Adrian-Martinez S., Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Baret B., Barrios-Marti J., Basa S., Bertin V., Biagi S., Bormuth R., Bouwhuis M. C., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Chiarusi T., Circella M., Coniglione R., Costantini H., Coyle P., Creusot A., Dekeyser I., Deschamps A., De Bonis G., Distefano C., Donzaud C., Dornic D., Drouhin D., Dumas A., Eberl T., Elsasser D., Enzenhofer A., Fehn K., Felis I., Fermani P., Folger F., Fusco L. A., Galata S., Gay P., Geisselsoder S., Geyer K., Giordano V., Gleixner A., Gracia-Ruiz R., Graf K., Hallmann S., van Haren H., Heijboer A. J., Hello Yann, et al. (2017). Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope. European Physical Journal C, 77 (1), p. art. 20 [10 p.]. ISSN 1434-6044.
Titre du document
Stacked search for time shifted high energy neutrinos from gamma ray bursts with the ANTARES neutrino telescope
Année de publication
2017
Auteurs
Adrian-Martinez S., Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Baret B., Barrios-Marti J., Basa S., Bertin V., Biagi S., Bormuth R., Bouwhuis M. C., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Chiarusi T., Circella M., Coniglione R., Costantini H., Coyle P., Creusot A., Dekeyser I., Deschamps A., De Bonis G., Distefano C., Donzaud C., Dornic D., Drouhin D., Dumas A., Eberl T., Elsasser D., Enzenhofer A., Fehn K., Felis I., Fermani P., Folger F., Fusco L. A., Galata S., Gay P., Geisselsoder S., Geyer K., Giordano V., Gleixner A., Gracia-Ruiz R., Graf K., Hallmann S., van Haren H., Heijboer A. J., Hello Yann, et al.
Source
European Physical Journal C, 2017,
77 (1), p. art. 20 [10 p.] ISSN 1434-6044
A search for high-energy neutrino emission correlated with gamma-ray bursts outside the electromagnetic prompt-emission time window is presented. Using a stacking approach of the time delays between reported gammaray burst alerts and spatially coincident muon-neutrino signatures, 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 significant 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.
Plan de classement
Sciences fondamentales / Techniques d'analyse et de recherche [020]
;
Limnologie physique / Océanographie physique [032]
;
Sciences de la Terre : généralités [060]
Localisation
Fonds IRD [F B010069411]
Identifiant IRD
fdi:010069411
