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dc.contributor.author | Albert, A. | es_ES |
dc.contributor.author | Andre, 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 | Avgitas, T. | 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 | Bourret, S. | es_ES |
dc.contributor.author | Bouwheis, M. C. | 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 | 2020-11-26T04:32:29Z | |
dc.date.available | 2020-11-26T04:32:29Z | |
dc.date.issued | 2017-07 | es_ES |
dc.identifier.issn | 0035-8711 | es_ES |
dc.identifier.uri | http://hdl.handle.net/10251/155863 | |
dc.description.abstract | [EN] Gamma-ray bursts are thought to be sites of hadronic acceleration, thus neutrinos are expected from the decay of charged particles, produced in p gamma interactions. The methods and results of a search for muon neutrinos in the data of the ANTARES neutrino telescope from four bright GRBs (GRB 080916C, GRB 110918A, GRB 130427A and GRB 130505A) observed between 2008 and 2013 are presented. Two scenarios of the fireball model have been investigated: the internal shock scenario, leading to the production of neutrinos with energies mainly above 100 TeV, and the photospheric scenario, characterized by a low-energy component in neutrino spectra due to the assumption of neutrino production closer to the central engine. Since no neutrino events have been detected in temporal and spatial coincidence with these bursts, upper limits at 90 per cent confidence level on the expected neutrino fluxes are derived. The non-detection allows for directly constraining the bulk Lorentz factor of the jet Gamma and the baryon loading f(p) | es_ES |
dc.description.sponsorship | We 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 programme and UnivEarthS Labex programme 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 programmes (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 | Oxford University Press | es_ES |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | es_ES |
dc.rights | Reserva de todos los derechos | es_ES |
dc.subject | Acceleration of particles | es_ES |
dc.subject | Neutrinos | es_ES |
dc.subject | Gamma-ray burst: individual: GRB 080916C | es_ES |
dc.subject | Gamma-ray burst: individual: GRB 110918A | es_ES |
dc.subject | Gamma-ray burst: individual: GRB 130427A | es_ES |
dc.subject | Gamma-ray burst: individual: GRB 130505A | es_ES |
dc.subject.classification | FISICA APLICADA | es_ES |
dc.title | Search for high-energy neutrinos from bright GRBs with ANTARES | es_ES |
dc.type | Artículo | es_ES |
dc.identifier.doi | 10.1093/mnras/stx902 | 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. Departamento de Física Aplicada - Departament de Física Aplicada | es_ES |
dc.description.bibliographicCitation | Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.; Ardid Ramírez, M.; Aubert, J.; Avgitas, T.... (2017). Search for high-energy neutrinos from bright GRBs with ANTARES. Monthly Notices of the Royal Astronomical Society. 469(1):906-915. https://doi.org/10.1093/mnras/stx902 | es_ES |
dc.description.accrualMethod | S | es_ES |
dc.relation.publisherversion | https://doi.org/10.1093/mnras/stx902 | es_ES |
dc.description.upvformatpinicio | 906 | es_ES |
dc.description.upvformatpfin | 915 | es_ES |
dc.type.version | info:eu-repo/semantics/publishedVersion | es_ES |
dc.description.volume | 469 | es_ES |
dc.description.issue | 1 | es_ES |
dc.relation.pasarela | S\340253 | 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 | 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 | Département du Var and Ville de La Seyne-sur-Mer | es_ES |
dc.contributor.funder | Bundesministerium für Bildung und Forschung, Alemania | es_ES |
dc.contributor.funder | National Authority for Scientific Research, Rumanía | es_ES |
dc.contributor.funder | Centre National pour la Recherche Scientifique et Technique, Marruecos | 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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