Exploring axion-like particle from observation of FSRQ Ton 599 by Fermi-LAT

[1]
P. Svrcek and E. Witten, JHEP 06, 051 (2006), arXiv: hepth/0605206
[2]
A. Arvanitaki, S. Dimopoulos, S. Dubovsky et al., Phys. Rev. D 81, 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. D 16, 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. D 37, 1237 (1988)
[9]
A. De Angelis, O. Mansutti, and M. Roncadelli, Phys. Lett. B 659, 847 (2008), arXiv: 0707.2695[astro-ph]
[10]
A. De Angelis, M. Roncadelli, and O. Mansutti, Phys. Rev. D 76, 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. D 77, 063001 (2008), arXiv: 0712.2825[astro-ph]
[13]
A. Mirizzi, G. G. Raffelt, and P. D. Serpico, Phys. Rev. D 76, 023001 (2007), arXiv: 0704.3044[astro-ph]
[14]
A. Mirizzi and D. Montanino, JCAP 12, 004 (2009), arXiv: 0911.0015[astro-ph.HE]
[15]
A. V. Belikov, L. Goodenough, and D. Hooper, Phys. Rev. D 83, 063005 (2011), arXiv: 1007.4862[astro-ph.HE]
[16]
A. De Angelis, G. Galanti, and M. Roncadelli, Phys. Rev. D 84, 105030 (2011), arXiv: 1106.1132[astro-ph.HE]
[17]
D. Horns, L. Maccione, M. Meyer et al., Phys. Rev. D 86, 075024 (2012), arXiv: 1207.0776[astro-ph.HE]
[18]
A. Abramowski et al., Phys. Rev. D 88, 102003 (2013), arXiv: 1311.3148[astro-ph.HE]
[19]
M. Meyer, D. Horns, and M. Raue, Phys. Rev. D 87, 035027 (2013), arXiv: 1302.1208[astro-ph.HE]
[20]
F. Tavecchio, M. Roncadelli, and G. Galanti, Phys. Lett. B 744, 375 (2015), arXiv: 1406.2303[astro-ph.HE]
[21]
M. Meyer, D. Montanino, and J. Conrad, JCAP 09, 003 (2014), arXiv: 1406.5972[astro-ph.HE]
[22]
M. Meyer and J. Conrad, JCAP 12, 016 (2014), arXiv: 1410.1556[astro-ph.HE]
[23]
M. Ajello et al., Phys. Rev. Lett. 116, 161101 (2016), arXiv: 1603.06978[astro-ph.HE]
[24]
M. Meyer, M. Giannotti, A. Mirizzi et al., Phys. Rev. Lett. 118, 011103 (2017), arXiv: 1609.02350[astro-ph.HE]
[25]
B. Berenji, J. Gaskins, and M. Meyer, Phys. Rev. D 93, 045019 (2016), arXiv: 1602.00091[astro-ph.HE]
[26]
G. Galanti, F. Tavecchio, M. Roncadelli et al., Mon. Not. Roy. Astron. Soc. 487, 123 (2019), arXiv: 1811.03548 [astro-ph.HE]
[27]
G. Galanti and M. Roncadelli, JHEAp 20, 1 (2018), arXiv: 1805.12055[astro-ph.HE]
[28]
C. Zhang, Y. F. Liang, S. Li et al., Phys. Rev. D 97, 063009 (2018), arXiv: 1802.08420[hep-ph]
[29]
Y. F. Liang, C. Zhang, Z. Q. Xia et al., JCAP 06, 042 (2019), arXiv: 1804.07186[hep-ph]
[30]
Z. Q. Xia, C. Zhang, Y. F. Liang et al., Phys. Rev. D 97, 063003 (2018), arXiv: 1801.01646[astro-ph.HE]
[31]
X. J. Bi, Y. Gao, J. Guo et al., Phys. Rev. D 103, 043018 (2021), arXiv: 2002.01796[astro-ph.HE]
[32]
J. Guo, H. J. Li, X. J. Bi et al., Chin. Phys. C 45, 025105 (2021), arXiv: 2002.07571[astro-ph.HE]
[33]
H. J. Li, J. G. Guo, X. J. Bi et al., Phys. Rev. D 103, 083003 (2021), arXiv: 2008.09464[astro-ph.HE]
[34]
Y. F. Liang, X. F. Zhang, J. G. Cheng et al., JCAP 11, 030 (2021), arXiv: 2012.15513[astro-ph.HE]
[35]
L. Q. Gao, X. J. Bi, J. G. Guo et al., Phys. Rev. D 109, 063003 (2024), arXiv: 2309.02166[astro-ph.HE]
[36]
L. Q. Gao, X. J. Bi, J. Li et al., JCAP 01, 026 (2024), arXiv: 2310.11391[astro-ph.HE]
[37]
J. Majumdar, F. Calore, and D. Horns, JCAP 04, 048 (2018), arXiv: 1801.08813[hep-ph]
[38]
Z. Q. Xia, Y. F. Liang, L. Feng et al., Phys. Rev. D 100, 123004 (2019), arXiv: 1911.08096[astroph.HE]
[39]
C. Eckner and F. Calore, Phys. Rev. D 106, 083020 (2022), arXiv: 2204.12487[astro-ph.HE]
[40]
G. Galanti, M. Roncadelli, F. Tavecchio et al., Phys. Rev. D 107, 103007 (2023), arXiv: 2202.12286[astro-ph.HE]
[41]
C. Dessert, D. Dunsky, and B. R. Safdi, Phys. Rev. D 105, 103034 (2022), arXiv: 2203.04319[hep-ph]
[42]
B. R. Safdi, Z. Sun, and A. Y. Chen, Phys. Rev. D 99, 123021 (2019), arXiv: 1811.01020[astro-ph.CO]
[43]
S. Hoof and L. Schulz, JCAP 03, 054 (2023), arXiv: 2212.09764[hep-ph]
[44]
T. Zhou, L. Q. Gao, X. J. Bi et 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. B 473, 281 (2000), arXiv: hep-ph/9911333
[47]
L. Wang and B. Q. Ma, Phys. Rev. D 108, 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. Abe et al., Phys. Dark Univ. 44, 101425 (2024), arXiv: 2401.07798[astro-ph.HE]
[51]
D. Malyshev, A. Neronov, D. Semikoz et al., (2018), arXiv: 1805.04388[astro-ph.HE]
[52]
J. Li, X. J. Bi, L. Q. Gao et al., Chin. Phys. C 48, 065107 (2024), arXiv: 2401.01829[astroph.HE]
[53]
S. J. Lloyd, P. M. Chadwick, and A. M. Brown, Phys. Rev. D 100, 063005 (2019), arXiv: 1908.03413[astro-ph.HE]
[54]
D. Noordhuis, A. Prabhu, S. J. Witte et al., Phys. Rev. Lett. 131, 111004 (2023), arXiv: 2209.09917[hep-ph]
[55]
K. D. Lozanov, S. Pi, M. Sasaki et al., (2023), arXiv: 2310.03594[astro-ph.CO]
[56]
F. Tavecchio, M. Roncadelli, G. Galanti et al., Phys. Rev. D 86, 085036 (2012), arXiv: 1202.6529[astro-ph.HE]
[57]
O. Mena and S. Razzaque, JCAP 11, 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. Tavecchio et al., Mon. Not. Roy. Astron. Soc. 495, 3463 (2020), arXiv: 2002.05052[astro-ph.HE]
[60]
H. J. Li, Phys. Lett. B 829, 137047 (2022), arXiv: 2203.08573[astro-ph.HE]
[61]
B. P. Pant, Phys. Rev. D 109, 023011 (2024), arXiv: 2310.16634[astro-ph.HE]
[62]
J. Zhang, E. W. Liang, S. N. Zhang et al., Astrophys. J. 752, 157 (2012), arXiv: 1108.0146[hep-ph]
[63]
F. Tavecchio, G. Ghisellini, G. Ghirlanda et 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. Dingus et 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. Collaboration et al., The Astronomer’s Telegram 11075, 1 (2017)
[68]
B. Rajput, A. K. Mandal, A. Pandey et al., Mon. Not. Roy. Astron. Soc. 527, 11900 (2023), arXiv: 2312.14857[astro-ph.HE]
[69]
C. Nigro, J. Sitarek, P. Gliwny et al., Astronomy & Astrophysics 660, 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. Dominguez et al., PoS TEXAS2010, 228 (2010), arXiv: 1103.4534[astro-ph.CO]
[74]
Q. H. Cao, Z. Liu, and J. C. Wang, JCAP 01, 099 (2025), arXiv: 2307.15602[hep-ph]
[75]
G. Galanti, Phys. Rev. D 107, 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, PoS ICRC2021, 557 (2021), arXiv: 2108.02061[astro-ph.HE]
[79]
R. Mirzoyan, The Astronomer’s Telegram 11061, 1 (2017)
[80]
T. Junk, Nucl. Instrum. Meth. A 434, 435 (1999), arXiv: hepex/9902006
[81]
A. L. Read, J. Phys. G 28, 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. Li et al., JCAP 01, 031 (2025), arXiv: 2407.20118[astro-ph.HE]
[84]
V. Anastassopoulos et al., Nature Phys. 13, 584 (2017), arXiv: 1705.02290[hep-ex]
[85]
C. O’Hare, cajohare/axionlimits: Axionlimits, (2020) https://cajohare.github.io/AxionLimits/