Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Avgitas T., Baret B., Barrios-Marti J., Basa S., Bertin V., Biagi S., Bormuth R., Bourret S., Bouwhuis M. C., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., Chiarusi T., Circella M., Coelho J. A. B., Coleiro A., Coniglione R., Costantini H., Coyle P., Creusot A., Deschamps A., De Bonis G., Distefano C., Di Palma I., Donzaud C., Dornic D., Drouhin D., Eberl T., El Bojaddaini I., Elsasser D., Enzenhofer A., Felis I., Fusco L. A., Galata S., Gay P., Geisselsoder S., Geyer K., Giordano V., Gleixner A., Glotin H., Gregoire T., Ruiz R. G., Graf K., Hallmann S., Van Haren H., Heijboer A. J., Hello Yann, et al. (2017). Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope [+ Erratum in Physical Letters : B. 2019, vol. 796, pp. 253-255]. Physics Letters B, 769, p. 249-254 [+ Erratum in Physical Letters : B. 2019, vol. 796, pp. 253-255]. ISSN 0370-2693.
Titre du document
Results from the search for dark matter in the Milky Way with 9 years of data of the ANTARES neutrino telescope [+ Erratum in Physical Letters : B. 2019, vol. 796, pp. 253-255]
Année de publication
2017
Auteurs
Albert A., Andre M., Anghinolfi M., Anton G., Ardid M., Aubert J. J., Avgitas T., Baret B., Barrios-Marti J., Basa S., Bertin V., Biagi S., Bormuth R., Bourret S., Bouwhuis M. C., Bruijn R., Brunner J., Busto J., Capone A., Caramete L., Carr J., Celli S., Chiarusi T., Circella M., Coelho J. A. B., Coleiro A., Coniglione R., Costantini H., Coyle P., Creusot A., Deschamps A., De Bonis G., Distefano C., Di Palma I., Donzaud C., Dornic D., Drouhin D., Eberl T., El Bojaddaini I., Elsasser D., Enzenhofer A., Felis I., Fusco L. A., Galata S., Gay P., Geisselsoder S., Geyer K., Giordano V., Gleixner A., Glotin H., Gregoire T., Ruiz R. G., Graf K., Hallmann S., Van Haren H., Heijboer A. J., Hello Yann, et al.
Source
Physics Letters B, 2017,
769, p. 249-254 [+ Erratum in Physical Letters : B. 2019, vol. 796, pp. 253-255] ISSN 0370-2693
Using data recorded with the ANTARES telescope from 2007 to 2015, a new search for dark matter annihilation in the Milky Way has been performed. Three halo models and five annihilation channels, WIMP + WIMP -> b (b) over bar, W+W-, tau(+)tau(-), mu(+)mu(-) and v (v) over bar, with WIMP masses ranging from 50 2 GeV/C-2 to 100 Tev/C-2, were considered. No excess over the expected background was found, and limits on the thermally averaged annihilation cross-section were set.
Plan de classement
Sciences fondamentales / Techniques d'analyse et de recherche [020]
;
Sciences de la Terre : généralités [060]
Localisation
Fonds IRD [F B010070199]
Identifiant IRD
fdi:010070199
