• [1]

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

  • [2]

    M. G. Aartsen et al. (IceCube), Nature 591 , 220 (2021) [Erratum: Nature 592 , E11 (2021)] arXiv: 2110.15051

  • [3]

    V. S. Berezinsky and A. Z. Gazizov, JETP Lett. 25, 254 (1977)

  • [4]

    R. W. Brown and F. W. Stecker, Phys. Rev. D 26, 373 (1982)

  • [5]

    L. A. Anchordoqui, H. Goldberg, F. Halzen et al., Phys. Lett. B 621, 18 (2005), arXiv:hep-ph/0410003

  • [6]

    S. Hummer, M. Maltoni, W. Winter et al., Astropart. Phys. 34, 205 (2010), arXiv:1007.0006

  • [7]

    Z. Z. Xing and S. Zhou, Phys. Rev. D 84, 033006 (2011), arXiv:1105.4114

  • [8]

    A. Bhattacharya, R. Gandhi, W. Rodejohann et al., JCAP 1110, 017 (2011), arXiv:1108.3163

  • [9]

    A. Bhattacharya, R. Gandhi, W. Rodejohann et al., On the interpretation of IceCube cascade events in terms of the Glashow resonance, arXiv: 1209.2422

  • [10]

    V. Barger, J. Learned, and S. Pakvasa, Phys. Rev. D 87(3), 037302 (2013), arXiv:1207.4571

  • [11]

    V. Barger, L. Fu, J. G. Learned et al., Phys. Rev. D 90, 121301 (2014), arXiv:1407.3255

  • [12]

    A. Palladino, G. Pagliaroli, F. L. Villante et al., Eur. Phys. J. C 76(2), 52 (2016), arXiv:1510.05921

  • [13]

    I. M. Shoemaker and K. Murase, Phys. Rev. D 93(8), 085004 (2016), arXiv:1512.07228

  • [14]

    L. A. Anchordoqui, M. M. Block, L. Durand et al., Phys. Rev. D 95(8), 083009 (2017), arXiv:1611.07905

  • [15]

    M. D. Kistler and R. Laha, Phys. Rev. Lett. 120(24), 241105 (2018), arXiv:1605.08781

  • [16]

    D. Biehl, A. Fedynitch, A. Palladino et al., JCAP 1701, 033 (2017), arXiv:1611.07983

  • [17]

    S. Sahu and B. Zhang, JHEAp 18, 1 (2018), arXiv:1612.09043

  • [18]

    G. Y. Huang and Q. Liu, JCAP 03, 005 (2020), arXiv:1912.02976

  • [19]

    S. Zhou, Cosmic Flavor Hexagon for Ultrahigh-energy Neutrinos and Antineutrinos at Neutrino Telescopes, arXiv: 2006.06181

  • [20]

    M. Bustamante, New limits on neutrino decay from the Glashow resonance of high-energy cosmic neutrinos, arXiv: 2004.06844

  • [21]

    V. P. Goncalves, D. R. Gratieri, and A. S. C. Quadros, Eur. Phys. J. C 82(11), 1011 (2022), arXiv:2208.04597

  • [22]

    G. Y. Huang, M. Lindner, and N. Volmer, Inferring astrophysical neutrino sources from the Glashow resonance, arXiv: 2303.13706

  • [23]

    Q. Liu, N. Song, and A. C. Vincent, Probing neutrino production in high-energy astrophysical neutrino sources with the Glashow Resonance, arXiv: 2304.06068

  • [24]

    M. G. Aartsen et al. (IceCube), Science 342, 1242856 (2013), arXiv:1311.5238

  • [25]

    M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 111, 021103 (2013), arXiv:1304.5356

  • [26]

    M. G. Aartsen et al. (IceCube), Science 361(6398), 147 (2018), arXiv:1807.08794

  • [27]

    R. Abbasi et al. (IceCube), Phys. Rev. D 104, 022002 (2021), arXiv:2011.03545

  • [28]

    R. Abbasi et al. (IceCube), Science 378(6619), 538 (2022), arXiv:2211.09972

  • [29]

    R. Abbasi et al., Science 380 (7), 6652 (2023), arXiv: 2307.04427

  • [30]

    V. S. Berezinsky and A. Yu. Smirnov, Astrophys. Space Sci. 32, 461 (1975)

  • [31]

    G. Domokos and S. Kovesi-Domokos, AIP Conf. Proc. 433(1), 390 (1998), arXiv:hep-ph/9801362

  • [32]

    G. Domokos and S. Kovesi-Domokos, Observation of ultrahigh-energy neutrino interactions by orbiting detectors, " arXiv: hep-ph/9805221

  • [33]

    K. S. Capelle, J. W. Cronin, G. Parente et al., Astropart. Phys. 8, 321 (1998), arXiv:astro-ph/9801313

  • [34]

    D. Fargion, A. Aiello, and R. Conversano, Horizontal tau air showers from mountains in deep valley: Traces of UHECR neutrino tau, in Proceedings, 26th International Cosmic Ray Conference (ICRC), August 17-25, 1999, Salt Lake City: Invited, Rapporteur, and Highlight Papers, p. 396. 1999, arXiv: astro-ph/9906450

  • [35]

    D. Fargion, Astrophys. J. 570, 909 (2002), arXiv:astro-ph/0002453

  • [36]

    A. Letessier-Selvon, AIP Conf. Proc. 566(1), 157 (2001), arXiv:astro-ph/0009444

  • [37]

    J. L. Feng, P. Fisher, F. Wilczek et al., Phys. Rev. Lett. 88, 161102 (2002), arXiv:hep-ph/0105067

  • [38]

    A. Kusenko and T. J. Weiler, Phys. Rev. Lett. 88, 161101 (2002), arXiv:hep-ph/0106071

  • [39]

    X. Bertou, P. Billoir, O. Deligny et al., Astropart. Phys. 17, 183 (2002), arXiv:astro-ph/0104452

  • [40]

    Z. Cao, M. A. Huang, P. Sokolsky et al., J. Phys. G 31, 571 (2005), arXiv:astro-ph/0411677

  • [41]

    E. Zas, New J. Phys. 7, 130 (2005), arXiv:astro-ph/0504610

  • [42]

    B. Baret and V. Van Elewyck, Rept. Prog. Phys. 74, 046902 (2011)

  • [43]

    G. Y. Huang, S. Jana, M. Lindner et al., JCAP 02(02), 038 (2022), arXiv:2112.09476

  • [44]

    R. M. Abraham et al., Tau Neutrinos in the Next Decade: from GeV to EeV, arXiv: 2203.05591

  • [45]

    M. Ackermann et al., JHEAp 36, 55 (2022), arXiv:2203.08096

  • [46]

    C. A. Argüelles et al., Snowmass White Paper: Beyond the Standard Model effects on Neutrino Flavor, in 2022 Snowmass Summer Study, 3, 2022, arXiv: 2203.10811

  • [47]

    A. Neronov, D. V. Semikoz, L. A. Anchordoqui et al., Phys. Rev. D 95(2), 023004 (2017), arXiv:1606.03629

  • [48]

    J. Álvarez-Muñiz et al. (GRAND), Sci. China Phys. Mech. Astron. 63(1), 219501 (2020), arXiv:1810.09994

  • [49]

    A. N. Otte, Phys. Rev. D 99(8), 083012 (2019), arXiv:1811.09287

  • [50]

    A. N. Otte, A. M. Brown, M. Doro et al., Trinity: An Air-Shower Imaging Instrument to detect Ultrahigh Energy Neutrinos, arXiv: 1907.08727

  • [51]

    P. Allison et al. (ARA), Phys. Rev. D 102(4), 043021 (2020), arXiv:1912.00987

  • [52]

    Q. Abarr et al., The Payload for Ultrahigh Energy Observations (PUEO): A White Paper, arXiv: 2010.02892

  • [53]

    A. Anker et al., "White Paper: ARIANNA-200 high energy neutrino telescope, " arXiv: 2004.09841.

  • [54]

    J. A. Aguilar et al. (RNO-G), JINST 16(03), P03025 (2021), arXiv:2010.12279

  • [55]

    M. G. Aartsen et al. (IceCube-Gen2), J. Phys. G 48(6), 060501 (2021), arXiv:2008.04323

  • [56]

    A. V. Olinto et al. (POEMMA), JCAP 06, 007 (2021), arXiv:2012.07945

  • [57]

    A. Romero-Wolf et al., An Andean Deep-Valley Detector for High-Energy Tau Neutrinos, in Latin American Strategy Forum for Research Infrastructure, 2, 2020, arXiv: 2002.06475

  • [58]

    S. Wissel et al., PoS ICRC2019, 1033 (2020)

  • [59]

    S. Wissel et al., JCAP 11, 065 (2020), arXiv:2004.12718

  • [60]

    S. Hallmann et al. (IceCube-Gen2), PoS ICRC2021, 1183 (2021), arXiv:2107.08910

  • [61]

    S. Ogawa and M. Sasaki, PoS ICRC2021, 970 (2021)

  • [62]

    K. de Vries et al., PoS ICRC2021, 1195 (2021)

  • [63]

    T. Ježo, M. Klasen, F. Lyonnet et al., Phys. Rev. D 89(7), 077702 (2014), arXiv:1401.6012

  • [64]

    Y. Jho and S. C. Park, Phys. Rev. D 104(1), 015018 (2021), arXiv:1806.03063

  • [65]

    P. B. Denton and Y. Kini, Phys. Rev. D 102, 123019 (2020), arXiv:2007.10334

  • [66]

    A. G. Soto, P. Zhelnin, I. Safa et al., Phys. Rev. Lett. 128(17), 171101 (2022), arXiv:2112.06937

  • [67]

    V. B. Valera, M. Bustamante, and C. Glaser, JHEP 06, 105 (2022), arXiv:2204.04237

  • [68]

    G. Y. Huang, S. Jana, M. Lindner et al., Probing Heavy Sterile Neutrinos at Ultrahigh Energy Neutrino Telescopes via the Dipole Portal, arXiv: 2204.10347

  • [69]

    I. Esteban, S. Prohira, and J. F. Beacom, Detector Requirements for Model-Independent Measurements of Ultrahigh Energy Neutrino Cross Sections, arXiv: 2205.09763

  • [70]

    G. Y. Huang, Eur. Phys. J. C 82(12), 1089 (2022), arXiv:2207.02222

  • [71]

    V. Brdar, P. S. B. Dev, R. Plestid et al., Phys. Lett. B 833, 137358 (2022), arXiv:2207.02860

  • [72]

    A. Garcia Soto, D. Garg, M. H. Reno et al., Phys. Rev. D 107(3), 033009 (2023), arXiv:2209.06282

  • [73]

    V. B. Valera, M. Bustamante, and C. Glaser, Near-future discovery of the diffuse flux of ultra-high-energy cosmic neutrinos, arXiv: 2210.03756

  • [74]

    R. Heighton, L. Heurtier, and M. Spannowsky, Hunting for Neutral Leptons with Ultra-High-Energy Cosmic Rays, arXiv: 2303.11352

  • [75]

    T. Bertólez-Martínez, C. A. Argüelles, I. Esteban et al., JHEP 07, 005 (2023), arXiv:2305.03746

  • [76]

    K. Greisen, Phys. Rev. Lett. 16, 748 (1966)

  • [77]

    G. T. Zatsepin and V. A. Kuzmin, JETP Lett. 4, 78 (1966)

  • [78]

    V. S. Berezinsky and G. T. Zatsepin, Phys. Lett. 28, (1969)

  • [79]

    A. Aab et al. (Pierre Auger), Nucl. Instrum. Meth. A 798, 172 (2015), arXiv:1502.01323

  • [80]

    C. A. Argüelles, J. Salvado, and C. N. Weaver, Comput. Phys. Commun. 255, 107405 (2020)

  • [81]

    J. Alvarez-Muñiz, W. R. Carvalho, A. L. Cummings et al., Phys. Rev. D 97 (2), 023021 (2018) [Erratum: Phys. Rev. D 99 , 069902 (2019)], arXiv: 1707.00334

  • [82]

    A. Garcia, R. Gauld, A. Heijboer, and J. Rojo, JCAP 09, 025 (2020), arXiv:2004.04756

  • [83]

    S. Patel et al. (NuSpaceSim), PoS ,ICRC2021, 1203 (2021), arXiv:2109.08198

  • [84]

    J. H. Koehne, K. Frantzen, M. Schmitz et al., Comput. Phys. Commun. 184, 2070 (2013)

  • [85]

    I. Safa, A. Pizzuto, C. A. Argüelles et al., JCAP 01, 012 (2020), arXiv:1909.10487

  • [86]

    I. Safa, J. Lazar, A. Pizzuto et al., TauRunner: A Public Python Program to Propagate Neutral and Charged Leptons, arXiv: 2110.14662

  • [87]

    https://education.nationalgeographic.org/resource/canyon/.

  • [88]

    A. M. Dziewonski and D. L. Anderson, Phys. Earth Planet. Interiors 25, 297 (1981)

  • [89]

    J. F. Beacom, P. Crotty, and E. W. Kolb, Phys. Rev. D 66, 021302 (2002), arXiv:astro-ph/0111482

  • [90]

    S. I. Dutta, M. H. Reno, and I. Sarcevic, Phys. Rev. D 66, 077302 (2002), arXiv:hep-ph/0207344

  • [91]

    J. Stettner et al. (IceCube), Measurement of the Diffuse Astrophysical Muon-Neutrino Spectrum with Ten Years of IceCube Data, in HAWC Contributions to the 36th International Cosmic Ray Conference (ICRC2019), 2019, arXiv: 1908.09551

  • [92]

    M. G. Aartsen et al. (IceCube), Phys. Rev. D 98(6), 062003 (2018), arXiv:1807.01820

  • [93]

    A. Aab et al. (Pierre Auger), JCAP 10, 022 (2019), arXiv:1906.07422

  • [94]

    O. Mena, S. Palomares-Ruiz, and A. C. Vincent, Phys. Rev. Lett. 113, 091103 (2014), arXiv:1404.0017

  • [95]

    C. Y. Chen, P. S. Bhupal Dev, and A. Soni, Phys. Rev. D 92(7), 073001 (2015), arXiv:1411.5658

  • [96]

    S. Palomares-Ruiz, A. C. Vincent, and O. Mena, Phys. Rev. D 91(10), 103008 (2015), arXiv:1502.02649

  • [97]

    M. G. Aartsen et al. (IceCube), Phys. Rev. Lett. 114(17), 171102 (2015), arXiv:1502.03376

  • [98]

    A. Palladino, G. Pagliaroli, F. L. Villante et al., Phys. Rev. Lett. 114(17), 171101 (2015), arXiv:1502.02923

  • [99]

    C. A. Argüelles, T. Katori, and J. Salvado, Phys. Rev. Lett. 115, 161303 (2015), arXiv:1506.02043

  • [100]

    M. Bustamante, J. F. Beacom, and W. Winter, Phys. Rev. Lett. 115(16), 161302 (2015), arXiv:1506.02645

  • [101]

    M. G. Aartsen et al. (IceCube), Astrophys. J. 809(1), 98 (2015), arXiv:1507.03991

  • [102]

    V. Brdar, J. Kopp, and X.-P. Wang, JCAP 01, 026 (2017), arXiv:1611.04598

  • [103]

    G. D'Amico, Astropart. Phys. 101, 8 (2018), arXiv:1712.04979

  • [104]

    G. Pagliaroli, A. Palladino, F. L. Villante et al., Phys. Rev. D 92(11), 113008 (2015), arXiv:1506.02624

  • [105]

    R. W. Rasmussen, L. Lechner, M. Ackermann et al., Phys. Rev. D 96(8), 083018 (2017), arXiv:1707.07684

  • [106]

    V. Brdar and R. S. L. Hansen, JCAP 02, 023 (2019), arXiv:1812.05541

  • [107]

    M. Bustamante and M. Ahlers, Phys. Rev. Lett. 122(24), 241101 (2019), arXiv:1901.10087

  • [108]

    A. Palladino, Eur. Phys. J. C 79(6), 500 (2019), arXiv:1902.08630

  • [109]

    J. Stachurska et al. (IceCube), EPJ Web Conf. 207, 02005 (2019), arXiv:1905.04237

  • [110]

    N. Song, S. W. Li, C. A. Argüelles et al., JCAP 04, 054 (2021), arXiv:2012.12893

  • [111]

    G. Punzi, eConf C 030908, MODT002 (2003), arXiv:physics/0308063

  • [112]

    M. Agostini, G. Benato, and J. Detwiler, Phys. Rev. D 96(5), 053001 (2017), arXiv:1705.02996

  • [113]

    C. A. Argüelles et al., Eur. Phys. J. C 83(1), 15 (2023), arXiv:2203.10811