[1] | Gould R and Schréder G 1966 Phys. Rev. Lett. 16 252 | Opacity of the Universe to High-Energy Photons
[2] | Fazio G G and Stecker F W 1970 Nature 226 135 | Predicted High Energy Break in the Isotropic Gamma Ray Spectrum: a Test of Cosmological Origin
[3] | Protheroe R J and Meyer H 2000 Phys. Lett. B 493 1 | An infrared background-TeV gamma-ray crisis?
[4] | Breit G and Wheeler J A 1934 Phys. Rev. 46 1087 | Collision of Two Light Quanta
[5] | Zyla P A et al. (Particle Data Group) 2020 Prog. Theor. Exp. Phys. 2020 083C01 |
[6] | Cao Z, Aharonian F A, An Q et al. (LHAASO Collaboration) 2021 Nature 594 33 | Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources
[7] | Cao Z, Aharonian F A, An Q et al. (LHAASO Collaboration) 2021 Science 373 425 | Peta–electron volt gamma-ray emission from the Crab Nebula
[8] | Li C Y Y and Ma B Q 2021 Phys. Rev. D 104 063012 | Ultrahigh-energy photons from LHAASO as probes of Lorentz symmetry violations
[9] | Li H and Ma B Q 2021 J. High Energy Astrophys. 32 1 |
[10] | Li C and Ma B Q 2021 Sci. Bull. 66 2254 | LHAASO discovery of highest-energy photons towards new physics
[11] | He P and Ma B Q 2022 Universe 8 323 | Lorentz Symmetry Violation of Cosmic Photons
[12] | Coriano C and Irges N 2007 Phys. Lett. B 651 298 | Windows over a new low energy axion
[13] | Chang S, Tazawa S, and Yamaguchi M 2000 Phys. Rev. D 61 084005 | Axion model in extra dimensions with TeV scale gravity
[14] | Svrcek P and Witten E 2006 J. High Energy Phys. 2006(06) 051 | Axions in string theory
[15] | Arvanitaki A, Dimopoulos S, Dubovsky S, Kaloper N, and March-Russell J 2010 Phys. Rev. D 81 123530 | String axiverse
[16] | Peccei R D and Quinn H R 1977 Phys. Rev. Lett. 38 1440 | Conservation in the Presence of Pseudoparticles
[17] | Sikivie P 1983 Phys. Rev. Lett. 51 1415 | Experimental Tests of the "Invisible" Axion
[18] | Masso E and Toldra R 1995 Phys. Rev. D 52 1755 | Light spinless particle coupled to photons
[19] | De Angelis A, Roncadelli M, and Mansutti O 2007 Phys. Rev. D 76 121301 | Evidence for a new light spin-zero boson from cosmological gamma-ray propagation?
[20] | De Angelis A, Mansutti O, Persic M, and Roncadelli M 2009 Mon. Not. Roy. Astron. Soc. 394 L21 | Photon propagation and the very high energy γ-ray spectra of blazars: how transparent is the Universe?
[21] | Sanchez-Conde M A, Paneque D, Bloom E, Prada F, and Dominguez A 2009 Phys. Rev. D 79 123511 | Hints of the existence of axionlike particles from the gamma-ray spectra of cosmological sources
[22] | Mirizzi A and Montanino D 2009 J. Cosmol. Astropart. Phys. 2009(12) 004 |
[23] | Dominguez A, Sanchez-Conde M A, and Prada F 2011 J. Cosmol. Astropart. Phys. 2011(11) 020 |
[24] | Simet M, Hooper D, and Serpico P D 2008 Phys. Rev. D 77 063001 | Milky Way as a kiloparsec-scale axionscope
[25] | Galanti G, Tavecchio F, Roncadelli M, and Evoli C 2019 Mon. Not. Roy. Astron. Soc. 487 123 | Blazar VHE spectral alterations induced by photon–ALP oscillations
[26] | Long G B, Chen S, Xu S, and Zhang H H 2021 Phys. Rev. D 104 083014 | Probing ALPs with future LHAASO observations of AGN -ray spectra
[27] | Liang Y F, Zhang X F, Cheng J G, Zeng H D, Fan Y Z, and Liang E W 2021 J. Cosmol. Astropart. Phys. 2021(11) 030 |
[28] | Li H and Ma B Q 2022 arXiv:2210.05563 [astro-ph.HE] | Searching Lorentz invariance violation from cosmic photon attenuation
[29] | Li H and Ma B Q 2022 arXiv:2210.06338 [astro-ph.HE] | Lorentz invariance violation induced threshold anomaly versus very-high energy cosmic photon emission from GRB 221009A
[30] | Brevik I, Chaichian M, and Oksanen M 2021 Eur. Phys. J. C 81 926 | Dispersion of light traveling through the interstellar space, induced and intrinsic Lorentz invariance violation
[31] | Zhu J and Ma B Q 2022 arXiv:2210.11376 [astro-ph.HE] | Light speed variation from GRB 221009A
[32] | Huang Y, Hu S, and Chen S et al. 2022 GCN Circular No. 32677 | Abstract EP54: Ideal Cardiovascular Health Metrics: Are They Just Cardiovascular Protective Factors?
[33] | Galanti G, Roncadelli M, and Tavecchio F 2022 arXiv:2210.05659 [astro-ph.HE] | Explanation of the very-high-energy emission from GRB221009A
[34] | Baktash A, Horns D, and Meyer M 2022 arXiv:2210.07172 [astro-ph.HE] | Interpretation of multi-TeV photons from GRB221009A
[35] | Troitsky S V 2022 JETP Lett. 116 745 |
[36] | Nakagawa S, Takahashi F, Yamada M, and Yin W 2022 arXiv:2210.10022 [hep-ph] | Axion dark matter from first-order phase transition, and very high energy photons from GRB 221009A
[37] | Krasnikov S V 1996 Phys. Rev. Lett. 76 2633 | New Astrophysical Constraints on the Light-Pseudoscalar–Photon Coupling
[38] | Fairbairn M, Rashba T, and Troitsky S 2011 Phys. Rev. D 84 125019 | Photon-axion mixing and ultra-high energy cosmic rays from BL Lac type objects: Shining light through the Universe
[39] | Raffelt G and Stodolsky L 1988 Phys. Rev. D 37 1237 | Mixing of the photon with low-mass particles
[40] | De Miguel J and Otani C 2022 Phys. Rev. D 106 L041302 | Axion-photon multimessenger astronomy with giant flares
[41] | O'Hare C 2022 Axion Limits https://cajohare.github.io/ AxionLimits/docs/ap.html |
[42] | Dzhappuev D D, Afashokov Y Z, Dzaparova I M, Dzhatdoev T A, Gorbacheva E A et al. 2022 Astronomer's Telegram No. 15669 |