\begin{document}$g_{a\gamma} \gtrsim 2 \times 10^{-11} \; {\rm GeV}^{-1}$\end{document} for the ALP mass of \begin{document}$ \sim 8\times 10^{-9} \lesssim m_a \lesssim 2\times 10^{-7}\rm \; eV $\end{document} at 95% confidence level. The main uncertainties of the analysis originate from the blazar jet magnetic field model. We also find that the ALP hypothesis can slightly improve the fit to the PG 1553+113 results in several parameter regions. We do not set the limit in this case."> Searching for axion-like particles with the blazar observations of MAGIC and Fermi-LAT -
  • [1]

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

  • [2]

    R. Peccei and H. R. Quinn, Phys. Rev. Lett.38, 1440 (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. B120, 127 (1983)

  • [6]

    L. Abbott and P. Sikivie, Phys. Lett. B120, 133 (1983)

  • [7]

    M. Dine and W. Fischler, Phys. Lett. B120, 137 (1983)

  • [8]

    M. Khlopov, A. Sakharov, and D. Sokoloff, Nucl. Phys. B Proc. Suppl.72, 105 (1999)

  • [9]

    P. Sikivie, Int. J. Mod. Phys. A25, 554 (2010), arXiv:0909.0949[hep-ph

  • [10]

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

  • [11]

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

  • [12]

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

  • [13]

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

  • [14]

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

  • [15]

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

  • [16]

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

  • [17]

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

  • [18]

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

  • [19]

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

  • [20]

    A. Dominguez, M. A. Sanchez-Conde, and F. Prada, JCAP11, 020 (2011), arXiv:1106.1860[astro-ph.CO

  • [21]

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

  • [22]

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

  • [23]

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

  • [24]

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

  • [25]

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

  • [26]

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

  • [27]

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

  • [28]

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

  • [29]

    R. Reesman and T. Walker, JCAP08, 021 (2014), arXiv:1402.2533[astro-ph.HE

  • [30]

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

  • [31]

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

  • [32]

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

  • [33]

    K. Kohri and H. Kodama, Phys. Rev. D96, 051701 (2017), arXiv:1704.05189[hep-ph

  • [34]

    J. Majumdar, F. Calore, and D. Horns, PoSIFS2017, 168 (2017), arXiv:1711.08723[hep-ph

  • [35]

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

  • [36]

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

  • [37]

    G. Galanti and M. Roncadelli, Phys. Rev. D98, 043018 (2018), arXiv:1804.09443[astro-ph.HE

  • [38]

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

  • [39]

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

  • [40]

    M. Libanov and S. Troitsky, Phys. Lett. B802, 135252 (2020), arXiv:1908.03084[astro-ph.HE

  • [41]

    G. Long, W. Lin, P. Tamet al., Phys. Rev. D101, 063004 (2020), arXiv:1912.05309[astro-ph.HE

  • [42]

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

  • [43]

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

  • [44]

    R. Buehler, G. Gallardo, G. Maieret al., JCAP09, 027 (2020), arXiv:2004.09396[astro-ph.HE

  • [45]

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

  • [46]

    J.-G. Cheng, Y.-J. He, Y.-F. Lianget al., Phys. Lett. B821, 136611 (2021), arXiv:2010.12396[astro-ph.HE

  • [47]

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

  • [48]

    G. Long, S. Chen, S. Xuet al., Phys. Rev. D104, 083014 (2021), arXiv:2101.10270[astro-ph.HE

  • [49]

    J. Davies, M. Meyer, and G. Cotter, Phys. Rev. D103, 023008 (2021), arXiv:2011.08123[astro-ph.HE

  • [50]

    J. Zhou, Z. Wang, F. Huanget al., JCAP08, 007 (2021), arXiv:2102.05833[astro-ph.HE

  • [51]

    I. Batković, A. De Angelis, M. Doroet al., Universe7, 185 (2021), arXiv: 2106.03424[astro-ph.HE]

  • [52]

    H. Abdallaet al. (H.E.S.S., LAT), Astron. Astrophys.600, A89 (2017), arXiv:1612.01843[astro-ph.HE

  • [53]

    B. Bartoliet al. (ARGO-YBJ), Astrophys. J. Suppl.222, 6 (2016), arXiv:1511.06851[astro-ph.HE

  • [54]

    V. Acciariet al. (MAGIC), Mon. Not. Roy. Astron. Soc.486, 4233 (2019), arXiv:1904.00134[astro-ph.HE

  • [55]

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

  • [56]

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

  • [57]

    G. Ghisellini and F. Tavecchio, Mon. Not. Roy. Astron. Soc.397, 985 (2009), arXiv:0902.0793[astro-ph.CO

  • [58]

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

  • [59]

    A. Celotti and G. Ghisellini, Mon. Not. Roy. Astron. Soc.385, 283 (2008), arXiv:0711.4112[astro-ph

  • [60]

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

  • [61]

    P. Adeet al. (Planck), Astron. Astrophys.594, A19 (2016), arXiv:1502.01594[astro-ph.CO

  • [62]

    A. Franceschini, G. Rodighiero, and M. Vaccari, Astron. Astrophys.487, 837 (2008), arXiv:0805.1841[astro-ph

  • [63]

    R. Jansson and G. R. Farrar, Astrophys. J. Lett.761, L11 (2012), arXiv:1210.7820[astro-ph.GA

  • [64]

    J. Aleksićet al., Astropart. Phys.72, 61 (2016), arXiv:1409.6073[astro-ph.IM

  • [65]

    J. Aleksićet al. (MAGIC), Astropart. Phys.72, 76 (2016), arXiv:1409.5594[astro-ph.IM

  • [66]

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

  • [67]

    B. Acharyaet al. (CTA Consortium), Astropart. Phys.43, 3 (2013)

  • [68]

    Z. Caoet al. (LHAASO), Chin. Phys. C34, 249 (2010)

  • [69]

    X. Huanget al., Astropart. Phys.78, 35 (2016), arXiv:1509.02672[astro-ph.HE

  • [70]

    A. E. Egorov, N. P. Topchiev, A. M. Galperet al., JCAP11, 049 (2020), arXiv:2005.09032[astro-ph.HE

  • [71]

    L. A. Kuzmichevet al., Phys. Atom. Nucl.81, 497 (2018)

Baidu
map