Zum Hauptinhalt springen Zur Suche springen Zur Hauptnavigation springen
Beschreibung
This thesis is devoted to ANTARES, the first underwater neutrino telescope in the Mediterranean sea. As the main scientific analysis, a search for high-energy neutrino emission from the region of the Fermi bubbles has been performed using data from the ANTARES detector. A method for the background estimation using off-zones has been developed specially for this measurement. A new likelihood for the limits calculation which treats both observations in the on-zone and in the off-zone in the similar way and also includes different systematic uncertainties has been constructed. The analysis of 2008-2011 ANTARES data yielded a 1.2 s excess of events in the Fermi bubble regions, compatible with the no-signal hypothesis. For the optimistic case of no energy cutoff in the flux, the upper limit is within a factor of three of the prediction of the purely hadronic model based on the measured gamma-ray flux. The sensitivity improves as more data are accumulated (more than 65% gain in the sensitivity is expected once 2012-2016 data are added to the analysis).
This thesis is devoted to ANTARES, the first underwater neutrino telescope in the Mediterranean sea. As the main scientific analysis, a search for high-energy neutrino emission from the region of the Fermi bubbles has been performed using data from the ANTARES detector. A method for the background estimation using off-zones has been developed specially for this measurement. A new likelihood for the limits calculation which treats both observations in the on-zone and in the off-zone in the similar way and also includes different systematic uncertainties has been constructed. The analysis of 2008-2011 ANTARES data yielded a 1.2 s excess of events in the Fermi bubble regions, compatible with the no-signal hypothesis. For the optimistic case of no energy cutoff in the flux, the upper limit is within a factor of three of the prediction of the purely hadronic model based on the measured gamma-ray flux. The sensitivity improves as more data are accumulated (more than 65% gain in the sensitivity is expected once 2012-2016 data are added to the analysis).
Zusammenfassung
2006 - 2008 Master thesis, Moscow State University. KM3NeT detector simulations.
2009 - 2011 INFN fellow, Genoa. Supernova detection with ANTARES.
2011 - 2013 PhD thesis, Genoa & Paris VII. Fermi bubbles analysis with the ANTARES data. Neutrino mass hierarchy study with ORCA.
2014 - 2015 INFN Postdoc, Laboratori Nazionali del Sud. KM3NeT detector construction & tests. KM3NeT sensitivity to Dark Matter.
Inhaltsverzeichnis
Introduction.- The ANTARES Detector.- Simulation of the ANTARES Detector Work.- Event Reconstruction and Data Selection.- Fermi Bubbles Analysis.- Conclusions.
Details
Erscheinungsjahr: 2016
Fachbereich: Astronomie
Genre: Physik
Rubrik: Naturwissenschaften & Technik
Medium: Taschenbuch
Inhalt: xiii
119 S.
51 s/w Illustr.
34 farbige Illustr.
119 p. 85 illus.
34 illus. in color.
ISBN-13: 9783319387154
ISBN-10: 3319387154
Sprache: Englisch
Herstellernummer: 978-3-319-38715-4
Einband: Kartoniert / Broschiert
Autor: Kulikovskiy, Vladimir
Auflage: Softcover reprint of the original 1st ed. 2015
Hersteller: Springer
Springer, Berlin
Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, D-69121 Heidelberg, juergen.hartmann@springer.com
Abbildungen: XIII, 119 p. 85 illus., 34 illus. in color.
Maße: 234 x 157 x 6 mm
Von/Mit: Vladimir Kulikovskiy
Erscheinungsdatum: 17.10.2016
Gewicht: 0,221 kg
Artikel-ID: 111862213