\begin{document}$ g_{a\gamma} \approx 1.61 \times 10^{-13}\; \mathrm{GeV}^{-1} $\end{document} for ALP masses \begin{document}$ m_a \lesssim 10^{-9}\; \mathrm{eV} $\end{document} in the galactic center. These results indicate that future MeV missions will probe unexplored regions of the ALP parameter space, with conservative estimates suggesting they could constrain \begin{document}$ g_{a\gamma} $\end{document} values two orders of magnitude below current astrophysical limits. Such observations would provide the most stringent tests to date for ALPs as dark matter candidates in the ultra-light mass regime."> Unveiling axion signals in galactic supernovae with future MeV telescopes -
  • [1]

    L. F. Abbott and P. Sikivie, Phys. Lett. B120(1-3), 133 (1983)

  • [2]

    M. Dine and W. Fischler, Phys. Lett. B120(1-3), 137 (1983)

  • [3]

    John Preskill, Mark B Wise, and Frank Wilczek, Phys. Lett. B120(1-3), 127 (1983)

  • [4]

    R. D. Peccei and H. R. Quinn, Phys. Rev. Lett.38(25), 1440 (1977)

  • [5]

    G. G. Raffelt, J. Redondo, and N. V. Maira, Phys. Rev. D84(10), 103008 (2011)

  • [6]

    P. Sikivie, Phys. Rev. Lett.51(14), 1415 (1983)

  • [7]

    G. G. Raffelt,Stars as laboratories for fundamental physics: The astrophysics of neutrinos, axions, and other weakly interacting particles(Chicago: University of Chicago Press, 1996)

  • [8]

    M. Meyer, M. Giannotti, A. Mirizziet al., Phys. Rev. Lett.118(1), 011103 (2017)

  • [9]

    F. Calore, P. Carenza, C. Eckner,et al, Phys. Rev. D109, 043010 (2024)

  • [10]

    S. Hoof and L. Schulz, JCAP2023(03), 054 (2023)

  • [11]

    H. Primakoff, Phys. Rev.81, 899 (1951)

  • [12]

    A. De Angelis, V. Tatischeff, M. Tavaniet al., Experimental Astronomy44(1), 25 (2017)

  • [13]

    H. Fleischhack for the AMEGO-X team, AMEGO-X: MeV gamma-ray Astronomy in the Multi-messenger Era, in37th International Cosmic Ray Conference(Berlin: Pos, 2022), p.649

  • [14]

    J. A. Tomsick, A. Zoglauer, C. Sleatoret al, arXiv: 1908.04334

  • [15]

    A. Payez, C. Evoli, T. Fischeret al., JCAP2015(02), 006 (2015)

  • [16]

    S. Andriamonje, S. Aune, D. Autieroet al., JCAP2007(04), 010 (2007)

  • [17]

    D. Horns, L. Maccione, M. Meyeret al, Phys. Rev. D86(7), 075024 (2012)

  • [18]

    P. Carenza, M. Giannotti, J. Isernet al., Phys. Rep.1117, 1 (2025)

  • [19]

    A. Lella, F. Calore, P. Carenzaet al., JCAP2024(11), 009 (2024)

  • [20]

    L. Di Lella, A. Pilaftsis, G. Raffeltet al., Phys. Rev. D62, 125011 (2000)

  • [21]

    G.G. Raffelt, J. Phys. A: Math. Theor.40(25), 6607 (2007)

  • [22]

    P. Carenza, A. Mirizzi, and G. Sigl, Phys. Rev. D101, 103016 (2020)

  • [23]

    A. Caputo, G. G. Raffelt, and E. Vitagliano, Phys. Rev. D105, 035022 (2022)

  • [24]

    F. Calore, P. Carenza, M. Giannottiet al., Phys. Rev. D105, 063026 (2022)

  • [25]

    T. Rembiasz, M. Obergaulinger, M. Masipet al., Phys. Rev. D98, 103010 (2018)

  • [26]

    K. Mori, T. Takiwaki, K. Kotakeet al., Phys. Rev. D105, 063009 (2022)

  • [27]

    Z. Berezhiani and A. Drago, Phys. Lett. B473(3–4), 281 (2000)

  • [28]

    M. D. Diamond and G. Marques-Tavares, Phys. Rev. Lett.128, 211101 (2022)

  • [29]

    K. Mori, T. Takiwaki, K. Kotakeet al., Phys. Rev. D108(6), 063027 (2023)

  • [30]

    J. McEnery, J. A. Barrio, I. Agudoet al., arXiv: 1907.07558

  • [31]

    B. W. Carroll and D. A. Ostlie,An Introduction to Modern Astrophysics(2nd edition, New York: Pearson Education Inc., 2006)

  • [32]

    E. M. Levesque, P. Massey, and K.A. G. Olsen, ApJ628(2), 973 (2005)

  • [33]

    J. Binney and M. Merrifield,Galactic astronomy(Princeton: Princeton University Press, 2021)

  • [34]

    Z. Xie, B. Liu, J. Liuet al., Phys. Rev. D109, 043020 (2024)

  • [35]

    T. Siegert, J. Berteaud, F. Caloreet al., A&A660, A130 (2022)

  • [36]

    A. E. Vladimirov, S. W. Digel, G. Jóhannessonet al., Comput. Phys. Commun.182, 1156 (2011)

  • [37]

    The Fermi-LAT collaboration. Galactic interstellar emission model for the 4fgl catalog analysis.open document, 2019.

  • [38]

    G. J. Feldman and R. D. Cousins, Phys. Rev. D57(7), 3873 (1998)

  • [39]

    R. Jansson and G. R. Farrar, ApJ757(1), 14 (2012)

  • [40]

    R. Neilson, J. B. Lester, X. Hauboiset al., Asp conf. ser. Vol. 451, 9th pacific rim conference on stellar astrophysics. 2011.

  • [41]

    R. Diehl, H. Halloin, K. Kretschmeret al., Nature439(7072), 45 (2006)

  • [42]

    E. F. Keane and M. Kramer, Mon. Not. R. Astron. Soc.391(4), 2009 (2008)

  • [43]

    S. M. Adams, C.S. Kochanek, J. F. Beacomet al., ApJ778(2), 164 (2013)

  • [44]

    J. F. Beacom and P. Vogel, Phys. Rev. D60, 033007 (1999)

  • [45]

    R. Tomàs, D. Semikoz, G. G. Raffeltet al. , Phys. Rev. D68(9), 093013 (2003)

  • [46]

    M. Mukhopadhyay, C. Lunardini, F.X. Timmeset al., The Astrophysical Journal899(2), 153 (2020)

  • [47]

    V. Syvolap and O. Ruchayskiy, Phys. Rev. D110(11), 115043 (2024)

  • [48]

    D.A. Green, Journal of Astrophysics and Astronomy46(1), 1 (2025)

  • [49]

    S. Abe, M. Eizuka, S. Futagiet al., arXiv: 2404.09920

  • [50]

    A. D. Santos, arXiv: 2405.07900

  • [51]

    N. Kurahashi for the IceCube Collaboration, arXiv: 2310.12840

  • [52]

    F. Di Lodovicoet al., J. Phys. Conf. Ser.888, 012020 (2017)

  • [53]

    JUNO Collaborationet al., arXiv: 2405.18008

  • [54]

    B. Abi, R. Acciarri, M. A. Aceroet al., J. Instrum.15(08), T08008 (2020)

  • [55]

    K. Scholberg, Annu. Rev. Nucl. Part. Sci.62(1), 81 (2012)

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