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dc.contributor.authorAlbert, A.
dc.contributor.authorAndré, Michel
dc.contributor.authorAnghinolfi, Marco
dc.contributor.authorAnton, G.
dc.contributor.authorAvgitas, T.
dc.contributor.authorBertin, V.
dc.contributor.authorBormuth, R.
dc.contributor.authorPuricelli, Stefano
dc.contributor.authorConiglione, R.
dc.contributor.authorGleixner, A
dc.contributor.authorLefèvre, Dominique
dc.contributor.authorMichael, Turner
dc.contributor.authorPellegrino, Carlo
dc.contributor.authorPiattelli, P.
dc.contributor.authorSanchez Losa, Agustín
dc.contributor.authorSchnabel, J.
dc.contributor.authorTrovato, A.
dc.contributor.authorZúñiga Román, Juan
dc.contributor.otherCentre Tecnològic de Vilanova i la Geltrú
dc.date.accessioned2017-09-01T11:16:05Z
dc.date.available2017-09-01T11:16:05Z
dc.date.issued2017-07-01
dc.identifier.citationAlbert, A., Andre, M., Anghinolfi, M., Anton, G., Avgitas, T., Bertin, V., Bormuth, R., Puricelli, S., Coniglione, R., Gleixner, A., Lefèvre, D., Michael, T., Pellegrino, C., Piattelli, P., Sanchez-Losa, A., Schnabel, J., Trovato, A., Zúñiga, J. Search for high-energy neutrinos from bright GRBs with ANTARES. "Monthly notices of the Royal Astronomical Society", 1 Juliol 2017, vol. 469, núm. 1, p. 906-915.
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/2117/107298
dc.description.abstractGamma-ray bursts are thought to be sites of hadronic acceleration, thus neutrinos are expected from the decay of charged particles, produced in p¿ 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 G and the baryon loading fp.
dc.format.extent10 p.
dc.language.isoeng
dc.rightsAttribution-NonCommercial-NoDerivs 3.0 Spain
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/es/
dc.subjectÀrees temàtiques de la UPC::Física::Astronomia i astrofísica
dc.subject.lcshNeutrino astrophysics
dc.subject.lcshNeutrinos
dc.subject.otherAcceleration of particles
dc.subject.otherneutrinos
dc.subject.otherGamma-ray burst: individual: GRB 080916C
dc.subject.otherGamma-ray burst: individual: GRB 110918A
dc.subject.otherGamma-ray burst: individual: GRB 130427A
dc.subject.otherGamma-ray burst: individual: GRB 130505A
dc.titleSearch for high-energy neutrinos from bright GRBs with ANTARES
dc.typeArticle
dc.subject.lemacAcceleradors de partícules
dc.subject.lemacNeutrins
dc.subject.lemacAstrofísica
dc.contributor.groupUniversitat Politècnica de Catalunya. LAB - Laboratori d'Aplicacions Bioacústiques
dc.identifier.doi10.1093/mnras/stx902
dc.relation.publisherversionhttps://academic.oup.com/mnras/article-abstract/469/1/906/3605380/Search-for-high-energy-neutrinos-from-bright-GRBs?redirectedFrom=fulltext
dc.rights.accessOpen Access
drac.iddocument21105483
dc.description.versionPostprint (author's final draft)
upcommons.citation.authorAlbert, A., Andre, M., Anghinolfi, M., Anton, G., Avgitas, T., Bertin, V., Bormuth, R., Puricelli, S., Coniglione, R., Gleixner, A., Lefèvre, D., Michael, T., Pellegrino, C., Piattelli, P., Sanchez-Losa, A., Schnabel, J., Trovato, A., Zúñiga, J.
upcommons.citation.publishedtrue
upcommons.citation.publicationNameMonthly notices of the Royal Astronomical Society
upcommons.citation.volume469
upcommons.citation.number1
upcommons.citation.startingPage906
upcommons.citation.endingPage915


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