Neutrino non-standard interactions with theKM3NeT/ORCA detector

Mańczak, J.; Khan-Chowdhury, N. R.; Hernández-Rey, J. J.; Navas, S.; Ageron, M.; Aiello, S.; Albert, Arnauld; Alshamsi, Maitha; Garre, S. Alves; Aly, Z.; Ambrosone, Antonio; Ameli, F.; André, M.; Androulakis, G.; Anghinolfi, M.; Anguita, M.; Anton, Gisela; Ardid, M.; Ardid, Salva; Assal, William; Aublin, J.; Bagatelas, C.; Baret, B.; Pree, S. Başeğmez du; Bendahman, M.; Benfenati, F.; Berbee, E.; Berg, Ad van den; Bertín, V.; Beurthey, S.; Beveren, V. van; Biagi, S.; Billault, M.; Bissinger, M.; Boettcher, Markus; Cabo, Manuel Bou; Boumaaza, J.; Bouta, M.; Boutonnet, C.; Bouvet, Gilles; Bouwhuis, M. C.; Bozza, C.; Brânzaş, H.; Bruijn, R.; Brunner, J.; Bruno, Riccardo; Buis, E. J.; Buompane, R.; Busto, J.; Caiffi, B.; Caillat, L.; Calvo, David; Campion, S.; Capone, A.; Carduner, Hervé; Carretero, V.; Castaldi, Paolo; Celli, S.; Cereseto, R.; Chabab, M.; Champion, C.; Chau, N.; Chen, Andrew; Cherubini, S.; Chiarella, V.; Chiarusi, T.; Circella, M.; Cocimano, R.; Coelho, J. A. B.; Coleiro, A.; Colomer-Molla, M.; Colonges, S.; Coniglione, R.; Cosquer, A.; Coyle, P.; Cresta, Massimiliano; Creusot, A.; Cruz, Anvil; Cuttone, G.; D’Amico, Antonio; Dallier, R.; Martino, B. De; Palma, M. De; Palma, I. Di; Diaz, Antonio; Diego-Tortosa, D.; Distefano, C.; Domi, Alba; Donzaud, C.; Dornic, D.; Doerr, Manuel; Drouhin, D.; Eberl, Thomas; Eddyamoui, A.; Eeden, T. van; Eijk, D. van; Bojaddaini, I. El; Eljarrari, Hassnae; Elsäesser, D.; Enzenhoefer, Alexander; Espinosa, V.; Fermani, P.; Ferrara, G.; Filipović, Miroslav; Filippini, F.; Fransen, Jean-Paul; Fusco, L.; Gajanana, D.; Gal, T.; Méndez, J. García; Garcia, A.; Garcon, Evelyne; Garufi, F.; Oliver, Clara Gatius; Geißelbrecht, N.; Gialanella, L.; Giorgio, Emidio; Gozzini, S. R.; Gracía, R.; Graf, Κ.; Grella, G.; Guderian, D.; Guidi, C.; Guillon, B.; Gutiérrez, Miguel; Haefner, Julia; Hallmann, S.; Hamdaoui, H.; Haren, Hans van; Heijboer, A.; Hekalo, A.; Hennig, L.; Henry, S.; Hofestaedt, Jannik; Huang, F.; Ibnsalih, W. Idrissi; Ilioni, Alin; Illuminati, G.; James, C. W.; Janezashvili, D.; Jansweijer, P.; Jong, M. de; Jong, P. de; Jung, B. J.; Kadler, M.; Kalaczyński, P.; Kalekin, O.; Katz, U.; Kayzel, F.E.; Keller, Pascale; Kistauri, G.; Knaap, F. van der; Kooijman, P.; Kouchner, A.; Kreter, M.; Kulikovskiy, V.; Labalme, M.; Lagier, P.; Lahmann, R.; Lamare, P.; Lamoureux, Mathieu; Larosa, G.; Lastoria, C.; Laurence, Jerome M.; Lazo, Alfonso; Breton, R. Le; Guirriec, E. Le; Stum, S. Le; Lehaut, G.; Leonardi, O.; Leone, F.; Leonora, E.; Lerouvillois, Christophe; Lesrel, J.; Lessing, N.; Levi, G.; Lincetto, Massimiliano; Clark, M. Lindsey; Lipreau, T.; Alvarez, Carlos LLorens; Lonardo, A.; Longhitano, F.; Coto, Daniel López; Lumb, N.; Maderer, L.; Majumdar, Jhilik; Margiotta, A.; Marinelli, A.; Marini, A.; Markou, C.; Martin, L.; Martínez-Mora, J. A.; Martini, A.; Marzaioli, Fabio; Mastroianni, S.; Melis, K.; Miele, Gennaro; Migliozzi, P.; Migneco, E.; Mijakowski, P.; Palacios, Luis Salvador Miranda; Mollo, C.M.; Mongelli, M.; Moussa, A.; Müller, R.; Musico, P.; Musumeci, M.; Nauta, L.; Nicolau, C. A.; Nkosi, B.; O’Fearraigh, B.; O’Sullivan, Mitchell; Orlando, A.; Ottonello, G.; Ottonello, Stefano; González, J. Palacios; Papalashvili, G.; Papaleo, R.; Pastore, C.; Păun, A.; Păvălaş, G. E.; Pellegrini, G.; Pellegrino, C.; Perrin-Terrin, M.; Pestel, V.; Piattelli, P.; Pieterse, C.; Pisanti, O.; Poirè, C.; Popa, V.; Pradier, T.; Pratolongo, F.; Probst, Isabella; Puehlhofer, G.; Pulvirenti, S.; Quéméner, Gilles; Randazzo, N.; Rapicavoli, Antonio; Razzaque, S.; Real, D.; Reck, S.; Riccobene, G.; Rigalleau, Louis-Marie; Romanov, A.; Rovelli, A.; Royon, Jérôme; Greus, F. Salesa; Samtleben, D. F. E.; Losa, A. Sánchez; Sanguineti, M.; Santangelo, A.; Santonocito, D.; Sapienza, P.; Schmelling, Jan-Willem; Schnabel, J.; Schneider, Martin Friedrich; Schümann, J.; Schutte, H. M.; Seneca, J.; Sgura, I.; Shanidze, R.; Sharma, Ankur; Sinopoulou, A.; Spisso, B.; Spurio, M.; Stavropoulos, D.; Steijger, J. J. M.; Stellacci, Simona Maria; Taiuti, M.; Tatone, Francesca; Tayalati, Y.; Tenllado, E.; Tézier, D.; Thakore, T.; Theraube, Stephane; Thiersen, Hannes; Timmer, P.; Tingay, Steven; Tsagkli, S.; Tsourapis, V.; Tzamariudaki, E.; Tzanetatos, D.; Valieri, C.; Elewyck, V. Van; Vasileiadis, G.; Versari, F.; Viola, Salvatore; Vivolo, D.; Wasseige, Gwenhaël de; Wilms, J.; Wojaczyński, R.; Wolf, E. de; Yousfi, T.; Zavatarelli, S.; Zegarelli, A.; Zito, D.; Zornoza, J. D.; Zúñiga, J.; Żywucka, N.; NeT, Km

doi:10.22323/1.395.1165

Cited by 5 publications

(4 citation statements)

References 2 publications

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“…A version with six lines has been taking data since more than one year. A preliminary study [56] restricted to the ε µτ parameter shows that the sensitivity is just a factor 4 worse than the current best limits, i.e limits around 10 −2 for this parameter could be achieved with such a small detector (5% of the full ORCA) and with just one year of data. The analysis with real data is ongoing and results will be soon obtained.…”

Section: Neutrino Physics and Search For New Physicsmentioning

confidence: 85%

Science with Neutrino Telescopes in Spain

et al. 2022

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The primary scientific goal of neutrino telescopes is the detection and study of cosmic neutrino signals. However, the range of physics topics that these instruments can tackle is exceedingly wide and diverse. Neutrinos coming from outside the Earth, in association with other messengers, can contribute to clarify the question of the mechanisms that power the astrophysical accelerators which are known to exist from the observation of high-energy cosmic and gamma rays. Cosmic neutrinos can also be used to bring relevant information about the nature of dark matter, to study the intrinsic properties of neutrinos and to look for physics beyond the Standard Model. Likewise, atmospheric neutrinos can be used to study an ample variety of particle physics issues, such as neutrino oscillation phenomena, the determination of the neutrino mass ordering, non-standard neutrino interactions, neutrino decays and a diversity of other physics topics. In this article, we review a selected number of these topics, chosen on the basis of their scientific relevance and the involvement in their study of the Spanish physics community working in the KM3NeT and ANTARES neutrino telescopes.

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Section: Neutrino Physics and Search For New Physicsmentioning

confidence: 85%

Science with Neutrino Telescopes in Spain

et al. 2022

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“…[30,31]. Nevertheless, the strongest bounds on several NSI parameters can be expected from future atmospheric neutrino experiments [85].…”

Section: Discussionmentioning

confidence: 99%

Improved sensitivities of ESS$ν$SB from a two-detector fit

Capozzi¹,

Giunti²,

Ternes³

2023

Preprint

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We discuss the improvement of the sensitivity of ESSνSB to the discovery of CP violation and to new neutrino physics which can be obtained with a two-detector fit of the data of the near and far detectors. In particular, we consider neutrino non-standard interactions generated by very heavy vector mediators, nonunitary neutrino mixing, and neutrino oscillations due to the mixing of the ordinary active neutrinos with a light sterile neutrino. Contents I. Introduction 1 II. Simulation details 2 III. CP-sensitivity 2 IV. Non-standard interactions 3 V. Nonunitary neutrino mixing 4 VI. Light sterile neutrinos 9 VII. Summary and conclusions 11 References 12

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“…Other BSM scenarios can be also tested with ORCA detector. In particular, competitive sensitivities to NSI and invisible neutrino decay can already be achieved with partial configurations of the detector [578,579]. When completed, the ORCA detector will potentially become a leading tool for probing these models.…”

Section: Orcamentioning

confidence: 99%