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  • Open Access

Universal bound on QCD axions from supernovae

Konstantin Springmann1,2,*, Michael Stadlbauer1,3,†, Stefan Stelzl4,‡, and Andreas Weiler1,§

  • *Contact author: konstantin.springmann@weizmann.ac.il
  • †Contact author: michael.stadlbauer@tum.de
  • ‡Contact author: stefan.stelzl@epfl.ch
  • §Contact author: andreas.weiler@tum.de

Phys. Rev. D 112, 075009 – Published 6 October, 2025

DOI: https://doi.org/10.1103/18t2-1w3b

Abstract

We identify a new production channel for quantum chromodynamics (QCD) axions in supernova environments that contributes to axion emissivity for all models solving the strong CP problem. This channel arises at tree-level from a shift-symmetry-breaking operator constructed at next-to-leading order in chiral perturbation theory. In scenarios where model-dependent derivative couplings to nucleons are absent, this sets the strongest model-independent constraint on the axion mass, improving on existing bounds by two orders of magnitude.

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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. F. Wilczek, Phys. Rev. Lett. 40, 279 (1978).
  4. S. Weinberg, Phys. Rev. Lett. 40, 223 (1978).
  5. G. Raffelt and D. Seckel, Phys. Rev. Lett. 60, 1793 (1988).
  6. J. R. Ellis and K. A. Olive, Phys. Lett. B 193, 525 (1987).
  7. M. S. Turner, Phys. Rev. Lett. 60, 1797 (1988).
  8. R. Mayle, J. R. Wilson, J. R. Ellis, K. A. Olive, D. N. Schramm, and G. Steigman, Phys. Lett. B 203, 188 (1988).
  9. R. Mayle, J. R. Wilson, J. R. Ellis, K. A. Olive, D. N. Schramm, and G. Steigman, Phys. Lett. B 219, 515 (1989).
  10. R. P. Brinkmann and M. S. Turner, Phys. Rev. D 38, 2338 (1988).
  11. G. Raffelt and D. Seckel, Phys. Rev. Lett. 67, 2605 (1991).
  12. G. Raffelt and D. Seckel, Phys. Rev. D 52, 1780 (1995).
  13. H.-T. Janka, W. Keil, G. Raffelt, and D. Seckel, Phys. Rev. Lett. 76, 2621 (1996).
  14. G. Raffelt and G. Sigl, Phys. Rev. D 60, 023001 (1999).
  15. A. Sedrakian and A. E. L. Dieperink, Phys. Rev. D 62, 083002 (2000).
  16. E. N. E. van Dalen, A. E. L. Dieperink, and J. A. Tjon, Phys. Rev. C 67, 065807 (2003).
  17. G. I. Lykasov, C. J. Pethick, and A. Schwenk, Phys. Rev. C 78, 045803 (2008).
  18. J. H. Chang, R. Essig, and S. D. McDermott, J. High Energy Phys. 09 (2018) 051.
  19. P. Carenza, T. Fischer, M. Giannotti, G. Guo, G. Martínez-Pinedo, and A. Mirizzi, J. Cosmol. Astropart. Phys. 10 (2019) 016; 05 (2020) E01.
  20. G. Guo and G. Martínez-Pinedo, Astrophys. J. 887, 58 (2019).
  21. D. R. Entem, R. Machleidt, and Y. Nosyk, Phys. Rev. C 96, 024004 (2017).
  22. A. Bartl, Neutrino interactions with supernova matter, Ph.D. thesis, Darmstadt, Technische Universität, 2016.
  23. M. Buschmann, C. Dessert, J. W. Foster, A. J. Long, and B. R. Safdi, Phys. Rev. Lett. 128, 091102 (2022).
  24. G. G. Raffelt, Stars as Laboratories for Fundamental Physics: The Astrophysics of Neutrinos, Axions, and Other Weakly Interacting Particles (1996).
  25. A. Caputo and G. Raffelt, in 1st Training School of the COST Action COSMIC WISPers (CA21106) (2024), arXiv:2401.13728.
  26. L. Di Luzio, F. Mescia, E. Nardi, P. Panci, and R. Ziegler, Phys. Rev. Lett. 120, 261803 (2018).
  27. M. Badziak and K. Harigaya, J. High Energy Phys. 06 (2023) 014.
  28. P. Carenza, B. Fore, M. Giannotti, A. Mirizzi, and S. Reddy, Phys. Rev. Lett. 126, 071102 (2021).
  29. K. Springmann, M. Stadlbauer, S. Stelzl, and A. Weiler, J. High Energy Phys. 02 (2025) 138.
  30. R. L. Workman et al. (Particle Data Group), Prog. Theor. Exp. Phys. 2022, 083C01 (2022).
  31. Y. Aoki et al. [Flavour Lattice Averaging Group (FLAG], Eur. Phys. J. C 82, 869 (2022).
  32. M. Hoferichter, J. Ruiz de Elvira, B. Kubis, and U.-G. Meißner, Phys. Rev. Lett. 115, 192301 (2015).
  33. V. Bernard, N. Kaiser, and U.-G. Meissner, Nucl. Phys. A615, 483 (1997).
  34. E. Epelbaum, U. G. Meissner, W. Gloeckle, and C. Elster, Phys. Rev. C 65, 044001 (2002).
  35. Note that this term has been extensively used in the literature as it can lead to the sourcing of light scalar fields in dense and large objects [36, 37, 38, 39, 40, 41, 42, 43].

  36. A. Hook and J. Huang, J. High Energy Phys. 06 (2018) 036.
  37. J. Zhang, Z. Lyu, J. Huang, M. C. Johnson, L. Sagunski, M. Sakellariadou, and H. Yang, Phys. Rev. Lett. 127, 161101 (2021).
  38. R. Balkin, J. Serra, K. Springmann, S. Stelzl, and A. Weiler, Phys. Rev. D 109, 095032 (2024).
  39. A. Gómez-Bañón, K. Bartnick, K. Springmann, and J. A. Pons, arXiv:2408.07740.
  40. R. Balkin, J. Serra, K. Springmann, and A. Weiler, J. High Energy Phys. 07 (2020) 221.
  41. R. Balkin, J. Serra, K. Springmann, S. Stelzl, and A. Weiler, SciPost Phys. 14, 071 (2023).
  42. R. Balkin, J. Serra, K. Springmann, S. Stelzl, and A. Weiler, J. High Energy Phys. 06 (2022) 023.
  43. R. Balkin, J. Serra, K. Springmann, S. Stelzl, and A. Weiler, J. High Energy Phys. 02 (2025) 141.
  44. G. Lucente, L. Mastrototaro, P. Carenza, L. Di Luzio, M. Giannotti, and A. Mirizzi, Phys. Rev. D 105, 123020 (2022).
  45. R. J. Crewther, P. Di Vecchia, G. Veneziano, and E. Witten, Phys. Lett. 88B, 123 (1979); Phys. Lett.91B, 487(E) (1980).
  46. M. Pospelov and A. Ritz, Phys. Rev. Lett. 83, 2526 (1999).
  47. A similar term is the dominant production channel for light pseudoscalars that couple to the quark mass matrix. On the other hand, if, unlike the QCD axion, a pseudoscalar field couples directly to a quark EDM, the nucleon EDM operator [44] is generated at tree level and thus dominant.

  48. S. Weinberg, Physica A (Amsterdam) 96, 327 (1979).
  49. S. Weinberg, Phys. Lett. B 251, 288 (1990).
  50. E. E. Jenkins and A. V. Manohar, Phys. Lett. B 255, 558 (1991).
  51. S. Weinberg, Nucl. Phys. B363, 3 (1991).
  52. S. Weinberg, Phys. Lett. B 295, 114 (1992).
  53. L. Di Luzio, V. Fiorentino, M. Giannotti, F. Mescia, and E. Nardi, Phys. Rev. D 111, 015018 (2025).
  54. Note that we are slightly deviating from the basis choice of, e.g., [55] in that we split χ− into its trace and its traceless part.

  55. N. Fettes, U.-G. Meissner, M. Mojzis, and S. Steininger, Ann. Phys. (Amsterdam) 283, 273 (2000); 288, 249(E) (2001).
  56. T. Vonk, F.-K. Guo, and U.-G. Meißner, J. High Energy Phys. 03 (2020) 138.
  57. Garching Core-Collapse Supernova Archive: https://wwwmpa.mpa-garching.mpg.de/ccsnarchive/.
  58. R. Bollig, W. DeRocco, P. W. Graham, and H.-T. Janka, Phys. Rev. Lett. 125, 051104 (2020); 126, 189901(E) (2021).
  59. M. Rampp and H. T. Janka, Astron. Astrophys. 396, 361 (2002).
  60. A. Marek, H. Dimmelmeier, H. T. Janka, E. Muller, and R. Buras, Astron. Astrophys. 445, 273 (2006).
  61. G. G. Raffelt, Lect. Notes Phys. 741, 51 (2008).
  62. C. O’Hare, cajohare/axionlimits: Axionlimits, GitHub, https://cajohare.github.io/AxionLimits/ (2020).
  63. I. Schulthess et al., Phys. Rev. Lett. 129, 191801 (2022).
  64. C. Abel et al., Phys. Rev. X 7, 041034 (2017).
  65. T. S. Roussy et al., Phys. Rev. Lett. 126, 171301 (2021).
  66. E. Madge, G. Perez, and Z. Meir, Phys. Rev. D 110, 015008 (2024).
  67. E. Fuchs, F. Kirk, E. Madge, C. Paranjape, E. Peik, G. Perez, W. Ratzinger, and J. Tiedau, Phys. Rev. X 15, 021055 (2025).
  68. S. Karanth et al. (JEDI Collaboration), Phys. Rev. X 13, 031004 (2023).
  69. X. Zhang, A. Banerjee, M. Leyser, G. Perez, S. Schiller, D. Budker, and D. Antypas, Phys. Rev. Lett. 130, 251002 (2023).
  70. P. J. Fox, N. Weiner, and H. Xiao, Phys. Rev. D 108, 095043 (2023).
  71. K. Blum, R. T. D’Agnolo, M. Lisanti, and B. R. Safdi, Phys. Lett. B 737, 30 (2014).
  72. V. M. Mehta, M. Demirtas, C. Long, D. J. E. Marsh, L. Mcallister, and M. J. Stott, arXiv:2011.08693.
  73. M. Baryakhtar, M. Galanis, R. Lasenby, and O. Simon, Phys. Rev. D 103, 095019 (2021).
  74. C. Ünal, F. Pacucci, and A. Loeb, J. Cosmol. Astropart. Phys. 05 (2021) 007.
  75. L. Di Luzio, B. Gavela, P. Quilez, and A. Ringwald, J. High Energy Phys. 05 (2021) 184.
  76. L. Caloni, M. Gerbino, M. Lattanzi, and L. Visinelli, J. Cosmol. Astropart. Phys. 09 (2022) 021.
  77. M. Badziak, K. Harigaya, M. Łukawski, and R. Ziegler, J. High Energy Phys. 09 (2024) 136.
  78. S. Hoof, D. J. E. Marsh, J. Sisk-Reynés, J. H. Matthews, and C. Reynolds, arXiv:2406.10337.

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