Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

Aartsen, M. G.; Ackermann, M.; Adams, J.; Aguilar, J. A.; Ahlers, M.; Ahrens, M.; Alispach, Cyril Martin; Andeen, K.; Anderson, Tyler; Ansseau, I.; Anton, Gisela; Argüelles, C.; Arlen, T. C.; Auffenberg, J.; Axani, Spencer; Backes, Paul; Bagherpour, H.; Bai, X.; Balagopal, Aswathi; Barbano, Anastasia Maria; Bartos, I.; Barwick, S. W.; Bastian, Benjamin; Baum, V.; Baur, S.; Bay, R.; Beatty, J. J.; Becker, K.-H.; Tjus, Julia Becker; BenZvi, S.; Berley, D.; Bernardini, E.; Besson, D.; Binder, G.; Bindig, D.; Blaufuss, E.; Blot, Summer; Böhm, C.; Böhmer, M.; 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; With, M. de; DeYoung, Tyce; Dı́az, A.; Díaz–Vélez, Juan Carlos; Dujmović, Hrvoje; Dunkman, M.; DuVernois, Michael; Dvorak, Emily; Eberhardt, B.; Ehrhardt, Thomas; Eller, P.; Engel, R.; Evans, Justin J.; Evenson, P. A.; Fahey, S.; Farrag, Kareem Ramadan; Fazely, A. R.; Felde, J.; Filimonov, K.; Finley, C.; Fox, D. B.; Franckowiak, A.; Friedman, E.; Fritz, A.; Gaisser, T. K.; Gallagher, J.; Ganster, Erik; Garrappa, S.; Gärtner, Andreas; Gerhardt, L.; Gernhäeuser, R.; Ghorbani, K.; Glauch, Theo; Glüsenkamp, T.; Goldschmidt, A.; González, J. G.; Grant, D.; Griffith, Z.; Griswold, Spencer; Günder, M.; Gündüz, Mehmet; Haack, Christian; Hallgren, A.; Halliday, R.; Halve, L.; Halzen, F.; Hanson, K.; Haugen, J.; 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, Benjamin D.; Hoffmann, R.; Hoinka, Tobias; Hokanson-Fasig, B.; Holzapfel, K.; Hoshina, K.; Huang, Feng; Huber, Matthías; Huber, Thomas; Huege, T.; Hultqvist, K.; Hünnefeld, Mirco; Hussain, Raamis; In, S.; Iovine, N.; Ishihara, A.; Japaridze, G. S.; Jeong, Minjin; Jero, K.; Jones, B. J. P.; Jonske, F.; Joppe, R.; Kalekin, O.; Kang, D.; Kang, W.; Kappes, A.; Kappesser, David; Karg, T.; Karl, Martina; Karle, A.; Katori, T.; Katz, U.; Kauer, M.; Keivani, A.; 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.; Krauss, C. B.; Krings, K.; Krückl, G.; Kulacz, N.; Kurahashi, N.; Kyriacou, A.; Lanfranchi, J. L.; Larson, M. J.; Lauber, Frederik Hermann; Lazar, J. P.; Leonard, K.; Leszczyńska, Agnieszka; Leuermann, M.; Liu, Q. R.; Lohfink, Elisa; LoSecco, J. M.; Mariscal, Cristian Jesús Lozano; Lu, Lina; Lucarelli, Francesco; Lünemann, J.; Luszczak, William; Lyu, Yang; Y., W.; Madsen, J.; Maggi, G.; Mahn, Kendall; Makino, Yuya; Mallik, P.; Mallot, K.; Mancina, Sarah; Mandalia, Shivesh; Maris, Ioana Codrina; Márka, S.; Márka, Z.; 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.; Papp, L.; Park, N.; Peiffer, P.; Heros, C. Pérez de los; Petersen, T. C.; Philippen, Saskia; Pieloth, D.; Pinat, E.; Pinfold, J. L.; 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; Reimann, R.; Relethford, B.; Renschler, M.; Renzi, Giovanni; Resconi, E.; Rhode, W.; Richman, M.; Riegel, Michael; Robertson, Sally; Rongen, Martin; Rott, C.; Ruhe, T.; Ryckbosch, D.; Rysewyk, D.; Safa, Ibrahim; Herrera, S. E. Sanchez; Sandrock, Alexander; Sandroos, J.; Sandstrom, P.; Santander, M.; Sarkar, Sourav; 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.; Shaevitz, M. H.; Shefali, S.; Silva, M.; Snihur, R.; Soedingrekso, Jan; Soldin, D.; Söldner-Rembold, S.; 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.; Taketa, A.; Tanaka, Hiroyuki; Tenholt, F.; Ter–Antonyan, S.; Terliuk, A.; Tilav, S.; Tollefson, K.; Tomankova, L.; Tönnis, Christoph; Toscano, S.; Tosi, D.; Trettin, Alexander; Tselengidou, M.; Tung, Chunfai; 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.; Veberič, D.; Verpoest, Stef; Vraeghe, M.; Walck, C.; Wallace, A.; Wallraff, M.; 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, Christopher; Wille, L.; Williams, D. R.; Wills, L.; Wolf, M.; Wood, J.; Wood, T. R.; Woschnagg, K.; Wrede, Gerrit; Wren, Steven; Xu, Dawei; Xu, X. W.; Yañez, J. P.; Yodh, G.; Yoshida, Shigeru; Yuan, Tianlu; Zöcklein, M.; Bezerra, T. J. C.; Birkenfeld, Thilo; Blum, D.; Bongrand, M.; Cabrera, A.; Cheng, Yaping; Depnering, Wilfried; Dötterl, O.; Enqvist, T.; Enzmann, Heike; Genster, Christoph; Grassi, M.; Göttel, Alexandre; Hackspacher, Paul; Hagner, C.; Han, Yang; Heinz, Tobias; Kampmann, Philipp; Kuusiniemi, P.; Lachenmaier, T.; Loo, Kai; Lorenz, Sebastian; Лубсандоржиев, Б.; Ludhová, L.; Malyshkin, Y. M.; Meyhöfer, David; Miramonti, L.; Müller, Axel; Oberauer, L.; Pilarczyk, Oliver; Rebber, Henning; Sawatzki, Julia; Schever, Michaela; Schweizer, Konstantin; Settimo, M.; Sirignano, C.; Smirnov, Mikhail; Stahl, A.; Steiger, Hans; Steinmann, J.; Sterr, Tobias; Stock, Matthias Raphael; Studenikin, Alexander; Tietzsch, Alexander; Trzaska, W. H.; Viaud, B.; Volpe, Cristina; Wang, W.; Wonsak, B.; Wurm, M.; Wysotzki, Christian; Yin, Xuefeng; Ding, X. F.; Yermia, F.

doi:10.1103/physrevd.101.032006

Cited by 46 publications

(43 citation statements)

References 50 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…The analysis achieves an energy resolution of about 25% (30%) at ∼20 GeV for muon-like (cascade-like) events and a median angular resolution of 10°(16°). Full sensitivity to lower neutrino energies, for example to reach the next oscillation minimum at ∼6 GeV, can only be achieved with a denser array, like the proposed PINGU low-energy extension [76].…”

Section: Fig 6 Left Panelmentioning

confidence: 99%

See 1 more Smart Citation

Probing particle physics with IceCube

2018

View full text Add to dashboard Cite

The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov telescope primarily designed for the detection of high-energy astrophysical neutrinos. IceCube became fully operational in 2010, after a seven-year construction phase, and reached a milestone in 2013 by the first observation of cosmic neutrinos in the TeV-PeV energy range. This observation does not only mark an important breakthrough in neutrino astronomy, but it also provides a new probe of particle physics related to neutrino production, mixing, and interaction. In this review we give an overview of the various possibilities how IceCube can address fundamental questions related to the phenomena of neutrino oscillations and interactions, the origin of dark matter, and the existence of exotic relic particles, like monopoles. We will summarize recent results and highlight future avenues.Keywords IceCube · physics beyond the Standard Model · neutrino telescopes · neutrino oscillation · neutrino interactions · sterile neutrinos · dark matter · magnetic monopoles PACS 95.35.+d · 14.80.Hv · 13.15.+g · 14.60.Lm arXiv:1806.05696v1 [astro-ph.HE]

show abstract

Section: Fig 6 Left Panelmentioning

confidence: 99%

“…Note that the full likelihood analysis in [232] used a rather simple energy proxy based on the number of hit DOMs. Better energy reconstruction algorithms being developed within IceCube, particularly at low energies, will further improve the performance of this method [76].…”

Section: Dark Matter Signals From the Sunmentioning

confidence: 99%

Probing particle physics with IceCube

2018

View full text Add to dashboard Cite

show abstract

“…of the future experiments in the field of neutrino physics 6 (see, e.g., refs. [1,62,[67][68][69][70][71]). Data on the absolute neutrino mass scale (or on min(m j )) can be obtained, e.g., from measurements of the spectrum of electrons near the end point in 3 H β-decay experiments [72][73][74] and from cosmological and astrophysical observations.…”

Section: The Three-neutrino Mixingmentioning

confidence: 99%

Discrete flavour symmetries, neutrino mixing and leptonic CP violation

2018

View full text Add to dashboard Cite

The current status of our knowledge of the 3-neutrino mixing parameters and of the CP violation in the lepton sector is summarised. The non-Abelian discrete symmetry approach to understanding the observed pattern of neutrino mixing and the related predictions for neutrino mixing angles and leptonic Dirac CP violation are reviewed. Possible tests of these predictions using the existing data on neutrino mixing angles as well as prospective data from current and future neutrino oscillation experiments (T2K, NOνA, Daya Bay, T2HK, T2HKK, DUNE) are also discussed.

show abstract

“…Dark matter (DM) composes one-fourth of the Universe, however, its essence is still elusive. Many terrestrial detectors are built to reveal the particle nature of DM either from measuring the coupling strength between DM and the Standard Model (SM) particles [1][2][3][4][5][6][7] or the indirect signal from DM annihilation in the space [8][9][10][11][12][13]. But the definitive evidence is yet to come.…”

Section: Introductionmentioning

confidence: 99%

Reheating neutron stars with the annihilation of self-interacting dark matter

Chen¹,

Lin²

2018

J. High Energ. Phys.

View full text Add to dashboard Cite

Compact stellar objects such as neutron stars (NS) are ideal places for capturing dark matter (DM) particles. We study the effect of self-interacting DM (SIDM) captured by nearby NS that can reheat it to an appreciated surface temperature through absorbing the energy released due to DM annihilation. When DM-nucleon cross section σ χn is small enough, DM self-interaction will take over the capture process and make the number of captured DM particles increased as well as the DM annihilation rate. The corresponding NS surface temperature resulted from DM self-interaction is about hundreds of Kelvin and is potentially detectable by the future infrared telescopes. Such observations could act as the complementary probe on DM properties to the current DM direct searches.

show abstract

Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU

Cited by 46 publications

References 50 publications

Probing particle physics with IceCube

Probing particle physics with IceCube

Discrete flavour symmetries, neutrino mixing and leptonic CP violation

Reheating neutron stars with the annihilation of self-interacting dark matter

Contact Info

Product

Resources

About