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Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope
- Source :
- Physics Letters B, 714(2-5), 224. Elsevier, ANTARES Collaboration Bigongiari, C. Dornic, Damien Emanuele, U. Gómez González, Juan Pablo Hernández Rey, Juan José Lambard, Guillaume Mangano, Salvatore Ruiz-Rivas Onsés, Joaquín Sánchez Losa, Agustín Yepes Ramírez, Harold Zornoza Gómez, Juan de Dios Zúñiga Román, Juan 2012 Measurement of atmospheric neutrino oscillations with the ANTARES neutrino telescope Physics Letters B 714 2-5 224 230, RODERIC. Repositorio Institucional de la Universitat de Valéncia, instname, Physics Letters B, Physics Letters B, Elsevier, 2012, 714, pp.224-230. ⟨10.1016/j.physletb.2012.07.002⟩, Physics Letters B, 2012, 714, pp.224-230. ⟨10.1016/j.physletb.2012.07.002⟩, Recercat. Dipósit de la Recerca de Catalunya, Physics Letters. B, Vol. 714, No 2-5 (2012) pp. 224-230, UPCommons. Portal del coneixement obert de la UPC, Universitat Politècnica de Catalunya (UPC), RiuNet. Repositorio Institucional de la Universitat Politécnica de Valéncia, Physics Letters B, 714(2-5), 224-230. Elsevier
- Publication Year :
- 2012
- Publisher :
- Elsevier, 2012.
-
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 maximal mixing, a mass difference of Delta m(32)(2) = (3.1 +/- 0.9) . 10(-3) eV(2) is obtained, in good agreement with the world average value. (C) 2012 Elsevier B.V. All rights reserved.<br />The authors acknowledge the financial support of the funding agencies: Centre National de la Recherche Scientifique (CNRS), Commissariat a l'energie atomique et aux energies alternatives (CEA), Commission Europeenne (FEDER fund and Marie Curie Program), Region Alsace (contrat CPER), Region Provence-Alpes-Cote d'Azur, Departement du Var and Ville de La Seyne-sur-Mer, France; Bundesministerium fur Bildung und Forschung (BMBF), Germany; Istituto Nazionale di Fisica Nucleare (INFN), Italy; Stichting voor Fundamenteel Onderzoek der Materie (FOM), Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO), the Netherlands; Council of the President of the Russian Federation for young scientists and leading scientific schools supporting grants, Russia; National Authority for Scientific Research (ANCS-UEFISCDI), Romania; Ministerio de Ciencia e Innovacion (MICINN), Prometeo of Generalitat Valenciana and MultiDark, Spain; Agence de l'Oriental and CNRST, Morocco. We also acknowledge the technical support of Ifremer, AIM and Foselev Marine for the sea operation and the CC-IN2P3 for the computing facilities.
- Subjects :
- Nuclear and High Energy Physics
Particle physics
[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
Physics::Instrumentation and Detectors
Solar neutrino
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
ddc:500.2
Neutrino telescope
01 natural sciences
Partícules (Física nuclear)
High Energy Physics - Experiment
Nuclear physics
High Energy Physics - Experiment (hep-ex)
Experiment
0103 physical sciences
Neutrins
High Energy Physics
Neutrinos
010306 general physics
Neutrino oscillation
Physics
Muon
ANTARES
Física [Àrees temàtiques de la UPC]
010308 nuclear & particles physics
Neutrino oscillations
[SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]
High Energy Physics::Phenomenology
Solar neutrino problem
Neutrino astrophysics
Cosmic neutrino background
Neutrino detector
FISICA APLICADA
Measurements of neutrino speed
Física nuclear
High Energy Physics::Experiment
Neutrino
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Subjects
Details
- Language :
- English
- ISSN :
- 18732445 and 03702693
- Volume :
- 714
- Issue :
- 2-5
- Database :
- OpenAIRE
- Journal :
- Physics Letters B
- Accession number :
- edsair.doi.dedup.....8f6891dde3c7d3d38ae7b9ab09127cdf
- Full Text :
- https://doi.org/10.1016/j.physletb.2012.07.002⟩