<p>The existence of an eV-scale sterile neutrino has been proposed to explain several anomalous experimental results obtained over the course of the past 25 years. The first search for such a sterile neutrino conducted with data from KM3NeT/ORCA — a water Cherenkov neutrino telescope under construction at the bottom of the Mediterranean Sea — is reported in this paper. GeV-scale atmospheric neutrino oscillations are measured by reconstructing the energy and arrival direction of up-going neutrinos that have traversed the Earth. This study is based on a data sample containing 5828 neutrino candidates collected with 6 detection units (5% of the complete detector), corresponding to an exposure of 433 kton-years. From the expected effect of an eV-scale sterile neutrino on the first <i>ν</i><sub><i>μ</i></sub> → <i>ν</i><sub><i>τ</i></sub> standard oscillation maximum, simultaneous constraints are put on the magnitude of the <i>U</i><sub><i>μ</i>4</sub> and <i>U</i><sub><i>τ</i>4</sub> mixing elements assuming <InlineEquation ID="IEq1"> <EquationSource Format="MATHML"><math display="inline"> <mi mathvariant="normal">Δ</mi> <msubsup> <mi>m</mi> <mn>41</mn> <mn>2</mn> </msubsup> <mo>≥</mo> <mn>1</mn> </math></EquationSource> <EquationSource Format="TEX">\( \Delta {m}_{41}^2\ge 1 \)</EquationSource> </InlineEquation> eV<sup>2</sup>. The results are compatible with the absence of mixing between active neutrinos and a sterile state, with |<i>U</i><sub><i>μ</i>4</sub>|<sup>2</sup> &lt; 0.138 and |<i>U</i><sub><i>τ</i>4</sub>|<sup>2</sup> &lt; 0.076 at a 90% confidence level. Such constraints are compatible with the results reported by other long-baseline experiments, and indicate that with KM3NeT/ORCA it is possible to bring crucial contributions to sterile neutrino searches in the coming years.</p>

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Search for an eV-scale sterile neutrino with the first six detection units of KM3NeT/ORCA

  • O. Adriani,
  • A. Albert,
  • A. R. Alhebsi,
  • S. Alshalloudi,
  • M. Alshamsi,
  • 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,
  • Y. Becherini,
  • M. Bendahman,
  • F. Benfenati Gualandi,
  • M. Benhassi,
  • D. M. Benoit,
  • Z. Beňušová,
  • E. Berbee,
  • E. Berti,
  • V. Bertin,
  • P. Betti,
  • S. Biagi,
  • M. Boettcher,
  • D. Bonanno,
  • M. Bondì,
  • S. Bottai,
  • A. B. Bouasla,
  • J. Boumaaza,
  • M. Bouta,
  • M. Bouwhuis,
  • C. Bozza,
  • R. M. Bozza,
  • H. Brânzaş,
  • F. Bretaudeau,
  • M. Breuhaus,
  • R. Bruijn,
  • J. Brunner,
  • R. Bruno,
  • E. Buis,
  • R. Buompane,
  • I. Burriel,
  • J. Busto,
  • B. Caiffi,
  • D. Calvo,
  • A. Capone,
  • F. Carenini,
  • V. Carretero,
  • T. Cartraud,
  • P. Castaldi,
  • V. Cecchini,
  • S. Celli,
  • L. Cerisy,
  • 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,
  • 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,
  • T. van Eeden,
  • M. Eff,
  • D. van Eijk,
  • I. El Bojaddaini,
  • S. El Hedri,
  • S. El Mentawi,
  • V. Ellajosyula,
  • A. Enzenhöfer,
  • M. Farino,
  • G. Ferrara,
  • M. D. Filipović,
  • F. Filippini,
  • D. Franciotti,
  • L. A. Fusco,
  • T. Gal,
  • J. García Méndez,
  • A. Garcia Soto,
  • C. Gatius Oliver,
  • N. Geißelbrecht,
  • E. Genton,
  • 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,
  • U. F. Katz,
  • J. Keegans,
  • V. Kikvadze,
  • 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,
  • 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,
  • C. Pastore,
  • A. M. Păun,
  • G. E. Păvălaş,
  • S. Peña Martínez,
  • M. Perrin-Terrin,
  • V. Pestel,
  • M. Petropavlova,
  • P. Piattelli,
  • A. Plavin,
  • C. Poirè,
  • V. Popa,
  • T. Pradier,
  • J. Prado,
  • S. Pulvirenti,
  • C. A. Quiroz-Rangel,
  • 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,
  • J. Seneca,
  • P. A. Sevle Myhr,
  • I. Sgura,
  • R. Shanidze,
  • Chengyu Shao,
  • A. Sharma,
  • Y. Shitov,
  • F. Šimkovic,
  • A. Simonelli,
  • A. Sinopoulou,
  • B. Spisso,
  • M. Spurio,
  • O. Starodubtsev,
  • D. Stavropoulos,
  • I. Štekl,
  • D. Stocco,
  • M. Taiuti,
  • Y. Tayalati,
  • 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,
  • E. de Wolf,
  • I. Lhenry-Yvon,
  • S. Zavatarelli,
  • D. Zito,
  • J. D. Zornoza,
  • J. Zúñiga

摘要

The existence of an eV-scale sterile neutrino has been proposed to explain several anomalous experimental results obtained over the course of the past 25 years. The first search for such a sterile neutrino conducted with data from KM3NeT/ORCA — a water Cherenkov neutrino telescope under construction at the bottom of the Mediterranean Sea — is reported in this paper. GeV-scale atmospheric neutrino oscillations are measured by reconstructing the energy and arrival direction of up-going neutrinos that have traversed the Earth. This study is based on a data sample containing 5828 neutrino candidates collected with 6 detection units (5% of the complete detector), corresponding to an exposure of 433 kton-years. From the expected effect of an eV-scale sterile neutrino on the first νμντ standard oscillation maximum, simultaneous constraints are put on the magnitude of the Uμ4 and Uτ4 mixing elements assuming Δ m 41 2 1 \( \Delta {m}_{41}^2\ge 1 \) eV2. The results are compatible with the absence of mixing between active neutrinos and a sterile state, with |Uμ4|2 < 0.138 and |Uτ4|2 < 0.076 at a 90% confidence level. Such constraints are compatible with the results reported by other long-baseline experiments, and indicate that with KM3NeT/ORCA it is possible to bring crucial contributions to sterile neutrino searches in the coming years.