Characteristics of the Diffuse Astrophysical Electron and Tau Neutrino Flux with Six Years of IceCube High Energy Cascade Data

Aartsen, M. G.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alispach, Cyril Martin; Andeen, K.; Anderson, W. G.; Ansseau, I.; Anton, G.; Argüelles, C.; Auffenberg, J.; Axani, Spencer; Backes, Paul; Bagherpour, H.; Bai, X.; Barbano, Anastasia Maria; Barwick, S. W.; Bastian, Benjamin; Baum, V.; Baur, S.; Bay, R.; Beatty, J. J.; Becker, K. H.; Tjus, J. Becker; BenZvi, S.; Berley, D.; Bernardini, E.; Besson, D.; 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; Carver, T.; Chen, C.; Cheung, E.; Chirkin, D.; Choi, S.; 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; Desiati, P.; Vries, Krijn de; Wasseige, Gwenhaël de; DeYoung, T.; Dı́az, A.; Díaz-Vélez, J. C.; Dujmović, Hrvoje; Dunkman, M.; Dvorak, Emily; Eberhardt, B.; Ehrhardt, Thomas; Eller, P.; Engel, R.; Evenson, P. A.; Fahey, S.; Fazely, A. R.; Felde, J.; Filimonov, K.; Finley, C.; Fox, D. B.; Franckowiak, A.; Friedman, E.; Fritz, A.; Gaisser, T. K.; Gallagher, John S.; Ganster, Erik; Garrappa, S.; Gerhardt, L.; Ghorbani, K.; Glauch, Theo; Glüsenkamp, T.; Goldschmidt, A.; González, J. G.; Grant, D.; Grégoire, T.; Griffith, Z.; Griswold, Spencer; Günder, M.; Gündüz, Mehmet; Haack, Christian; Hallgren, A.; Halliday, R.; Halve, L.; Halzen, F.; Hanson, K.; Haungs, A.; Hebecker, D.; Heereman, D.; Heix, P.; Helbing, K.; Hellauer, R.; Henningsen, Felix; Hickford, S.; Hignight, J.; Hill, G. C.; Hoffman, K. D.; Hoffmann, R.; Hoinka, Tobias; Hokanson-Fasig, B.; Hoshina, K.; Huang, F.; Huber, Matthías; Huber, Thomas; Hultqvist, K.; Hünnefeld, Mirco; Hussain, Raamis; In, S.; Iovine, N.; Ishihara, A.; Jansson, Matti; Japaridze, G. S.; Jeong, Minjin; Jero, K.; Jones, B. J. P.; Jonske, F.; Joppe, R.; Kang, D.; Kang, Woosik; Kappes, A.; Kappesser, David; Karg, T.; Karl, Martina; Karle, A.; Katz, U.; Kauer, M.; Kelley, J. L.; Kheirandish, Ali; Kim, J.; Kintscher, T.; Kiryluk, J.; Kittler, T.; Klein, S. R.; Koirala, R.; Kolanoski, H.; Köpke, L.; Kopper, C.; Kopper, S.; Koskinen, D. J.; Kowalski, M.; Krings, K.; Krückl, G.; Kulacz, N.; Kurahashi, N.; Kyriacou, A.; Lanfranchi, J. L.; Larson, M. J.; Lauber, Frederik Hermann; Lazar, Jeffrey; Leonard, K.; Lesiak-Bzdak, M.; Leszczyńska, Agnieszka; Leuermann, M.; Liu, Q. R.; Lohfink, Elisa; Mariscal, Cristian Jesús Lozano; Lu, Lu; Lucarelli, F.; Lünemann, J.; Luszczak, William; Lyu, Y.; Y., W.; Madsen, J.; Maggi, G.; Mahn, Kendall; Makino, Yuya; Mallik, P.; Mallot, K.; Mancina, Sarah; Maris, Ioana Codrina; Maruyama, R.; Mase, K.; Maunu, R.; McNally, F.; Meagher, K.; Medici, M.; Medina, Andrés; Meier, Maximilian; Meighen-Berger, Stephan; Merino, G.; Meures, T.; Micallef, Jessie; Mockler, D.; Momenté, G.; Montaruli, T.; Moore, R. W.; Morse, R.; Moulai, Marjon; Muth, P.; Nagai, Ryo; Naumann, Uwe; Neer, G.; Niederhausen, H.; Nisa, Mehr; Nowicki, S. C.; Nygren, D. R.; Pollmann, A. Obertacke; Oehler, Marie; Olivas, A.; O’Murchadha, A.; O’Sullivan, Erin; Palczewski, T.; Pandya, Hershal; Pankova, D. V.; Park, N.; Peiffer, P.; Heros, C. Pérez de los; Philippen, Saskia; Pieloth, D.; Pieper, Sarah; Pinat, E.; Pizzuto, A.; Plum, M.; Porcelli, A.; Price, P. B.; Przybylski, G. T.; Raab, Christoph; Raissi, Amirreza; Rameez, M.; Rauch, L.; Rawlins, K.; Rea, Immacolata Carmen; Rehman, Abdul; Reimann, R.; Relethford, B.; Renschler, M.; Renzi, Giovanni; Resconi, E.; Rhode, W.; Richman, M.; Robertson, Sally; Rongen, Martin; Rott, C.; Ruhe, T.; Ryckbosch, D.; Rysewyk, D.; Safa, Ibrahim; Herrera, S. E. Sanchez; Sandrock, A.; Sandroos, J.; Santander, M.; Sarkar, S.; Satalecka, K.; Schaufel, Merlin; Schieler, H.; Schlunder, P.; Schmidt, T.; Schneider, A.; Schneider, Judith; Schröder, Frank G.; Schumacher, Lisa Johanna; Sclafani, S.; Seckel, D.; Seunarine, S.; Shefali, S.; Silva, M.; 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.; Stößl, A.; 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.; Ty, Bunheng; Unger, E.; Elorrieta, M. A. Unland; Usner, M.; Vandenbroucke, J.; Driessche, W. Van; Eijk, D. van; Eijndhoven, N. van; Santen, J. V.; Verpoest, Stef; Vraeghe, M.; Walck, C.; Wallace, A.; Wallraff, M.; Wandkowsky, N.; Watson, T. B.; Weaver, Ch.; Weindl, A.; Weiss, Matthew J.; Weldert, Jan; Wendt, C.; Werthebach, Johannes; Whelan, B. J.; Whitehorn, N.; Wiebe, K.; Wiebusch, Christopher; Wille, L.; Williams, D. R.; Wills, L.; Wolf, M.; Wood, J.; Wood, T. R.; Woschnagg, K.; Wrede, Gerrit; Xu, D. L.; Xu, X. W.; Yin, Xuefeng; Yañez, J. P.; Yodh, G.; Yoshida, Shigeru; Yuan, Tony; Zöcklein, M.

doi:10.1103/physrevlett.125.121104

Cited by 192 publications

(210 citation statements)

References 72 publications

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“…In addition, cosmic rays interacting within Earth's atmosphere produce showers of particles, including atmospheric muons and neutrinos, which comprise a large background when searching for astrophysical neutrinos. Despite these challenges, a diffuse astrophysical neutrino flux has been detected (Aartsen et al 2016a(Aartsen et al , 2013a(Aartsen et al , 2014(Aartsen et al , 2020aSchneider 2020;Stettner 2020), and has been described, using simple power laws, from energies of about 10 TeV to 10 PeV. Although evidence for a first high-energy neutrino source has been presented, it is estimated that any neutrino flux from the object TXS 0506+056 could account for no more than 1% of the total diffuse flux (Aartsen et al 2020a).…”

Section: Introductionmentioning

confidence: 99%

Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

Abbasi¹,

Ackermann²,

Adams³

et al. 2021

ApJ

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In multi-messenger astronomy, rapid investigation of interesting transients is imperative. As an observatory with a 4π steradian field of view, and ∼99% uptime, the IceCube Neutrino Observatory is a unique facility to follow up transients, as well as to provide valuable insights for other observatories and inform their observational decisions. Since 2016, IceCube has been using low-latency data to rapidly respond to interesting astrophysical events reported by the multi-messenger observational community. Here, we describe the pipeline used to perform these followup analyses, and provide a summary of the 58 analyses performed as of July 2020. We find no significant signal in the first 58 analyses performed. The pipeline has helped inform various electromagnetic observation strategies, and has constrained neutrino emission from potential hadronic cosmic accelerators.

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Section: Introductionmentioning

confidence: 99%

Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

Abbasi¹,

Ackermann²,

Adams³

et al. 2021

ApJ

Self Cite

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“…The non-standard interactions of solar neutrinos with electrons and nuclei, in neutrino experiments (e.g., COHERENT) and DM experiments (e.g., LZ and Darwin), examine this light Z region [101,102]. The Z -resonant non-standard interactions of high-energy neutrinos with cosmic neutrino background lead to a "dip" in the high-energy neutrino spectrum [91,103,104], which may explain (though not statistically significant) the null detection of astrophysical neutrinos with 200-400 TeV in IceCube [105][106][107]. The light Z can be probed as missing-energy events in colliders [108,109].…”

Section: Jhep12(2020)202mentioning

confidence: 99%

Maximally self-interacting dark matter: models and predictions

Kamada

Kim

Kuwahara

2020

J. High Energ. Phys.

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We study self-interacting dark matter (SIDM) scenarios, where the s-wave self-scattering cross section almost saturates the Unitarity bound. Such self-scattering cross sections are singly parameterized by the dark matter mass, and are featured by strong velocity dependence in a wide range of velocities. They may be indicated by observations of dark matter halos in a wide range of masses, from Milky Way’s dwarf spheroidal galaxies to galaxy clusters. We pin down the model parameters that saturates the Unitarity bound in well-motivated SIDM models: the gauged Lμ− Lτ model and composite asymmetric dark matter model. We discuss implications and predictions of such model parameters for cosmology like the H0 tension and dark-matter direct-detection experiments, and particle phenomenology like the beam-dump experiments.

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“…25 −0.24 [GeV cm −2 s −1 sr −1 ] (per-flavor) and γ astro = 2.28 +0.08 −0.09 . A summary of these results for all 3 datasets discussed in this dissertation can be found in Table 2.1 and Figure 2.7 [92]. Although this may seem strange at first since we expect a common origin for the astrophysical neutrinos independently of the morphology of their signals in the detector, these datasets are actually consistent with each other at a ∼ 2σ level.…”

Section: Through-going µ-Track Datasetmentioning

confidence: 62%

“…Just as before, events below 60 TeV (shaded region) are excluded from the analysis/fit, leaving us with 60 events above this threshold. [92]. Crosses represent the differential model best fit results (see caption in Fig.…”

Section: Table Of Contentsmentioning

confidence: 99%

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Cascaded Gamma-Ray Counterpart of the Icecube Neutrinos

GALVAO¹

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Characteristics of the Diffuse Astrophysical Electron and Tau Neutrino Flux with Six Years of IceCube High Energy Cascade Data

Cited by 192 publications

References 72 publications

Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory

Maximally self-interacting dark matter: models and predictions

Cascaded Gamma-Ray Counterpart of the Icecube Neutrinos

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