\begin{document}$ \gamma $\end{document}-ray sources with significant magnetic field strengths provide an ideal environment to investigate this phenomenon. Ton 599, a flat spectrum radio quasar with a magnetic field strength on the order of Gauss in its emission region, presents a promising opportunity for studying ALP-photon oscillations. In this study, we analyze the effects of ALP-photon oscillations on the γ-ray spectrum of Ton 599, as observed by Fermi-LAT. Our investigation considers the potential influences of the broad-line region and dusty torus on the \begin{document}$ \gamma $\end{document}-ray spectrum of Ton 599. We set the constraints on the ALP parameters at a 95% confidence level and show that the constraints on \begin{document}$ g_{a\gamma} $\end{document} can reach approximately \begin{document}$ 2 \times 10^{-12}\; \text{GeV}^{-1} $\end{document} for \begin{document}$ m_a \sim 10^{-9}\; \text{eV} $\end{document}."> Exploring axion-like particle from observation of FSRQ Ton 599 by Fermi-LAT -
  • [1]

    P. Svrcek and E. Witten, JHEP06, 051 (2006), arXiv: hepth/0605206

  • [2]

    A. Arvanitaki, S. Dimopoulos, S. Dubovskyet al., Phys. Rev. D81, 123530 (2010), arXiv: 0905.4720[hep-th]

  • [3]

    D. J. E. Marsh, Phys. Rept.643, 1 (2016), arXiv: 1510.07633[astro-ph.CO]

  • [4]

    R. D. Peccei and H. R. Quinn, Phys. Rev. Lett.38, 1440 (1977)

  • [5]

    R. D. Peccei and H. R. Quinn, Phys. Rev. D16, 1791 (1977)

  • [6]

    S. Weinberg, Phys. Rev. Lett.40, 223 (1978)

  • [7]

    F. Wilczek, Phys. Rev. Lett.40, 279 (1978)

  • [8]

    G. Raffelt and L. Stodolsky, Phys. Rev. D37, 1237 (1988)

  • [9]

    A. De Angelis, O. Mansutti, and M. Roncadelli, Phys. Lett. B659, 847 (2008), arXiv: 0707.2695[astro-ph]

  • [10]

    A. De Angelis, M. Roncadelli, and O. Mansutti, Phys. Rev. D76, 121301 (2007), arXiv: 0707.4312[astro-ph]

  • [11]

    D. Hooper and P. D. Serpico, Phys. Rev. Lett.99, 231102 (2007), arXiv: 0706.3203[hep-ph]

  • [12]

    M. Simet, D. Hooper, and P. D. Serpico, Phys. Rev. D77, 063001 (2008), arXiv: 0712.2825[astro-ph]

  • [13]

    A. Mirizzi, G. G. Raffelt, and P. D. Serpico, Phys. Rev. D76, 023001 (2007), arXiv: 0704.3044[astro-ph]

  • [14]

    A. Mirizzi and D. Montanino, JCAP12, 004 (2009), arXiv: 0911.0015[astro-ph.HE]

  • [15]

    A. V. Belikov, L. Goodenough, and D. Hooper, Phys. Rev. D83, 063005 (2011), arXiv: 1007.4862[astro-ph.HE]

  • [16]

    A. De Angelis, G. Galanti, and M. Roncadelli, Phys. Rev. D84, 105030 (2011), arXiv: 1106.1132[astro-ph.HE]

  • [17]

    D. Horns, L. Maccione, M. Meyeret al., Phys. Rev. D86, 075024 (2012), arXiv: 1207.0776[astro-ph.HE]

  • [18]

    A. Abramowskiet al., Phys. Rev. D88, 102003 (2013), arXiv: 1311.3148[astro-ph.HE]

  • [19]

    M. Meyer, D. Horns, and M. Raue, Phys. Rev. D87, 035027 (2013), arXiv: 1302.1208[astro-ph.HE]

  • [20]

    F. Tavecchio, M. Roncadelli, and G. Galanti, Phys. Lett. B744, 375 (2015), arXiv: 1406.2303[astro-ph.HE]

  • [21]

    M. Meyer, D. Montanino, and J. Conrad, JCAP09, 003 (2014), arXiv: 1406.5972[astro-ph.HE]

  • [22]

    M. Meyer and J. Conrad, JCAP12, 016 (2014), arXiv: 1410.1556[astro-ph.HE]

  • [23]

    M. Ajelloet al., Phys. Rev. Lett.116, 161101 (2016), arXiv: 1603.06978[astro-ph.HE]

  • [24]

    M. Meyer, M. Giannotti, A. Mirizziet al., Phys. Rev. Lett.118, 011103 (2017), arXiv: 1609.02350[astro-ph.HE]

  • [25]

    B. Berenji, J. Gaskins, and M. Meyer, Phys. Rev. D93, 045019 (2016), arXiv: 1602.00091[astro-ph.HE]

  • [26]

    G. Galanti, F. Tavecchio, M. Roncadelliet al., Mon. Not. Roy. Astron. Soc.487, 123 (2019), arXiv: 1811.03548 [astro-ph.HE]

  • [27]

    G. Galanti and M. Roncadelli, JHEAp20, 1 (2018), arXiv: 1805.12055[astro-ph.HE]

  • [28]

    C. Zhang, Y. F. Liang, S. Liet al., Phys. Rev. D97, 063009 (2018), arXiv: 1802.08420[hep-ph]

  • [29]

    Y. F. Liang, C. Zhang, Z. Q. Xiaet al., JCAP06, 042 (2019), arXiv: 1804.07186[hep-ph]

  • [30]

    Z. Q. Xia, C. Zhang, Y. F. Lianget al., Phys. Rev. D97, 063003 (2018), arXiv: 1801.01646[astro-ph.HE]

  • [31]

    X. J. Bi, Y. Gao, J. Guoet al., Phys. Rev. D103, 043018 (2021), arXiv: 2002.01796[astro-ph.HE]

  • [32]

    J. Guo, H. J. Li, X. J. Biet al., Chin. Phys. C45, 025105 (2021), arXiv: 2002.07571[astro-ph.HE]

  • [33]

    H. J. Li, J. G. Guo, X. J. Biet al., Phys. Rev. D103, 083003 (2021), arXiv: 2008.09464[astro-ph.HE]

  • [34]

    Y. F. Liang, X. F. Zhang, J. G. Chenget al., JCAP11, 030 (2021), arXiv: 2012.15513[astro-ph.HE]

  • [35]

    L. Q. Gao, X. J. Bi, J. G. Guoet al., Phys. Rev. D109, 063003 (2024), arXiv: 2309.02166[astro-ph.HE]

  • [36]

    L. Q. Gao, X. J. Bi, J. Liet al., JCAP01, 026 (2024), arXiv: 2310.11391[astro-ph.HE]

  • [37]

    J. Majumdar, F. Calore, and D. Horns, JCAP04, 048 (2018), arXiv: 1801.08813[hep-ph]

  • [38]

    Z. Q. Xia, Y. F. Liang, L. Fenget al., Phys. Rev. D100, 123004 (2019), arXiv: 1911.08096[astroph.HE]

  • [39]

    C. Eckner and F. Calore, Phys. Rev. D106, 083020 (2022), arXiv: 2204.12487[astro-ph.HE]

  • [40]

    G. Galanti, M. Roncadelli, F. Tavecchioet al., Phys. Rev. D107, 103007 (2023), arXiv: 2202.12286[astro-ph.HE]

  • [41]

    C. Dessert, D. Dunsky, and B. R. Safdi, Phys. Rev. D105, 103034 (2022), arXiv: 2203.04319[hep-ph]

  • [42]

    B. R. Safdi, Z. Sun, and A. Y. Chen, Phys. Rev. D99, 123021 (2019), arXiv: 1811.01020[astro-ph.CO]

  • [43]

    S. Hoof and L. Schulz, JCAP03, 054 (2023), arXiv: 2212.09764[hep-ph]

  • [44]

    T. Zhou, L. Q. Gao, X. J. Biet al., (2025), arXiv: 2501.18860[astro-ph.HE]

  • [45]

    S. V. Troitsky, Pisma Zh. Eksp. Teor. Fiz.116, 745 (2022), arXiv: 2210.09250[astro-ph.HE]

  • [46]

    Z. Berezhiani and A. Drago, Phys. Lett. B473, 281 (2000), arXiv: hep-ph/9911333

  • [47]

    L. Wang and B. Q. Ma, Phys. Rev. D108, 023002 (2023), arXiv: 2304.01819[astro-ph.HE]

  • [48]

    B. B. Kamenetskaia, N. Fraija, and G. Herrera, (2024), arXiv: 2408.07352

  • [49]

    D. Wouters and P. Brun, Astrophys. J.772, 44 (2013), arXiv: 1304.0989[astro-ph.HE]

  • [50]

    H. Abeet al., Phys. Dark Univ.44, 101425 (2024), arXiv: 2401.07798[astro-ph.HE]

  • [51]

    D. Malyshev, A. Neronov, D. Semikozet al., (2018), arXiv: 1805.04388[astro-ph.HE]

  • [52]

    J. Li, X. J. Bi, L. Q. Gaoet al., Chin. Phys. C48, 065107 (2024), arXiv: 2401.01829[astroph.HE]

  • [53]

    S. J. Lloyd, P. M. Chadwick, and A. M. Brown, Phys. Rev. D100, 063005 (2019), arXiv: 1908.03413[astro-ph.HE]

  • [54]

    D. Noordhuis, A. Prabhu, S. J. Witteet al., Phys. Rev. Lett.131, 111004 (2023), arXiv: 2209.09917[hep-ph]

  • [55]

    K. D. Lozanov, S. Pi, M. Sasakiet al., (2023), arXiv: 2310.03594[astro-ph.CO]

  • [56]

    F. Tavecchio, M. Roncadelli, G. Galantiet al., Phys. Rev. D86, 085036 (2012), arXiv: 1202.6529[astro-ph.HE]

  • [57]

    O. Mena and S. Razzaque, JCAP11, 023 (2013), arXiv: 1306.5865[astro-ph.HE]

  • [58]

    G. Galanti, Frascati Phys. Ser.69, 102 (2019), arXiv: 1911.09372[astro-ph.HE]

  • [59]

    G. Galanti, M. Landoni, F. Tavecchioet al., Mon. Not. Roy. Astron. Soc.495, 3463 (2020), arXiv: 2002.05052[astro-ph.HE]

  • [60]

    H. J. Li, Phys. Lett. B829, 137047 (2022), arXiv: 2203.08573[astro-ph.HE]

  • [61]

    B. P. Pant, Phys. Rev. D109, 023011 (2024), arXiv: 2310.16634[astro-ph.HE]

  • [62]

    J. Zhang, E. W. Liang, S. N. Zhanget al., Astrophys. J.752, 157 (2012), arXiv: 1108.0146[hep-ph]

  • [63]

    F. Tavecchio, G. Ghisellini, G. Ghirlandaet al., Mon. Not. Roy. Astron. Soc.401, 1570 (2010), arXiv: 0909.0651 [astro-ph.HE]

  • [64]

    L. Chen, Astrophys. J. Suppl.235, 39 (2018), arXiv: 1803.05715[astro-ph.HE]

  • [65]

    D. Thompson, D. Bertsch, B. Dinguset al., Astrophysical Journal Supplement v.101, 259 (1995)

  • [66]

    A. A. Abdo (Fermi-LAT), Astrophys. J.715, 429 (2010), arXiv: 1002.0150[astro-ph.HE]

  • [67]

    R. Mukherjee, V. Collaborationet al., The Astronomer’s Telegram11075, 1 (2017)

  • [68]

    B. Rajput, A. K. Mandal, A. Pandeyet al., Mon. Not. Roy. Astron. Soc.527, 11900 (2023), arXiv: 2312.14857[astro-ph.HE]

  • [69]

    C. Nigro, J. Sitarek, P. Gliwnyet al., Astronomy & Astrophysics660, A18 (2022)

  • [70]

    R. E. Pudritz, M. J. Hardcastle, and D. C. Gabuzda, Space Sci. Rev.169, 27 (2012), arXiv: 1205.2073[astro-ph.HE]

  • [71]

    M. C. Begelman, R. D. Blandford, and M. J. Rees, Rev. Mod. Phys.56, 255 (1984)

  • [72]

    S. P. O’Sullivan and D. C. Gabuzda, Mon. Not. Roy. Astron. Soc.400, 26 (2009), arXiv: 0907.5211[astro-ph.CO]

  • [73]

    A. Dominguezet al., PoSTEXAS2010, 228 (2010), arXiv: 1103.4534[astro-ph.CO]

  • [74]

    Q. H. Cao, Z. Liu, and J. C. Wang, JCAP01, 099 (2025), arXiv: 2307.15602[hep-ph]

  • [75]

    G. Galanti, Phys. Rev. D107, 043006 (2023), arXiv: 2202.11675[astro-ph.HE]

  • [76]

    R. Jansson and G. R. Farrar, Astrophys. J.757, 14 (2012), arXiv: 1204.3662[astro-ph.GA]

  • [77]

    J. M. Cordes and T. J. W. Lazio, (2002), arXiv: astroph/0207156

  • [78]

    M. Meyer, J. Davies, and J. Kuhlmann, PoSICRC2021, 557 (2021), arXiv: 2108.02061[astro-ph.HE]

  • [79]

    R. Mirzoyan, The Astronomer’s Telegram11061, 1 (2017)

  • [80]

    T. Junk, Nucl. Instrum. Meth. A434, 435 (1999), arXiv: hepex/9902006

  • [81]

    A. L. Read, J. Phys. G28, 2693 (2002)

  • [82]

    L. Lista, in 2016 European School of High-Energy Physics (2017) pp. 213–258, arXiv: 1609.04150[physics.data-an]

  • [83]

    L. Q. Gao, X. J. Bi, J. Liet al., JCAP01, 031 (2025), arXiv: 2407.20118[astro-ph.HE]

  • [84]

    V. Anastassopouloset al., Nature Phys.13, 584 (2017), arXiv: 1705.02290[hep-ex]

  • [85]

    C. O’Hare,cajohare/axionlimits: Axionlimits, (2020) https://cajohare.github.io/AxionLimits/

Baidu
map