Publisher Correction: Detection of a particle shower at the Glashow resonance with IceCube

Aartsen, M. G.; Abbasi, Rasha; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alispach, Cyril Martin; Amin, Najia Moureen Binte; Andeen, K.; Anderson, T.; Ansseau, I.; Anton, G.; Argüelles, C.; Auffenberg, J.; Axani, Spencer; Bagherpour, H.; Bai, Xiaozhi; Balagopal, Aswathi; Barbano, Anastasia Maria; Barwick, S. W.; Bastian, Benjamin; Basu, Vedant; Baum, V.; Baur, S.; Bay, R.; Beatty, J. J.; Becker, K.; Tjus, Julia Becker; Bellenghi, Chiara; BenZvi, S.; Berley, D.; Bernardini, E.; Besson, D. Z.; Binder, G.; Bindig, D.; Blaufuss, E.; Blot, Summer; Böhm, C.; Böser, S.; Botner, O.; Böttcher, Jakob; Bourbeau, Etienne; Bourbeau, J.; Bradascio, Federica; Braun, J.; Bron, S.; Brostean-Kaiser, Jannes; Burgman, A.; Büscher, J.; Busse, Raffaela; Campana, Michael; Carver, T.; Chen, C.; Cheung, E.; Chirkin, D.; Choi, Seong Youl; Clark, Brian; Clark, K.; Classen, L.; Coleman, Alan; Collin, Gabriel; Conrad, J. M.; Coppin, Paul; Correa, Pablo; Cowen, D. F.; Cross, R.; Dave, Pranav; Clercq, C. De; DeLaunay, James; Dembinski, H.-P.; Deoskar, Kunal; Ridder, S. De; Desai, Abhishek; Desiati, P.; Vries, Krijn de; Wasseige, Gwenhaël de; DeYoung, T.; Dharani, Sukeerthi; Díaz, A. Casanova; Díaz-Vélez, J.C.; Dujmović, Hrvoje; Dunkman, M.; DuVernois, Michael; Dvorak, Emily; Ehrhardt, Thomas; Eller, P.; Engel, R.; Evenson, P. A.; Fahey, S.; Fazely, A. R.; Fedynitch, Anatoli; Felde, J.; Fienberg, A. T.; Filimonov, K.; Finley, C.; Fischer, Leander; Fox, D.; Franckowiak, A.; Friedman, E.; Fritz, A.; Gaisser, T. K.; Gallagher, J.; Ganster, Erik; Garrappa, S.; Gerhardt, L.; Ghadimi, Ava; Glauch, Theo; Glüsenkamp, T.; Goldschmidt, A.; González, J. G.; Goswami, Sreetama; Grant, D.; Grégoire, T.; Griffith, Z.; Griswold, Spencer; Gündüz, Mehmet; Haack, Christian; Hallgren, A.; Halliday, R.; Halve, L.; Halzen, F.; Hanson, K.; Hardin, John; Haungs, A.; Hauser, Simon; Hebecker, D.; Heix, P.; Helbing, K.; Hellauer, R.; Henningsen, Felix; Hickford, S.; Hignight, J.; Hill, C. W.; Hill, G.C.; Hoffman, K. D.; Hoffmann, R.; Hoinka, Tobias; Hokanson-Fasig, B.; Hoshina, K.; Huang, Fa Peng; Huber, M. E.; Huber, Thomas; Hultqvist, K.; Hünnefeld, Mirco; Hussain, Raamis; In, S.; Iovine, N.; Ishihara, A.; Jansson, Matti; Japaridze, G. S.; Jeong, M. S.; Jones, Ben; Jonske, F.; Joppe, R.; Kang, Dae Kyoung; Kang, W. G.; Kang, X. L.; Kappes, A.; Kappesser, David; Karg, T.; Karl, Martina; Karle, A.; Katz, Uf; Kauer, M.; Kellermann, Moritz; Kelley, J. L.; Kheirandish, Ali; Kim, J.; Kin, Ken'ichi; Kintscher, T.; Kiryluk, J.; Kittler, T.; Klein, S. R.; Koirala, R.; Kolanoski, H.; Köpke, L.; Kopper, C.; Kopper, S.; Koskinen, D. J.; Koundal, Paras; Kovacevich, Michael; Kowalski, M.; Krings, K.; Krückl, G.; Kulacz, N.; Kurahashi, N.; Kyriacou, A.; Gualda, Cristina Lagunas; Lanfranchi, J. L.; Larson, M. J.; Lauber, Frederik Hermann; Lazar, Jeffrey; Leonard, K.; Leszczyńska, Agnieszka; Li, Y.; Liu, Q. R.; Lohfink, Elisa; Mariscal, Cristian Jesús Lozano; Lu, L. C.; Lucarelli, Francesco; Ludwig, A.; Lünemann, J.; Luszczak, William; Lyu, Yang; Y., Ma W.; Madsen, J.; Mäggi, G.; Mahn, Kendall; Makino, Yuya; Mallik, P.; Mancina, Sarah; Maris, Ioana Codrina; Maruyama, R.; Mase, K.; Maunu, R.; McNally, F.; Meagher, K.; Medici, M.; Medina, Alberto Martin Gago; Meier, Michael D; Meighen-Berger, Stephan; Merz, J.; Micallef, J.; Mockler, D.; Momenté, G.; Montaruli, T.; Moore, R. W.; Morse, R.; Moulai, Marjon; Muth, P.; Naab, Richard; Nagai, R.; Naumann, Uwe; Necker, Jannis; Neer, G.; Nguyen, Le Viet; Niederhausen, H.; Nisa, Mehr; Nowicki, S. C.; Nygren, D. R.; Pollmann, A. Obertacke; Oehler, Marie; Olivas, A.; O’Sullivan, Erin; Pandya, Hershal; Pankova, D. V.; Park, N.; Parker, Grant; Paudel, Ek Narayan; Peiffer, P.; Heros, C. Pérez de los; Philippen, Saskia; Pieloth, D.; Pieper, Sarah; Pizzuto, A.; Plum, Michael; Popovych, Yuriy; Porcelli, A.; Rodriguez, Maria Prado; Price, P. Buford; Przybylski, G. T.; Raab, Clemens G.; Raissi, Amirreza; Rameez, M.; Rauch, L.; Rawlins, K.; Rea, Immacolata Carmen; Rehman, A.; Reimann, R.; Relich, M.; Renschler, M.; Renzi, Giovanni; Resconi, E.; Reusch, Simeon; Rhode, W.; Richman, M.; Riedel, Benedikt; Robertson, S.; Roellinghoff, Gerrit; Rongen, Martin; Rott, C.; Ruhe, T.; Ryckbosch, D.; Cantu, Devyn Rysewyk; Safa, Ibrahim; Herrera, S. E. Sanchez; Sandrock, A.; Sandroos, J.; Santander, M.; Sarkar, S.; Satalecka, K.; Scharf, Maximilian Karl; Schaufel, Merlin; Schieler, H.; Schlunder, P.; Schmidt, Th.; Schneider, A.; Schneider, Judith; Schröder, Frank G.; Schumacher, Lisa Johanna; Sclafani, S.; Seckel, D.; Seunarine, S.; Shefali, S.; Silva, M.; Smithers, B.; Snihur, R.; Soedingrekso, Jan; Soldin, D.; Song, M.; Spiczak, G. M.; Spiering, C.; Stachurska, J.; Stamatikos, M.; Stanev, T.; Stein, R.; Stettner, J.; Steuer, A.; Stezelberger, T.; Stokstad, R. G.; Strotjohann, N. L.; Stürwald, Timo; Stuttard, T.; Sullivan, G. W.; Taboada, I.; Tenholt, F.; Ter–Antonyan, S.; Terliuk, A.; Tilav, S.; Tollefson, K.; Tomankova, L.; Tönnis, Christoph; Toscano, S.; Tosi, D.; Trettin, Alexander; Tselengidou, M.; Tung, Chun Fai; Turcati, A.; Turcotte, Roxanne; Turley, C. F.; Twagirayezu, Jean Pierre; Ty, Bunheng; Unger, E.; Elorrieta, M. A. Unland; Vandenbroucke, J.; Eijk, D. van; Eijndhoven, N. van; Vannerom, D.; Santen, J. V.; Verpoest, Stef; Vraeghe, M.; Walck, C.; Wallace, A.; Wandkowsky, N.; Watson, Timothyblake; Weaver, Ch.; Weindl, A.; Weiss, Matthew J.; Weldert, Jan; Wendt, C.; Werthebach, Johannes; Whelan, B. J.; Whitehorn, N.; Wiebe, K.; Wiebusch, C. H.; Williams, D.; Wolf, M.; Wood, T. R.; Woschnagg, K.; Wrede, Gerrit; Wulff, Johan; W., Xu X.; Xu, Yuan-Guo; Yáñez, Juan-Pablo; Yoshida, Shinsuke; Yuan, Tzu-Chiang; Zhang, Z.; Zöcklein, M.

doi:10.1038/s41586-021-03450-1

Cited by 31 publications

(11 citation statements)

References 0 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…There is an exception for electron antineutrinos at 6.3 PeV, at which the induced event rate is enhanced via the W − Glashow resonance channel [58], as this phenomenon only occurs with νe 's. A candidate Glashow resonance event has lately been reported by IceCube [57], indicating the existence of 6 PeV cosmic antineutrinos. This may provide rare opportunities to test the result of [9][10][11] and the D-foam models.…”

Section: Discussionmentioning

confidence: 99%

See 1 more Smart Citation

Lorentz and CPT breaking in gamma-ray burst neutrinos from string theory

2023

J. High Energ. Phys.

View full text Add to dashboard Cite

Previous studies on high-energy gamma-ray burst neutrinos from IceCube suggest a neutrino speed variation at the Lorentz violation (LV) scale of ~6.4 × 1017 GeV, with opposite velocity variances between neutrinos and antineutrinos. Within a spacetime foam model, inspired by string theory, we develop an approach to describe the suggested neutrino/antineutrino propagation properties with both Lorentz invariance and CPT symmetry breaking. A threshold analysis on the bremsstrahlung of electron-positron pair (ν → νee+) for the superluminal (anti)neutrino is performed. We find that, due to the energy violation caused by the quantum foam, such reaction may be restricted to occur at sufficient high energies and could even be kinematically forbidden. Constraints on neutrino LV from vacuum ee+ pair emission are naturally avoided. Future experiments are appealed to test further the CPT violation of cosmic neutrinos and/or neutrino superluminality.

show abstract

Section: Discussionmentioning

confidence: 99%

“…We are grateful to an anonymous referee who reminded us that the cutoff at about 2 PeV has proven an outdated proposal, and who encouraged us to comment on the role played by the newly observed Glashow resonance at IceCube[57].…”

mentioning

confidence: 99%

Lorentz and CPT breaking in gamma-ray burst neutrinos from string theory

2023

J. High Energ. Phys.

View full text Add to dashboard Cite

show abstract

“…However, by assuming energy dependent couplings with LV and sign changes (time delay or time advanced), it is possible to find coincidences with GRBs, with the scale of new physics order ∼10 17 GeV [45] (See [46], regarding the implication of this results in the charged lepton sector). Although this is a very tantalizing result, it is challenging to verify it experimentally because the neutrino and anti-neutrino cross-section difference is less than 15% at ≥200 TeV [47][48][49], and the charge separation is possible only in special reactions, such as resonant W-boson production [50]. In the near future, data from IceCube and neutrino observatories, currently under construction, such as KM3NeT [51] and GVD [52], will provide increased sensitivity to Lorentz violation.…”

Section: Tests Of Lorentz Violation With Kinematic Observablesmentioning

confidence: 89%

Lorentz Symmetry and High-Energy Neutrino Astronomy

Argüelles

Katori

2021

Universe

View full text Add to dashboard Cite

The search of the violation of Lorentz symmetry, or Lorentz violation (LV), is an active research field. The effects of LV are expected to be very small, and special systems are often used to search it. High-energy astrophysical neutrinos offer a unique system to search signatures of LV, due to the three factors: high neutrino energy, long propagation distance, and the presence of quantum mechanical interference. In this brief review, we introduce tests of LV and summarize existing searches of LV, using atmospheric and astrophysical neutrinos.

show abstract

“…This array of detectors is sensitive to essentially two types of events: muon tracks and cascades or showers. The IceCube Collaboration has reported the detection of an approximately isotropic flux of astrophysical neutrinos, spanning energies between several TeV and several PeV [3,4]. In this study, we focus on the 6-year dataset of shower events presented in Ref.…”

Section: Pos(icrc2023)1044mentioning

confidence: 99%