and K. Masui, Phys. Rev. D 105, 063007 (2022).
  58. M. S. Pshirkov and S. B. Popov, J. Exp. Theor. Phys. 108, 384 (2009).
  59. F. P. Huang, K. Kadota, T. Sekiguchi, and H. Tashiro, Phys. Rev. D 97, 123001 (2018).
  60. A. Hook, Y. Kahn, B. R. Safdi, and Z. Sun, Phys. Rev. Lett. 121, 241102 (2018).
  61. B. R. Safdi, Z. Sun, and A. Y. Chen, Phys. Rev. D 99, 123021 (2019).
  62. R. A. Battye, B. Garbrecht, J. I. McDonald, F. Pace, and S. Srinivasan, Phys. Rev. D 102, 023504 (2020).
  63. M. Leroy, M. Chianese, T. D. P. Edwards, and C. Weniger, Phys. Rev. D 101, 123003 (2020).
  64. J. H. Buckley, P. B. Dev, F. Ferrer, and F. P. Huang, Phys. Rev. D 103, 043015 (2021).
  65. S. J. Witte, D. Noordhuis, T. D. P. Edwards, and C. Weniger, Phys. Rev. D 104, 103030 (2021).
  66. R. A. Battye, B. Garbrecht, J. McDonald, and S. Srinivasan, J. High Energy Phys. 09 (2021) 105.
  67. A. Prabhu, Phys. Rev. D 104, 055038 (2021).
  68. B. Garbrecht and J. I. McDonald, J. Cosmol. Astropart. Phys. 07 (2018) 044.
  69. F. Cruz, T. Grismayer, A. Y. Chen, A. Spitkovsky, and L. O. Silva, Astrophys. J. Lett. 919, L4 (2021).
  70. P. Goldreich and W. H. Julian, Astrophys. J. 157, 869 (1969).
  71. J. Chiang and R. W. Romani, Astrophys. J. 400, 629 (1992).
  72. M. A. Ruderman and P. G. Sutherland, Astrophys. J. 196, 51 (1975).
  73. J. Arons, Astrophys. J. 266, 215 (1983).
  74. K. S. Cheng, C. Ho, and M. Ruderman, Astrophys. J. 300, 500 (1986).
  75. G. Brambilla, C. Kalapotharakos, A. N. Timokhin, A. K. Harding, and D. Kazanas, Astrophys. J. 858, 81 (2018).
  76. R. Hu and A. M. Beloborodov, Astrophys. J. 939, 42 (2022).
  77. A. N. Timokhin and J. Arons, Mon. Not. R. Astron. Soc. 429, 20 (2013).
  78. A. Philippov, A. Timokhin, and A. Spitkovsky, Phys. Rev. Lett. 124, 245101 (2020).
  79. A. Levinson, D. Melrose, A. Judge, and Q. Luo, Astrophys. J. 631, 456 (2005).
  80. A. N. Timokhin and A. K. Harding, Astrophys. J. 810, 144 (2015).
  81. F. Cruz, T. Grismayer, and L. O. Silva, Astrophys. J. 908, 149 (2021).
  82. E. A. Tolman, A. A. Philippov, and A. N. Timokhin, Astrophys. J. Lett. 933, L37 (2022).
  83. M. E. Peskin, An Introduction to Quantum Field Theory (CRC Press, Boca Raton, 2018).
  84. See Supplemental Material at http://link.aps.org/supplemental/10.1103/PhysRevLett.131.111004 for further discussion pertaining to vacuum gap modeling, which includes Refs. [85,86]; radio flux computation, which includes Ref. [87]; properties of used pulsars, which includes Refs. [88–98]; our profile likelihood analysis, which includes Refs. [99–101]; and uncertainties, which includes Refs. [102–108].
  85. R. Fonseca, S. Martins, L. Silva, J. Tonge, F. Tsung, and W. Mori, Plasma Phys. Controlled Fusion 50, 124034 (2008).
  86. A. N. Timokhin and A. K. Harding, Astrophys. J. 871, 12 (2019).
  87. P. Carenza and M. C. D. Marsh, J. Cosmol. Astropart. Phys. 04 (2023) 021.
  88. L. Bondonneau, J.-M. Grießmeier, G. Theureau, A. Bilous, V. Kondratiev, M. Serylak, M. Keith, and A. Lyne, Astron. Astrophys. 635, A76 (2020).
  89. D. Lorimer, J. Yates, A. Lyne, and D. Gould, Mon. Not. R. Astron. Soc. 273, 411 (1995).
  90. R.-S. Zhao et al., Astrophys. J. 845, 156 (2017).
  91. J. M. Rankin, Astrophys. J. 405, 285 (1993).
  92. Y. Gupta and R. Gangadhara, Astrophys. J. 584, 418 (2003).
  93. J. Rankin, Mon. Not. R. Astron. Soc. 514, 3202 (2022).
  94. J. P. W. Verbiest, J. M. Weisberg, A. A. Chael, K. J. Lee, and D. R. Lorimer, Astrophys. J. 755, 39 (2012).
  95. J. Yao, R. Manchester, and N. Wang, Astrophys. J. 835, 29 (2017).
  96. S. Brownsberger and R. W. Romani, Astrophys. J. 784, 154 (2014).
  97. D. C. Price, C. Flynn, and A. Deller, Pub. Astron. Soc. Aust. 38, e038 (2021).
  98. F. Jankowski, W. van Straten, E. F. Keane, M. Bailes, E. D. Barr, S. Johnston, and M. Kerr, Mon. Not. R. Astron. Soc. 473, 4436 (2018).
  99. S. S. Wilks, Ann. Math. Stat. 9, 60 (1938).
  100. A. Wald, Trans. Am. Math. Soc. 54, 426 (1943).
  101. G. Cowan, K. Cranmer, E. Gross, and O. Vitells, Eur. Phys. J. C 71, 1554 (2011); 73, 2501(E) (2013).
  102. J. Li, A. Spitkovsky, and A. Tchekhovskoy, Astrophys. J. Lett. 746, L24 (2012).
  103. A. W. Steiner, S. Gandolfi, F. J. Fattoyev, and W. G. Newton, Phys. Rev. C 91, 015804 (2015).
  104. J. M. Lattimer, Annu. Rev. Nucl. Part. Sci. 71, 433 (2021).
  105. V. Radhakrishnan and D. Cooke, Astrophys. Lett. 3 225 (1969).
  106. A. M. Beloborodov, Astrophys. J. 683, L41 (2008).
  107. M. A. Belyaev and K. Parfrey, Astrophys. J. 830, 119 (2016).
  108. A. Szary, G. I. Melikidze, and J. Gil, Mon. Not. R. Astron. Soc. 447, 2295 (2015).
  109. J. D. Jackson, Classical Electrodynamics (Wiley, New York, 1998).
  110. A. Levinson, D. Melrose, A. Judge, and Q.-h. Luo, Astrophys. J. 631, 456 (2005).
  111. A. N. Timokhin, Mon. Not. R. Astron. Soc. 408, 2092 (2010).
  112. A. Levinson and B. Cerutti, Astron. Astrophys. 616, A184 (2018).
  113. A. Y. Chen and Y. Yuan, Astrophys. J. 895, 121 (2020).
  114. S. Kisaka, A. Levinson, and K. Toma, Astrophys. J. 902, 80 (2020).
  115. F. Cruz, T. Grismayer, and L. O. Silva, Astrophys. J. 908, 149 (2021).
  116. F. Cruz, T. Grismayer, S. Iteanu, P. Tortone, and L. O. Silva, Phys. Plasmas 29, 052902 (2022).
  117. T. Erber, Rev. Mod. Phys. 38, 626 (1966).
  118. R. A. Fonseca, L. O. Silva, F. S. Tsung, V. K. Decyk, W. Lu, C. Ren, W. B. Mori, S. Deng, S. Lee, T. Katsouleas et al., in Proceedings of the International Conference on Computational Science (Springer, New York, 2002), pp. 342–351.
  119. https://www.youtube.com/watch?v=wHSw5kp7Ik4online.
  120. D. Noordhuis, A. Prabhu, C. Weniger, and S. J. Witte, arXiv:2307.11811v1.
  121. A. J. Millar, S. Baum, M. Lawson, and M. C. D. Marsh, J. Cosmol. Astropart. Phys. 11 (2021) 013.
  122. A. Álvarez-Melcón et al., J. High Energy Phys. 10 (2021) 075.
  123. C. Dessert, A. J. Long, and B. R. Safdi, Phys. Rev. Lett. 128, 071102 (2022).
  124. C. Dessert, D. Dunsky, and B. R. Safdi, Phys. Rev. D 105, 103034 (2022).
  125. C. O’Hare, cajohare/axionlimits: Axionlimits, 10.5281/zenodo.3932430 (2020).

Outline

Information

Sign In to Your Journals Account

Filter

Filter

Article Lookup

Enter a citation