• [1]

    M. G. Aartsenet al. (IceCube), Science361(6398), 147-151 (2018), arXiv:1807.08794[astro-ph.HE

  • [2]

    Fermi-LATet al. (IceCube, Fermi-LAT, MAGIC, AGILE, ASAS-SN, HAWC, H.E.S.S., INTEGRAL, Kanata, Kiso, Kapteyn, Liverpool Telescope, Subaru, Swift NuSTAR, VERITAS, VLA/17B-403), Science361(6398), eaat1378 (2018), arXiv:1807.08816[astro-ph.HE

  • [3]

    M. G. Aartsenet al. (IceCube), Phys. Rev. Lett.124(5), 051103 (2020), arXiv:1910.08488[astro-ph.HE

  • [4]

    R. Abbasiet al. (IceCube),IceCube Data for Neutrino Point-Source Searches Years 2008-2018, arXiv:2101.09836[astro-ph.HE]

  • [5]

    T. D. Lee and C.-N. Yang, Phys. Rev. Lett.4, 307-311 (1960)

  • [6]

    S. L. Glashow, Phys. Rev.118, 316-317 (1960)

  • [7]

    T. D. Lee, C.-N. Yang, and P. Markstein, Phys. Rev. Lett.7, 429-433 (1961)

  • [8]

    D. Seckel, Phys. Rev. Lett.80, 900-903 (1998), arXiv:hep-ph/9709290

  • [9]

    M. G. Aartsenet al. (IceCube),Nature591(7849), 220–224 (2021), arXiv:2110.15051[hep-ex][Erratum: Nature592, E11 (2021)]

  • [10]

    M. G. Aartsenet al. (IceCube), Phys. Rev. D99(3), 032004 (2019), arXiv:1808.07629[hep-ex

  • [11]

    M. G. Aartsenet al. (IceCube), Nature551, 596-600 (2017), arXiv:1711.08119[hep-ex

  • [12]

    M. Bustamante and A. Connolly, Phys. Rev. Lett.122(4), 041101 (2019), arXiv:1711.11043[astro-ph.HE

  • [13]

    H. Abreuet al. (FASER),Technical Proposal: FASERnu, arXiv:2001.03073[physics.ins-det]

  • [14]

    J. F. Beacom, N. F. Bell, D. Hooperet al., Phys. Rev. Lett.90, 181301 (2003), arXiv:hep-ph/0211305

  • [15]

    D. Hooper, D. Morgan, and E. Winstanley, Phys. Rev. D72, 065009 (2005), arXiv:hep-ph/0506091

  • [16]

    P. Lipari, Phys. Rev. D64, 033002 (2001), arXiv:hep-ph/0102046

  • [17]

    T. Han and D. Hooper, New J. Phys.6, 150 (2004), arXiv:hep-ph/0408348

  • [18]

    J. F. Beacom, N. F. Bell, and G. D. Mack, Phys. Rev. Lett.99, 231301 (2007), arXiv:astro-ph/0608090

  • [19]

    I. F. M. Albuquerque, G. Burdman, and Z. Chacko, Phys. Rev. D75, 035006 (2007), arXiv:hep-ph/0605120

  • [20]

    H. Yuksel, S. Horiuchi, J. F. Beacomet al., Phys. Rev. D76, 123506 (2007), arXiv:0707.0196[astro-ph

  • [21]

    K. C. Y. Ng and J. F. Beacom,Phys. Rev. D90(6), 065035 (2014), arXiv:1404.2288[astro-ph.HE][Erratum: Phys. Rev. D90, 089904 (2014)]

  • [22]

    K. Ioka and K. Murase, PTEP2014(6), 061E (2014), arXiv:1404.2279[astro-ph.HE

  • [23]

    I. M. Shoemaker and K. Murase, Phys. Rev. D93(8), 085004 (2016), arXiv:1512.07228[astro-ph.HE

  • [24]

    K. Murase, R. Laha, S. Andoet al., Phys. Rev. Lett.115(7), 071301 (2015), arXiv:1503.04663[hep-ph

  • [25]

    M. Bustamante, J. F. Beacom, and K. Murase, Phys. Rev. D95(6), 063013 (2017), arXiv:1610.02096[astro-ph.HE

  • [26]

    M. G. Aartsenet al.(IceCube),Eur. Phys. J. C 77(3), 146 (2017)arXiv:1612.05949[astro-ph.HE][Erratum: Eur. Phys. J. C79, 214 (2019)]

  • [27]

    P. B. Denton and I. Tamborra, Phys. Rev. Lett.121(12), 121802 (2018), arXiv:1805.05950[hep-ph

  • [28]

    M. G. Aartsenet al. (IceCube), Eur. Phys. J. C78(10), 831 (2018), arXiv:1804.03848[astro-ph.HE

  • [29]

    A. Albertet al. (ANTARES, IceCube), Phys. Rev. D102(8), 082002 (2020), arXiv:2003.06614[astro-ph.HE

  • [30]

    M. Bustamante, C. Rosenstrøm, S. Shalgaret al., Phys. Rev. D101(12), 123024 (2020), arXiv:2001.04994[astro-ph.HE

  • [31]

    X.-J. Bi, J.-X. Wang, C. Zhanget al., Phys. Rev. D70, 123512 (2004), arXiv:hep-ph/0404263

  • [32]

    K. Kohri and F. Takayama, Phys. Rev. D76, 063507 (2007), arXiv:hep-ph/0605243

  • [33]

    S. Ando, J. F. Beacom, S. Profumoet al., JCAP04, 029 (2008), arXiv:0711.2908[hep-ph

  • [34]

    M. Ahlers, J. I. Illana, M. Masipet al., JCAP08, 008 (2007), arXiv:0705.3782[hep-ph

  • [35]

    P. Meade, S. Nussinov, M. Papucciet al., JHEP06, 029 (2010), arXiv:0910.4160[hep-ph

  • [36]

    J. L. Feng, Ann. Rev. Astron. Astrophys.48, 495-545 (2010), arXiv:1003.0904[astro-ph.CO

  • [37]

    K. Agashe, Y. Cui, L. Necibet al., JCAP10, 062 (2014), arXiv:1405.7370[hep-ph

  • [38]

    S. Kopperet al. (IceCube), PoS ICRC2015, 1104 (2016)

  • [39]

    M. G. Aartsenet al. (IceCube),The IceCube Neutrino Observatory - Contributions to ICRC 2015 Part IV: Searches for Dark Matter and Exotic Particles, arXiv:1510.05226[astro-ph.HE]

  • [40]

    J. L. Feng, J. Smolinsky, and P. Tanedo,Phys. Rev. D93(1), 015014 (2016), arXiv:1509.07525[hep-ph][Erratum: Phys. Rev. D96, 099901 (2017)]

  • [41]

    S.-F. Ge, M. Lindner, and W. Rodejohann, Phys. Lett. B772, 164-168 (2017), arXiv:1702.02617[hep-ph

  • [42]

    D. B. Fox, S. Sigurdsson, S. Shanderaet al., The ANITA Anomalous Events as Signatures of a Beyond Standard Model Particle, and Supporting Observations from IceCube, arXiv:1809.09615[astro-ph.HE]

  • [43]

    P. S. Bhupal Dev,Signatures of Supersymmetry in Neutrino Telescopes, pp. 317–352. 2020. arXiv:1906.02147[hep-ph]

  • [44]

    B. Zhou and J. F. Beacom, Phys. Rev. D101(3), 036010 (2020), arXiv:1910.10720[hep-ph

  • [45]

    B. Zhou and J. F. Beacom, Phys. Rev. D101(3), 036011 (2020), arXiv:1910.08090[hep-ph

  • [46]

    S. Meighen-Berger, M. Agostini, A. Ibarraet al., Phys. Lett. B811, 135929 (2020), arXiv:2005.07523[hep-ph

  • [47]

    J.-H. Schmidt-Denckeret al. (IceCube), PoS ICRC2021, 1117 (2021)

  • [48]

    I. Albuquerque, G. Burdman, and Z. Chacko, Phys. Rev. Lett.92, 221802 (2004), arXiv:hep-ph/0312197

  • [49]

    D. van der Drift and S. R. Klein, Phys. Rev. D88, 033013 (2013), arXiv:1305.5277[astro-ph.HE

  • [50]

    E. L. Berger, J. Gao, C. S. Liet al., Phys. Rev. Lett.116(21), 212002 (2016), arXiv:1601.05430[hep-ph

  • [51]

    J. Gao, JHEP02, 026 (2018), arXiv:1710.04258[hep-ph

  • [52]

    D. A. Mason,Measurement of the strange-antistrange asymmetry at NLO in QCD from NuTeV dimuon data. (University of Oregon, 2006)

  • [53]

    M. Goncharovet al. (NuTeV), Phys. Rev. D64, 112006 (2001), arXiv:hep-ex/0102049

  • [54]

    O. Samoylovet al. (NOMAD), Nucl. Phys. B876, 339-375 (2013), arXiv:1308.4750[hep-ex

  • [55]

    S. Adrian-Martinezet al. (KM3Net), J. Phys. G43(8), 084001 (2016), arXiv:1601.07459[astro-ph.IM

  • [56]

    B. Zhou and J. F. Beacom, Phys. Rev. D105, 093005 (2022)

  • [57]

    M. G. Aartsenet al. (IceCube), Phys. Rev. D89(6), 062007 (2014), arXiv:1311.7048[astro-ph.HE

  • [58]

    J. Ahrenset al. (IceCube), Astropart. Phys.20, 507-532 (2004), arXiv:astro-ph/0305196

  • [59]

    A. Cooper-Sarkar, P. Mertsch, and S. Sarkar, JHEP08, 042 (2011), arXiv:1106.3723[hep-ph

  • [60]

    V. Bertone, R. Gauld, and J. Rojo, JHEP01, 217 (2019), arXiv:1808.02034[hep-ph

  • [61]

    J. Gao, T. J. Hobbs, P. M. Nadolskyet al.,A general heavy-flavor mass scheme for charged-current DIS at NNLO and beyond, arXiv:2107.00460[hep-ph]

  • [62]

    I. F. M. Albuquerque, J. Lamoureux, and G. F. Smoot, Astrophys. J. Suppl.141, 195-209 (2002), arXiv:hep-ph/0109177

  • [63]

    M. G. Aartsenet al. (IceCube), Phys. Rev. D97(7), 072009 (2018), arXiv:1709.07079[hep-ex

  • [64]

    M. Honda, M. Sajjad Athar, T. Kajitaet al., Phys. Rev. D92(2), 023004 (2015), arXiv:1502.03916[astro-ph.HE

  • [65]

    S. Dulat, T.-J. Hou, J. Gaoet al., Phys. Rev. D93(3), 033006 (2016), arXiv:1506.07443[hep-ph

  • [66]

    T. Sjöstrand, S. Ask, J. R. Christiansenet al., Comput. Phys. Commun.191, 159-177 (2015), arXiv:1410.3012[hep-ph

  • [67]

    H. Abreuet al. (FASER), Eur. Phys. J. C80(1), 61 (2020), arXiv:1908.02310[hep-ex

  • [68]

    D. Chirkin and W. Rhode,Muon Monte Carlo: A High-precision tool for muon propagation through matter, arXiv:hep-ph/0407075

  • [69]

    F. Hu, Z. Li, and D. L. Xu, PoS ICRC2021, 1043 (2021), arXiv:2108.05515[astro-ph.IM

  • [70]

    M. G. Aartsenet al. (IceCube), Eur. Phys. J. C77(10), 692 (2017), arXiv:1705.07780[astro-ph.HE

Baidu
map