Atjaunināt sīkdatņu piekrišanu

Neutrino Astrophysics with the ANTARES Telescope 2015 ed. [Hardback]

  • Formāts: Hardback, 119 pages, height x width: 235x155 mm, weight: 3317 g, 34 Illustrations, color; 51 Illustrations, black and white; XIII, 119 p. 85 illus., 34 illus. in color., 1 Hardback
  • Sērija : Springer Theses
  • Izdošanas datums: 06-Jul-2015
  • Izdevniecība: Springer International Publishing AG
  • ISBN-10: 3319204114
  • ISBN-13: 9783319204116
  • Hardback
  • Cena: 91,53 €*
  • * ši ir gala cena, t.i., netiek piemērotas nekādas papildus atlaides
  • Standarta cena: 107,69 €
  • Ietaupiet 15%
  • Grāmatu piegādes laiks ir 3-4 nedēļas, ja grāmata ir uz vietas izdevniecības noliktavā. Ja izdevējam nepieciešams publicēt jaunu tirāžu, grāmatas piegāde var aizkavēties.
  • Daudzums:
  • Ielikt grozā
  • Piegādes laiks - 4-6 nedēļas
  • Pievienot vēlmju sarakstam
  • Formāts: Hardback, 119 pages, height x width: 235x155 mm, weight: 3317 g, 34 Illustrations, color; 51 Illustrations, black and white; XIII, 119 p. 85 illus., 34 illus. in color., 1 Hardback
  • Sērija : Springer Theses
  • Izdošanas datums: 06-Jul-2015
  • Izdevniecība: Springer International Publishing AG
  • ISBN-10: 3319204114
  • ISBN-13: 9783319204116
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).
Introduction.- The ANTARES Detector.- Simulation of the ANTARES Detector Work.- Event Reconstruction and Data Selection.- Fermi Bubbles Analysis.- Conclusions.
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.