Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA

Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA

KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile...

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Veröffentlicht in:arXiv.org 2021-11
Hauptverfasser: Albert, A, Aly, Z, Anguita, M, Anton, G, Ardid, M, Benfenati, F, A M van den Berg, Bertin, V, Biagi, S, Bouta, M, Bouwhuis, M, Bozza, C, Bretaudeau, F, Brunner, J, Buis, E, Busto, J, Castaldi, P, Celli, S, Circella, M, Coelho, J A B, Colomer Mollac, M, Cuttone, G, De Martino, B, Díaz, A F, Dorr, M, Drouhin, D, T van Eeden, I El Bojaddaini, Enzenhofer, A, Fermani, P, Ferrara, G, Filipovic, M D, Gal, T, Gatelet, Y, Gialanella, L, Gozzini, S R, Graf, K, Grella, G, Guderian, D, Gutierrez, M, Haefner, J, Hamdaoui, H, Heijboer, A, Hekalo, A, Hennig, L, Hernandez-Rey, J J, Huang, F, W Idrissi Ibnsalih, Illuminati, G, Kalekin, O, Khan Chowdhury, N R, Kistauri, G, Kulikovskiy, V, Lahmann, R, Lastoria, C, Leone, F, Lessing, N, Lincetto, M, M Lindsey Clark, Lipreau, T, Longhitano, F, Lygda, A, Mannheim, K, Margiotta, A, Marzaioli, F, Miele, G, Mollo, C M, Moser, M, Moussa, A, Muller, R, Musumeci, M, Navas, S, Nkosi, B, O'Sullivan, M, Organokov, M, Orlando, A, Păun, A M, Pellegrino, C, Poirè, C, Pradier, T, Probst, I, Real, D, Romanov, A, Samtleben, D F E, Sanguineti, M, Schneider, M F, Schumann, J, Seneca, J, Sharma, A, Spurio, M, Stavropoulos, D, Thakore, T, Thiersen, H, Tzamariudaki, E, V Van Elewyck, Versari, F, Wojaczyński, R, Zavatarelli, S, Zegarelli, A, Zúñiga, J
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Sprache:eng
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Anomalies
Cosmology
Hypotheses
Neutrinos
Parameter sensitivity
Sensitivity
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creator Albert, A
Aly, Z
Anguita, M
Anton, G
Ardid, M
Benfenati, F
A M van den Berg
Bertin, V
Biagi, S
Bouta, M
Bouwhuis, M
Bozza, C
Bretaudeau, F
Brunner, J
Buis, E
Busto, J
Castaldi, P
Celli, S
Circella, M
Coelho, J A B
Colomer Mollac, M
Cuttone, G
De Martino, B
Díaz, A F
Dorr, M
Drouhin, D
T van Eeden
I El Bojaddaini
Enzenhofer, A
Fermani, P
Ferrara, G
Filipovic, M D
Gal, T
Gatelet, Y
Gialanella, L
Gozzini, S R
Graf, K
Grella, G
Guderian, D
Gutierrez, M
Haefner, J
Hamdaoui, H
Heijboer, A
Hekalo, A
Hennig, L
Hernandez-Rey, J J
Huang, F
W Idrissi Ibnsalih
Illuminati, G
Kalekin, O
Khan Chowdhury, N R
Kistauri, G
Kulikovskiy, V
Lahmann, R
Lastoria, C
Leone, F
Lessing, N
Lincetto, M
M Lindsey Clark
Lipreau, T
Longhitano, F
Lygda, A
Mannheim, K
Margiotta, A
Marzaioli, F
Miele, G
Mollo, C M
Moser, M
Moussa, A
Muller, R
Musumeci, M
Navas, S
Nkosi, B
O'Sullivan, M
Organokov, M
Orlando, A
Păun, A M
Pellegrino, C
Poirè, C
Pradier, T
Probst, I
Real, D
Romanov, A
Samtleben, D F E
Sanguineti, M
Schneider, M F
Schumann, J
Seneca, J
Sharma, A
Spurio, M
Stavropoulos, D
Thakore, T
Thiersen, H
Tzamariudaki, E
V Van Elewyck
Versari, F
Wojaczyński, R
Zavatarelli, S
Zegarelli, A
Zúñiga, J
description KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles \(\theta_{14}\), \(\theta_{24}\), \(\theta_{34}\) and the effective angle \(\theta_{\mu e}\), over a broad range of mass squared difference \(\Delta m^2_{41} \sim [10^{-5}, 10]\) \(\rm{eV}^2\), allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements.
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KM3NeT/ORCA</title><title>arXiv.org</title><description>KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles \(\theta_{14}\), \(\theta_{24}\), \(\theta_{34}\) and the effective angle \(\theta_{\mu e}\), over a broad range of mass squared difference \(\Delta m^2_{41} \sim [10^{-5}, 10]\) \(\rm{eV}^2\), allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements.</description><subject>Anomalies</subject><subject>Cosmology</subject><subject>Hypotheses</subject><subject>Neutrinos</subject><subject>Parameter sensitivity</subject><subject>Sensitivity</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNys0KgkAUQOEhCJLyHS60lmxGnbYhhRAVlHtxcdMrOtrMtZ-3r0UP0OosvjMRnlRqHWwiKWfCd64Jw1AmWsax8kR2ReOI6UH8Bu6hpapmcIyWWgSDI1syPXT0IlPBUNqywy86eBLXcDiqE-ar8yXdLsT0VrYO_V_nYrnf5WkWDLa_j-i4aPrRmi8VMo601lJFifrv-gBW9zvf</recordid><startdate>20211123</startdate><enddate>20211123</enddate><creator>Albert, A</creator><creator>Aly, Z</creator><creator>Anguita, M</creator><creator>Anton, 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20211123</creationdate><title>Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA</title><author>Albert, A ; Aly, Z ; Anguita, M ; Anton, G ; Ardid, M ; Benfenati, F ; A M van den Berg ; Bertin, V ; Biagi, S ; Bouta, M ; Bouwhuis, M ; Bozza, C ; Bretaudeau, F ; Brunner, J ; Buis, E ; Busto, J ; Castaldi, P ; Celli, S ; Circella, M ; Coelho, J A B ; Colomer Mollac, M ; Cuttone, G ; De Martino, B ; Díaz, A F ; Dorr, M ; Drouhin, D ; T van Eeden ; I El Bojaddaini ; Enzenhofer, A ; Fermani, P ; Ferrara, G ; Filipovic, M D ; Gal, T ; Gatelet, Y ; Gialanella, L ; Gozzini, S R ; Graf, K ; Grella, G ; Guderian, D ; Gutierrez, M ; Haefner, J ; Hamdaoui, H ; Heijboer, A ; Hekalo, A ; Hennig, L ; Hernandez-Rey, J J ; Huang, F ; W Idrissi Ibnsalih ; Illuminati, G ; Kalekin, O ; Khan Chowdhury, N R ; Kistauri, G ; Kulikovskiy, V ; Lahmann, R ; Lastoria, C ; Leone, F ; Lessing, N ; Lincetto, M ; M Lindsey Clark ; Lipreau, T ; Longhitano, F ; Lygda, A ; Mannheim, K ; Margiotta, A ; Marzaioli, F ; Miele, G ; Mollo, C M ; Moser, M ; Moussa, A ; Muller, R ; Musumeci, M ; Navas, S ; Nkosi, B ; O'Sullivan, M ; Organokov, M ; Orlando, A ; Păun, A M ; Pellegrino, C ; Poirè, C ; Pradier, T ; Probst, I ; Real, D ; Romanov, A ; Samtleben, D F E ; Sanguineti, M ; Schneider, M F ; Schumann, J ; Seneca, J ; Sharma, A ; Spurio, M ; Stavropoulos, D ; Thakore, T ; Thiersen, H ; Tzamariudaki, E ; V Van Elewyck ; Versari, F ; Wojaczyński, R ; Zavatarelli, S ; Zegarelli, A ; Zúñiga, J</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_25477723463</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>Anomalies</topic><topic>Cosmology</topic><topic>Hypotheses</topic><topic>Neutrinos</topic><topic>Parameter sensitivity</topic><topic>Sensitivity</topic><toplevel>online_resources</toplevel><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>Aly, Z</creatorcontrib><creatorcontrib>Anguita, M</creatorcontrib><creatorcontrib>Anton, G</creatorcontrib><creatorcontrib>Ardid, M</creatorcontrib><creatorcontrib>Benfenati, F</creatorcontrib><creatorcontrib>A M van den Berg</creatorcontrib><creatorcontrib>Bertin, V</creatorcontrib><creatorcontrib>Biagi, S</creatorcontrib><creatorcontrib>Bouta, M</creatorcontrib><creatorcontrib>Bouwhuis, M</creatorcontrib><creatorcontrib>Bozza, C</creatorcontrib><creatorcontrib>Bretaudeau, 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N</creatorcontrib><creatorcontrib>Lincetto, M</creatorcontrib><creatorcontrib>M Lindsey Clark</creatorcontrib><creatorcontrib>Lipreau, T</creatorcontrib><creatorcontrib>Longhitano, F</creatorcontrib><creatorcontrib>Lygda, A</creatorcontrib><creatorcontrib>Mannheim, K</creatorcontrib><creatorcontrib>Margiotta, A</creatorcontrib><creatorcontrib>Marzaioli, F</creatorcontrib><creatorcontrib>Miele, G</creatorcontrib><creatorcontrib>Mollo, C M</creatorcontrib><creatorcontrib>Moser, M</creatorcontrib><creatorcontrib>Moussa, A</creatorcontrib><creatorcontrib>Muller, R</creatorcontrib><creatorcontrib>Musumeci, M</creatorcontrib><creatorcontrib>Navas, S</creatorcontrib><creatorcontrib>Nkosi, B</creatorcontrib><creatorcontrib>O'Sullivan, M</creatorcontrib><creatorcontrib>Organokov, M</creatorcontrib><creatorcontrib>Orlando, A</creatorcontrib><creatorcontrib>Păun, A M</creatorcontrib><creatorcontrib>Pellegrino, C</creatorcontrib><creatorcontrib>Poirè, C</creatorcontrib><creatorcontrib>Pradier, 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Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Albert, A</au><au>Aly, Z</au><au>Anguita, M</au><au>Anton, G</au><au>Ardid, M</au><au>Benfenati, F</au><au>A M van den Berg</au><au>Bertin, V</au><au>Biagi, S</au><au>Bouta, M</au><au>Bouwhuis, M</au><au>Bozza, C</au><au>Bretaudeau, F</au><au>Brunner, J</au><au>Buis, E</au><au>Busto, J</au><au>Castaldi, P</au><au>Celli, S</au><au>Circella, M</au><au>Coelho, J A B</au><au>Colomer Mollac, M</au><au>Cuttone, G</au><au>De Martino, B</au><au>Díaz, A F</au><au>Dorr, M</au><au>Drouhin, D</au><au>T van Eeden</au><au>I El Bojaddaini</au><au>Enzenhofer, A</au><au>Fermani, P</au><au>Ferrara, G</au><au>Filipovic, M D</au><au>Gal, T</au><au>Gatelet, Y</au><au>Gialanella, L</au><au>Gozzini, S R</au><au>Graf, K</au><au>Grella, G</au><au>Guderian, D</au><au>Gutierrez, M</au><au>Haefner, J</au><au>Hamdaoui, H</au><au>Heijboer, A</au><au>Hekalo, A</au><au>Hennig, L</au><au>Hernandez-Rey, J J</au><au>Huang, F</au><au>W Idrissi Ibnsalih</au><au>Illuminati, G</au><au>Kalekin, O</au><au>Khan Chowdhury, N R</au><au>Kistauri, G</au><au>Kulikovskiy, V</au><au>Lahmann, R</au><au>Lastoria, C</au><au>Leone, F</au><au>Lessing, N</au><au>Lincetto, M</au><au>M Lindsey Clark</au><au>Lipreau, T</au><au>Longhitano, F</au><au>Lygda, A</au><au>Mannheim, K</au><au>Margiotta, A</au><au>Marzaioli, F</au><au>Miele, G</au><au>Mollo, C M</au><au>Moser, M</au><au>Moussa, A</au><au>Muller, R</au><au>Musumeci, M</au><au>Navas, S</au><au>Nkosi, B</au><au>O'Sullivan, M</au><au>Organokov, M</au><au>Orlando, A</au><au>Păun, A M</au><au>Pellegrino, C</au><au>Poirè, C</au><au>Pradier, T</au><au>Probst, I</au><au>Real, D</au><au>Romanov, A</au><au>Samtleben, D F E</au><au>Sanguineti, M</au><au>Schneider, M F</au><au>Schumann, J</au><au>Seneca, J</au><au>Sharma, A</au><au>Spurio, M</au><au>Stavropoulos, D</au><au>Thakore, T</au><au>Thiersen, H</au><au>Tzamariudaki, E</au><au>V Van Elewyck</au><au>Versari, F</au><au>Wojaczyński, R</au><au>Zavatarelli, S</au><au>Zegarelli, A</au><au>Zúñiga, J</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA</atitle><jtitle>arXiv.org</jtitle><date>2021-11-23</date><risdate>2021</risdate><eissn>2331-8422</eissn><abstract>KM3NeT/ORCA is a next-generation neutrino telescope optimised for atmospheric neutrino oscillations studies. In this paper, the sensitivity of ORCA to the presence of a light sterile neutrino in a 3+1 model is presented. After three years of data taking, ORCA will be able to probe the active-sterile mixing angles \(\theta_{14}\), \(\theta_{24}\), \(\theta_{34}\) and the effective angle \(\theta_{\mu e}\), over a broad range of mass squared difference \(\Delta m^2_{41} \sim [10^{-5}, 10]\) \(\rm{eV}^2\), allowing to test the eV-mass sterile neutrino hypothesis as the origin of short baseline anomalies, as well as probing the hypothesis of a very light sterile neutrino, not yet constrained by cosmology. ORCA will be able to explore a relevant fraction of the parameter space not yet reached by present measurements.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record>
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subjects Anomalies
Cosmology
Hypotheses
Neutrinos
Parameter sensitivity
Sensitivity
title Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
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