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Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope

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Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope

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dc.contributor.author Adrián Martínez, Silvia es_ES
dc.contributor.author Albert, A. es_ES
dc.contributor.author André, M. es_ES
dc.contributor.author Anghinolfi, M. es_ES
dc.contributor.author Anton, G. es_ES
dc.contributor.author Ardid Ramírez, Miguel es_ES
dc.contributor.author Aubert, J.J. es_ES
dc.contributor.author Baret, B. es_ES
dc.contributor.author Barrios-Marti, J. es_ES
dc.contributor.author Basa, S. es_ES
dc.contributor.author Bertin, V. es_ES
dc.contributor.author Biagi, S. es_ES
dc.contributor.author Bormuth, R. es_ES
dc.contributor.author M. C. Bouwheis es_ES
dc.contributor.author R. Bruijn es_ES
dc.contributor.author Felis-Enguix, Iván es_ES
dc.contributor.author Martínez Mora, Juan Antonio es_ES
dc.contributor.author Saldaña-Coscollar, María es_ES
dc.date.accessioned 2020-11-24T04:31:43Z
dc.date.available 2020-11-24T04:31:43Z
dc.date.issued 2017-01-10 es_ES
dc.identifier.issn 1434-6044 es_ES
dc.identifier.uri http://hdl.handle.net/10251/155498
dc.description.abstract [EN] A search for high-energy neutrino emission cor-related with gamma-ray bursts outside the electromagnetic prompt-emission time window is presented. Using a stack-ing approach of the time delays between reported gamma-ray burst alerts and spatially coincident muon-neutrino sig-natures, data from the Antares neutrino telescope recorded between 2007 and 2012 are analysed. One year of public data from the IceCube detector between 2008 and 2009 have been also investigated. The respective timing profiles are scanned for statistically significant accumulations within 40 days of the Gamma Ray Burst, as expected from Lorentz Invariance Violation effects and some astrophysical models. No signif-icant excess over the expected accidental coincidence rate could be found in either of the two data sets. The average strength of the neutrino signal is found to be fainter than one detectable neutrino signal per hundred gamma-ray bursts in the Antares data at 90% confidence level. es_ES
dc.description.sponsorship 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), Institut Universitaire de France (IUF), IdEx program and UnivEarthS Labex program at Sorbonne Paris Cite (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02), Labex OCEVU (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02), Region Ile-de-France (DIM-ACAV), 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), Romania; Ministerio de Economia y Competitividad (MINECO): Plan Estatal de Investigacion (refs. FPA2015-65150-C3-1-P, -2-P and -3-P, (MINECO/FEDER)), Severo Ochoa Centre of Excellence and MultiDark Consolider (MINECO), and Prometeo and Grisolia programs (Generalitat Valenciana), 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 es_ES
dc.language Inglés es_ES
dc.publisher Springer-Verlag es_ES
dc.relation.ispartof The European Physical Journal C es_ES
dc.rights Reconocimiento (by) es_ES
dc.subject Gamma-ray burst es_ES
dc.subject High-energy neutrino es_ES
dc.subject IceCube es_ES
dc.subject Antares telescope es_ES
dc.subject.classification FISICA APLICADA es_ES
dc.title Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope es_ES
dc.type Artículo es_ES
dc.identifier.doi 10.1140/epjc/s10052-016-4496-8 es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-1-P/ES/PARTICIPACION DEL IFIC EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-LABX-0060/FR/Origines, Constituants et EVolution de l'Univers/OCEVU/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0005/FR/Université Sorbonne Paris Cité/USPC/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-11-IDEX-0001/FR/INITIATIVE D'EXCELLENCE AIX MARSEILLE UNIVERSITE/Amidex/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/ANR//ANR-10-LABX-0023/FR/Earth - Planets - Universe: observation, modeling, transfer/UnivEarthS/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-3-P/ES/PARTICIPACION DE LA UGR EN ANTARES, KM3NET-ARCA%2FORCA Y PDG/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MICINN//CSD2009-00064/ES/Método de Multimensajeros para la Detección de la Materia Oscura/ es_ES
dc.relation.projectID info:eu-repo/grantAgreement/MINECO//FPA2015-65150-C3-2-P/ES/PARTICIPACION DE LA UPV EN ANTARES Y KM3NET-ARCA%2FORCA/ es_ES
dc.rights.accessRights Abierto es_ES
dc.contributor.affiliation Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres es_ES
dc.contributor.affiliation Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada es_ES
dc.description.bibliographicCitation Adrián Martínez, S.; Albert, A.; André, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, M.; Aubert, J.... (2017). Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope. The European Physical Journal C. 77(1):1-10. https://doi.org/10.1140/epjc/s10052-016-4496-8 es_ES
dc.description.accrualMethod S es_ES
dc.relation.publisherversion https://doi.org/10.1140/epjc/s10052-016-4496-8 es_ES
dc.description.upvformatpinicio 1 es_ES
dc.description.upvformatpfin 10 es_ES
dc.type.version info:eu-repo/semantics/publishedVersion es_ES
dc.description.volume 77 es_ES
dc.description.issue 1 es_ES
dc.relation.pasarela S\329227 es_ES
dc.contributor.funder A*Midex Foundation es_ES
dc.contributor.funder Agence Nationale de la Recherche, Francia es_ES
dc.contributor.funder Region Ile-de-France es_ES
dc.contributor.funder Generalitat Valenciana es_ES
dc.contributor.funder Université Sorbonne Paris Cité es_ES
dc.contributor.funder Institut Universitaire de France es_ES
dc.contributor.funder European Regional Development Fund es_ES
dc.contributor.funder Instituto Nazionale di Fisica Nucleare es_ES
dc.contributor.funder Ministerio de Economía y Competitividad es_ES
dc.contributor.funder Conseil Régional Provence-Alpes-Côte d'Azur es_ES
dc.contributor.funder Netherlands Organization for Scientific Research es_ES
dc.contributor.funder Bundesministerium für Bildung und Forschung, Alemania es_ES
dc.contributor.funder Centre National de la Recherche Scientifique, Francia es_ES
dc.contributor.funder National Authority for Scientific Research, Rumanía es_ES
dc.contributor.funder Council on grants of the President of the Russian Federation es_ES
dc.contributor.funder Centre National pour la Recherche Scientifique et Technique, Marruecos es_ES
dc.contributor.funder Commissariat à l'Énergie Atomique et aux Énergies Alternatives, Francia es_ES
dc.contributor.funder Laboratoire d'Excellence OCEVU (Origines, Constituants & ÉVolution de l'Univers) es_ES
dc.contributor.funder Ministerio de Ciencia e Innovación es_ES
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