Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope

The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoi...

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Veröffentlicht in:	arXiv.org 2012-07
Hauptverfasser:	ANTARES collaboration, Adrian-Martinez, S, Albert, A, Andre, M, Anvar, S, Ardid, M, Astraatmadja, T, J -J Aubert, Basa, S, Biagi, S, Bigongiari, C, Bogazzi, C, Bou-Cabo, M, Brunner, J, Busto, J, Carloganu, C, Carr, J, Charif, Z, Charvis, Ph, Chiarusi, T, Circella, M, Coniglione, R, Costantini, H, Coyle, P, Creusot, A, De Bonis, G, Decowski, M P, Distefano, C, Donzaud, C, Dornic, D, Dorosti, Q, Drouhin, D, Eberl, T, Enzenhoefer, A, J -P Ernenwein, Escoffier, S, Fermani, P, Ferry, S, Folger, F, Fritsch, U, Galata, S, Gay, P, Giacomelli, G, Giordano, V, Gleixner, A, Gomez-Gonzalez, J P, Hamal, M, H van Haren, Hello, Y, Hernandez-Rey, J J, Hoessl, J, de Jong, M, Kadler, M, Kooijman, P, Kopper, C, Kreykenbohm, I, Kulikovskiy, V, Lambard, G, Larosa, G, Lattuada, D, D Lo Presti, Louis, F, Mangano, S, Marcelin, M, Margiotta, A, Martinez-Mora, J A, Meli, A, Montaruli, T, Morganti, M, Moscoso, L, Nezri, E, Pavalas, G E, Piattelli, P, Popa, V, Racca, C, Reed, C, Riccobene, G, Riviere, C, Roensch, K, Ruiz-Rivas, J, Russo, G V, Samtleben, D F E, Sanchez-Losa, A, Sapienza, P, Schoeck, F, J -P Schuller, Shanidze, R, Simeone, F, Spies, A, Spurio, M, Stolarczyk, Th, Taiuti, M, Trovato, A, Vallage, B, V Van Elewyck, Vecchi, M, Vernin, P, Wijnker, G, Wilms, J, de Wolf, E
Format:	Artikel
Sprache:	eng
Schlagworte:	Muons Neutrinos Oscillations Parameters Physics - High Energy Physics - Experiment Tracks (paths)
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creator	ANTARES collaboration Adrian-Martinez, S Albert, A Andre, M Anvar, S Ardid, M Astraatmadja, T J -J Aubert Basa, S Biagi, S Bigongiari, C Bogazzi, C Bou-Cabo, M Brunner, J Busto, J Carloganu, C Carr, J Charif, Z Charvis, Ph Chiarusi, T Circella, M Coniglione, R Costantini, H Coyle, P Creusot, A De Bonis, G Decowski, M P Distefano, C Donzaud, C Dornic, D Dorosti, Q Drouhin, D Eberl, T Enzenhoefer, A J -P Ernenwein Escoffier, S Fermani, P Ferry, S Folger, F Fritsch, U Galata, S Gay, P Giacomelli, G Giordano, V Gleixner, A Gomez-Gonzalez, J P Hamal, M H van Haren Hello, Y Hernandez-Rey, J J Hoessl, J de Jong, M Kadler, M Kooijman, P Kopper, C Kreykenbohm, I Kulikovskiy, V Lambard, G Larosa, G Lattuada, D D Lo Presti Louis, F Mangano, S Marcelin, M Margiotta, A Martinez-Mora, J A Meli, A Montaruli, T Morganti, M Moscoso, L Nezri, E Pavalas, G E Piattelli, P Popa, V Racca, C Reed, C Riccobene, G Riviere, C Roensch, K Ruiz-Rivas, J Russo, G V Samtleben, D F E Sanchez-Losa, A Sapienza, P Schoeck, F J -P Schuller Shanidze, R Simeone, F Spies, A Spurio, M Stolarczyk, Th Taiuti, M Trovato, A Vallage, B V Van Elewyck Vecchi, M Vernin, P Wijnker, G Wilms, J de Wolf, E
description	The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximum mixing, a mass difference of $\Delta m_{32}^2=(3.1\pm 0.9)\cdot 10^{-3}$ eV$^2$ is obtained, in good agreement with the world average value.
doi_str_mv	10.48550/arxiv.1206.0645
format	Article
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Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximum mixing, a mass difference of $\Delta m_{32}^2=(3.1\pm 0.9)\cdot 10^{-3}$ eV$^2$ is obtained, in good agreement with the world average value.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.1206.0645</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Muons ; Neutrinos ; Oscillations ; Parameters ; Physics - High Energy Physics - Experiment ; Tracks (paths)</subject><ispartof>arXiv.org, 2012-07</ispartof><rights>2012. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,782,786,887,27934</link.rule.ids><backlink>$$Uhttps://doi.org/10.48550/arXiv.1206.0645$$DView paper in arXiv$$Hfree_for_read</backlink><backlink>$$Uhttps://doi.org/10.1016/j.physletb.2012.07.002$$DView published paper (Access to full text may be restricted)$$Hfree_for_read</backlink></links><search><creatorcontrib>ANTARES collaboration</creatorcontrib><creatorcontrib>Adrian-Martinez, S</creatorcontrib><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>Andre, M</creatorcontrib><creatorcontrib>Anvar, 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J</creatorcontrib><creatorcontrib>Hoessl, J</creatorcontrib><creatorcontrib>de Jong, M</creatorcontrib><creatorcontrib>Kadler, M</creatorcontrib><creatorcontrib>Kooijman, P</creatorcontrib><creatorcontrib>Kopper, C</creatorcontrib><creatorcontrib>Kreykenbohm, I</creatorcontrib><creatorcontrib>Kulikovskiy, V</creatorcontrib><creatorcontrib>Lambard, G</creatorcontrib><creatorcontrib>Larosa, G</creatorcontrib><creatorcontrib>Lattuada, D</creatorcontrib><creatorcontrib>D Lo Presti</creatorcontrib><creatorcontrib>Louis, F</creatorcontrib><creatorcontrib>Mangano, S</creatorcontrib><creatorcontrib>Marcelin, M</creatorcontrib><creatorcontrib>Margiotta, A</creatorcontrib><creatorcontrib>Martinez-Mora, J A</creatorcontrib><creatorcontrib>Meli, A</creatorcontrib><creatorcontrib>Montaruli, T</creatorcontrib><creatorcontrib>Morganti, M</creatorcontrib><creatorcontrib>Moscoso, L</creatorcontrib><creatorcontrib>Nezri, E</creatorcontrib><creatorcontrib>Pavalas, G E</creatorcontrib><creatorcontrib>Piattelli, P</creatorcontrib><creatorcontrib>Popa, V</creatorcontrib><creatorcontrib>Racca, C</creatorcontrib><creatorcontrib>Reed, C</creatorcontrib><creatorcontrib>Riccobene, G</creatorcontrib><creatorcontrib>Riviere, C</creatorcontrib><creatorcontrib>Roensch, K</creatorcontrib><creatorcontrib>Ruiz-Rivas, J</creatorcontrib><creatorcontrib>Russo, G V</creatorcontrib><creatorcontrib>Samtleben, D F E</creatorcontrib><creatorcontrib>Sanchez-Losa, A</creatorcontrib><creatorcontrib>Sapienza, P</creatorcontrib><creatorcontrib>Schoeck, F</creatorcontrib><creatorcontrib>J -P Schuller</creatorcontrib><creatorcontrib>Shanidze, R</creatorcontrib><creatorcontrib>Simeone, F</creatorcontrib><creatorcontrib>Spies, A</creatorcontrib><creatorcontrib>Spurio, M</creatorcontrib><creatorcontrib>Stolarczyk, Th</creatorcontrib><creatorcontrib>Taiuti, M</creatorcontrib><creatorcontrib>Trovato, A</creatorcontrib><creatorcontrib>Vallage, B</creatorcontrib><creatorcontrib>V Van Elewyck</creatorcontrib><creatorcontrib>Vecchi, M</creatorcontrib><creatorcontrib>Vernin, P</creatorcontrib><creatorcontrib>Wijnker, G</creatorcontrib><creatorcontrib>Wilms, J</creatorcontrib><creatorcontrib>de Wolf, E</creatorcontrib><title>Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope</title><title>arXiv.org</title><description>The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximum mixing, a mass difference of $\Delta m_{32}^2=(3.1\pm 0.9)\cdot 10^{-3}$ eV$^2$ is obtained, in good agreement with the world average value.</description><subject>Muons</subject><subject>Neutrinos</subject><subject>Oscillations</subject><subject>Parameters</subject><subject>Physics - High Energy Physics - Experiment</subject><subject>Tracks 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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><scope>GOX</scope></search><sort><creationdate>20120702</creationdate><title>Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope</title><author>ANTARES collaboration ; Adrian-Martinez, S ; Albert, A ; Andre, M ; Anvar, S ; Ardid, M ; Astraatmadja, T ; J -J Aubert ; Basa, S ; Biagi, S ; Bigongiari, C ; Bogazzi, C ; Bou-Cabo, M ; Brunner, J ; Busto, J ; Carloganu, C ; Carr, J ; Charif, Z ; Charvis, Ph ; Chiarusi, T ; Circella, M ; Coniglione, R ; Costantini, H ; Coyle, P ; Creusot, A ; De Bonis, G ; Decowski, M P ; Distefano, C ; Donzaud, C ; Dornic, D ; Dorosti, Q ; Drouhin, D ; Eberl, T ; Enzenhoefer, A ; J -P Ernenwein ; Escoffier, S ; Fermani, P ; Ferry, S ; Folger, F ; Fritsch, U ; Galata, S ; Gay, P ; Giacomelli, G ; Giordano, V ; Gleixner, A ; Gomez-Gonzalez, J P ; Hamal, M ; H van Haren ; Hello, Y ; Hernandez-Rey, J J ; Hoessl, J ; de Jong, M ; Kadler, M ; Kooijman, P ; Kopper, C ; Kreykenbohm, I ; Kulikovskiy, V ; Lambard, G ; Larosa, G ; Lattuada, D ; D Lo Presti ; Louis, F ; Mangano, S ; Marcelin, M ; Margiotta, A ; Martinez-Mora, J A ; Meli, A ; Montaruli, T ; Morganti, M ; Moscoso, L ; Nezri, E ; Pavalas, G E ; Piattelli, P ; Popa, V ; Racca, C ; Reed, C ; Riccobene, G ; Riviere, C ; Roensch, K ; Ruiz-Rivas, J ; Russo, G V ; Samtleben, D F E ; Sanchez-Losa, A ; Sapienza, P ; Schoeck, F ; J -P Schuller ; Shanidze, R ; Simeone, F ; Spies, A ; Spurio, M ; Stolarczyk, Th ; Taiuti, M ; Trovato, A ; Vallage, B ; V Van Elewyck ; Vecchi, M ; Vernin, P ; Wijnker, G ; Wilms, J ; de Wolf, E</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a518-664c0bcb3fb378bbc5301190ce35cbfec345a4467d8b8f071b1fd721bb2be8763</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2012</creationdate><topic>Muons</topic><topic>Neutrinos</topic><topic>Oscillations</topic><topic>Parameters</topic><topic>Physics - High Energy Physics - Experiment</topic><topic>Tracks (paths)</topic><toplevel>online_resources</toplevel><creatorcontrib>ANTARES collaboration</creatorcontrib><creatorcontrib>Adrian-Martinez, S</creatorcontrib><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>Andre, M</creatorcontrib><creatorcontrib>Anvar, S</creatorcontrib><creatorcontrib>Ardid, M</creatorcontrib><creatorcontrib>Astraatmadja, T</creatorcontrib><creatorcontrib>J -J Aubert</creatorcontrib><creatorcontrib>Basa, S</creatorcontrib><creatorcontrib>Biagi, S</creatorcontrib><creatorcontrib>Bigongiari, C</creatorcontrib><creatorcontrib>Bogazzi, C</creatorcontrib><creatorcontrib>Bou-Cabo, M</creatorcontrib><creatorcontrib>Brunner, J</creatorcontrib><creatorcontrib>Busto, J</creatorcontrib><creatorcontrib>Carloganu, C</creatorcontrib><creatorcontrib>Carr, J</creatorcontrib><creatorcontrib>Charif, Z</creatorcontrib><creatorcontrib>Charvis, Ph</creatorcontrib><creatorcontrib>Chiarusi, T</creatorcontrib><creatorcontrib>Circella, M</creatorcontrib><creatorcontrib>Coniglione, R</creatorcontrib><creatorcontrib>Costantini, H</creatorcontrib><creatorcontrib>Coyle, P</creatorcontrib><creatorcontrib>Creusot, A</creatorcontrib><creatorcontrib>De Bonis, G</creatorcontrib><creatorcontrib>Decowski, M P</creatorcontrib><creatorcontrib>Distefano, C</creatorcontrib><creatorcontrib>Donzaud, C</creatorcontrib><creatorcontrib>Dornic, D</creatorcontrib><creatorcontrib>Dorosti, Q</creatorcontrib><creatorcontrib>Drouhin, D</creatorcontrib><creatorcontrib>Eberl, T</creatorcontrib><creatorcontrib>Enzenhoefer, 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Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>ANTARES collaboration</au><au>Adrian-Martinez, S</au><au>Albert, A</au><au>Andre, M</au><au>Anvar, S</au><au>Ardid, M</au><au>Astraatmadja, T</au><au>J -J Aubert</au><au>Basa, S</au><au>Biagi, S</au><au>Bigongiari, C</au><au>Bogazzi, C</au><au>Bou-Cabo, M</au><au>Brunner, J</au><au>Busto, J</au><au>Carloganu, C</au><au>Carr, J</au><au>Charif, Z</au><au>Charvis, Ph</au><au>Chiarusi, T</au><au>Circella, M</au><au>Coniglione, R</au><au>Costantini, H</au><au>Coyle, P</au><au>Creusot, A</au><au>De Bonis, G</au><au>Decowski, M P</au><au>Distefano, C</au><au>Donzaud, C</au><au>Dornic, D</au><au>Dorosti, Q</au><au>Drouhin, D</au><au>Eberl, T</au><au>Enzenhoefer, A</au><au>J -P Ernenwein</au><au>Escoffier, S</au><au>Fermani, P</au><au>Ferry, S</au><au>Folger, F</au><au>Fritsch, U</au><au>Galata, S</au><au>Gay, P</au><au>Giacomelli, G</au><au>Giordano, V</au><au>Gleixner, A</au><au>Gomez-Gonzalez, J P</au><au>Hamal, M</au><au>H van Haren</au><au>Hello, Y</au><au>Hernandez-Rey, J J</au><au>Hoessl, J</au><au>de Jong, M</au><au>Kadler, M</au><au>Kooijman, P</au><au>Kopper, C</au><au>Kreykenbohm, I</au><au>Kulikovskiy, V</au><au>Lambard, G</au><au>Larosa, G</au><au>Lattuada, D</au><au>D Lo Presti</au><au>Louis, F</au><au>Mangano, S</au><au>Marcelin, M</au><au>Margiotta, A</au><au>Martinez-Mora, J A</au><au>Meli, A</au><au>Montaruli, T</au><au>Morganti, M</au><au>Moscoso, L</au><au>Nezri, E</au><au>Pavalas, G E</au><au>Piattelli, P</au><au>Popa, V</au><au>Racca, C</au><au>Reed, C</au><au>Riccobene, G</au><au>Riviere, C</au><au>Roensch, K</au><au>Ruiz-Rivas, J</au><au>Russo, G V</au><au>Samtleben, D F E</au><au>Sanchez-Losa, A</au><au>Sapienza, P</au><au>Schoeck, F</au><au>J -P Schuller</au><au>Shanidze, R</au><au>Simeone, F</au><au>Spies, A</au><au>Spurio, M</au><au>Stolarczyk, Th</au><au>Taiuti, M</au><au>Trovato, A</au><au>Vallage, B</au><au>V Van Elewyck</au><au>Vecchi, M</au><au>Vernin, P</au><au>Wijnker, G</au><au>Wilms, J</au><au>de Wolf, E</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope</atitle><jtitle>arXiv.org</jtitle><date>2012-07-02</date><risdate>2012</risdate><eissn>2331-8422</eissn><abstract>The data taken with the ANTARES neutrino telescope from 2007 to 2010, a total live time of 863 days, are used to measure the oscillation parameters of atmospheric neutrinos. Muon tracks are reconstructed with energies as low as 20 GeV. Neutrino oscillations will cause a suppression of vertical upgoing muon neutrinos of such energies crossing the Earth. The parameters determining the oscillation of atmospheric neutrinos are extracted by fitting the event rate as a function of the ratio of the estimated neutrino energy and reconstructed flight path through the Earth. Measurement contours of the oscillation parameters in a two-flavour approximation are derived. Assuming maximum mixing, a mass difference of $\Delta m_{32}^2=(3.1\pm 0.9)\cdot 10^{-3}$ eV$^2$ is obtained, in good agreement with the world average value.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.1206.0645</doi><oa>free_for_read</oa></addata></record>
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source	arXiv.org; Free E- Journals
subjects	Muons Neutrinos Oscillations Parameters Physics - High Energy Physics - Experiment Tracks (paths)
title	Measurement of Atmospheric Neutrino Oscillations with the ANTARES Neutrino Telescope
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