Table of Contents
Fetching ...

Atmospheric neutrino constraints on Lorentz invariance violation with the first six detection units of KM3NeT/ORCA

KM3NeT Collaboration, O. Adriani, A. Albert, A. R. Alhebsi, S. Alshalloudi, S. Alves Garre, F. Ameli, M. Andre, L. Aphecetche, M. Ardid, S. Ardid, J. Aublin, F. Badaracco, L. Bailly-Salins, B. Baret, A. Bariego-Quintana, L. Barigione, M. Barnard, Y. Becherini, M. Bendahman, F. Benfenati Gualandi, M. Benhassi, D. M. Benoit, Z. Beňušová, E. Berbee, C. van Bergen, E. Berti, V. Bertin, P. Betti, S. Biagi, M. Boettcher, D. Bonanno, M. Bondì, M. Bongi, S. Bottai, A. B. Bouasla, J. Boumaaza, M. Bouta, C. Bozza, R. M. Bozza, H. Brânzaš, F. Bretaudeau, M. Breuhaus, R. Bruijn, J. Brunner, R. Bruno, E. Buis, R. Buompane, I. Burriel, J. Busto, B. Caiffi, D. Calvo, E. G. J. van Campenhout, A. Capone, F. Carenini, V. Carretero, T. Cartraud, P. Castaldi, V. Cecchini, S. Celli, M. Chabab, A. Chen, S. Cherubini, T. Chiarusi, W. Chung, M. Circella, R. Clark, R. Cocimano, J. A. B. Coelho, A. Coleiro, A. Condorelli, R. Coniglione, P. Coyle, A. Creusot, G. Cuttone, R. Dallier, A. De Benedittis, X. de La Bernardie, G. De Wasseige, V. Decoene, P. Deguire, I. Del Rosso, L. S. Di Mauro, I. Di Palma, A. F. Díaz, D. Diego-Tortosa, C. Distefano, A. Domi, C. Donzaud, D. Dornic, E. Drakopoulou, D. Drouhin, J. -G. Ducoin, P. Duverne, R. Dvornický, T. Eberl, E. Eckerová, A. Eddymaoui, M. Eff, D. van Eijk, I. El Bojaddaini, S. El Hedri, S. El Mentawi, V. Ellajosyula, A. Enzenhöfer, M. Farino, A. Ferrara, G. Ferrara, M. D. Filipović, F. Filippini, A. Foisseau, D. Franciotti, L. A. Fusco, S. Gagliardini, T. Gal, J. García Méndez, A. Garcia Soto, C. Gatius Oliver, N. Geißelbrecht, H. Ghaddari, L. Gialanella, B. K. Gibson, E. Giorgio, I. Goos, P. Goswami, S. R. Gozzini, R. Gracia, B. Guillon, C. Haack, C. Hanna, H. van Haren, E. Hazelton, A. Heijboer, L. Hennig, J. J. Hernández-Rey, A. Idrissi, W. Idrissi Ibnsalih, G. Illuminati, R. Jaimes, O. Janik, D. Joly, M. de Jong, P. de Jong, B. J. Jung, P. Kalaczyński, T. Kapoor, U. F. Katz, J. Keegans, T. Khvichia, G. Kistauri, C. Kopper, A. Kouchner, Y. Y. Kovalev, L. Krupa, V. Kueviakoe, V. Kulikovskiy, R. Kvatadze, M. Labalme, R. Lahmann, M. Lamoureux, A. Langella, G. Larosa, C. Lastoria, J. Lazar, A. Lazo, G. Lehaut, V. Lemaître, E. Leonora, N. Lessing, G. Levi, M. Lindsey Clark, F. Longhitano, M. Loup, A. Luashvili, S. Madarapu, F. Magnani, L. Malerba, F. Mamedov, A. Manfreda, A. Manousakis, M. Marconi, A. Margiotta, A. Marinelli, C. Markou, L. Martin, M. Mastrodicasa, S. Mastroianni, J. Mauro, K. C. K. Mehta, G. Miele, P. Migliozzi, E. Migneco, M. L. Mitsou, C. M. Mollo, L. Morales-Gallegos, N. Mori, A. Moussa, I. Mozun Mateo, R. Muller, M. R. Musone, M. Musumeci, S. Navas, A. Nayerhoda, C. A. Nicolau, B. Nkosi, B. Ó Fearraigh, V. Oliviero, A. Orlando, E. Oukacha, L. Pacini, D. Paesani, J. Palacios González, G. Papalashvili, P. Papini, V. Parisi, A. Parmar, G. Pascua, B. Pascual-Estrugo, C. Pastore, A. M. Păun, G. E. Păvălaš, S. Peña Martínez, M. Perrin-Terrin, V. Pestel, M. Petropavlova, P. Piattelli, A. Plavin, C. Poirè, T. Pradier, J. Prado, S. Pulvirenti, N. Randazzo, A. Ratnani, S. Razzaque, I. C. Rea, D. Real, G. Riccobene, J. Robinson, A. Romanov, E. Ros, A. Šaina, F. Salesa Greus, D. F. E. Samtleben, A. Sánchez Losa, S. Sanfilippo, M. Sanguineti, D. Santonocito, P. Sapienza, M. Scaringella, M. Scarnera, J. Schnabel, J. Schumann, M. Senniappan, P. A. Sevle Myhr, I. Sgura, R. Shanidze, Chengyu Shao, A. Sharma, Y. Shitov, F. Šimkovic, A. Simonelli, A. Sinopoulou, C. Sironneau, B. Spisso, M. Spurio, O. Starodubtsev, I. Štekl, D. Stocco, M. Taiuti, Y. Tayalati, J. Tena, H. Thiersen, S. Thoudam, I. Tosta e Melo, B. Trocmé, V. Tsourapis, C. Tully, E. Tzamariudaki, A. Ukleja, A. Vacheret, V. Valsecchi, V. Van Elewyck, G. Vannoye, E. Vannuccini, G. Vasileiadis, F. Vazquez de Sola, A. Veutro, S. Viola, D. Vivolo, A. van Vliet, L. Voorend, E. de Wolf, I. Lhenry-Yvon, S. Zavatarelli, D. Zito, J. D. Zornoza, J. Zúñiga

Abstract

Lorentz invariance is a fundamental symmetry underlying both the Standard Model of particle physics and General Relativity. Testing its validity provides a direct means of searching for new physics emerging near the Planck scale. A search for isotropic Lorentz invariance violation with 1.4 years of atmospheric neutrino data collected by a partial configuration of the KM3NeT/ORCA detector comprising six detection units is presented. No evidence for such violation is found; thus, competitive limits are set on a subset of isotropic Lorentz invariance violating coefficients, which complement and extend existing experimental constraints.

Atmospheric neutrino constraints on Lorentz invariance violation with the first six detection units of KM3NeT/ORCA

Abstract

Lorentz invariance is a fundamental symmetry underlying both the Standard Model of particle physics and General Relativity. Testing its validity provides a direct means of searching for new physics emerging near the Planck scale. A search for isotropic Lorentz invariance violation with 1.4 years of atmospheric neutrino data collected by a partial configuration of the KM3NeT/ORCA detector comprising six detection units is presented. No evidence for such violation is found; thus, competitive limits are set on a subset of isotropic Lorentz invariance violating coefficients, which complement and extend existing experimental constraints.
Paper Structure (14 sections, 10 equations, 6 figures, 3 tables)

This paper contains 14 sections, 10 equations, 6 figures, 3 tables.

Figures (6)

  • Figure 1: Muon neutrino survival probability as a function of neutrino energy. The neutrino is assumed to have traversed the Earth with a baseline $L \simeq D_{\oplus}$. The effect of mass dimension $d = 3$ coefficients is illustrated in the left panel using different values of $\mathring{a}_{\mu\tau}^{(3)}$ as an example. The $d>3$ case is shown in the right panel, with $\mathring{c}_{\mu\tau}^{(4)}$ being chosen as a representative example. The values for $\mathring{a}_{\mu\tau}^{(3)}$ and $\mathring{c}_{\mu\tau}^{(4)}$ are the 90% (orange) and 99% (red) confidence level (CL) constraints reported by the IceCube collaboration in IC2yrLIV. The oscillation probabilities are computed using OscProb oscprob.
  • Figure 2: Muon neutrino survival probability as a function of neutrino energy. The neutrino is assumed to have traversed the Earth with a baseline $L \simeq D_{\oplus}$. The left panel shows the effect of a nonzero $\mathring{k}_{ee}^{(d)}$, while the right panel illustrates the effect of a nonzero $\mathring{k}_{\mu\mu}^{(d)}$ and $- \mathring{k}_{\tau\tau}^{(d)}$, respectively. Mass dimension $d=3$ has been chosen as a representative example, using a coefficient value suitable for an illustration of LIV effects. The oscillation probabilities are computed using OscProb oscprob.
  • Figure 3: Two-dimensional sensitivities for the magnitude and phase of $d=3$ off-diagonal coefficients. The 95% confidence level contour is shown in each panel.
  • Figure 4: Likelihood ratio scans for $d=3$ off-diagonal coefficients. The intersections with the dashed lines define the upper limits.
  • Figure 5: Likelihood-ratio scans for diagonal coefficient combinations across $d = 3, \dots, 8$. The blue dot in each panel indicates the respective best-fit point for that dimension. The intersections with the dashed lines define the upper limits.
  • ...and 1 more figures