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Institut d'Astrophysique et
de Géophysique (Bât. B5c)
Quartier Agora
Allée du 6 août, 19C
B-4000 Liège 1 (Sart-Tilman)
Belgique
Tel.: 04.366.9779
Fax: 04.366.9729
de Géophysique (Bât. B5c)
Quartier Agora
Allée du 6 août, 19C
B-4000 Liège 1 (Sart-Tilman)
Belgique
Tel.: 04.366.9779
Fax: 04.366.9729
Seminars : Documents
BY DOWNLOADING THIS DOCUMENT,
YOU IMPLICITELY AGREE TO NOT PUBLISH EXTRACTS
WITHOUT PRIOR CONSENT OF THE AUTHOR :
Diego Aristizabal Sierra, <daristizabal@ulg.ac.be>
YOU IMPLICITELY AGREE TO NOT PUBLISH EXTRACTS
WITHOUT PRIOR CONSENT OF THE AUTHOR :
Diego Aristizabal Sierra, <daristizabal@ulg.ac.be>
Seminar n°3: Thursday 16 february, 15h45
Basic Implications of Astrophysical Neutrino Backgrounds for Direct Detection Dark Matter Searches
Diego Aristizabal Sierra (Universidad Tecnica Federico Santa Maria - Departamento de Fisica)
Next-generation dark matter direct detection searches will be subject to unavoidable backgrounds from astrophysical neutrinos (solar, atmospheric and diffuse supernova neutrinos), the so-called neutrino floor. In this talk I will discuss very basic aspects of the physics challenges that the neutrino floor gives and of the opportunities that it provides. I will mention the importance that neutrino non-standard-interactions have on the determination of the background.
Diego Aristizabal Sierra (Universidad Tecnica Federico Santa Maria - Departamento de Fisica)
Next-generation dark matter direct detection searches will be subject to unavoidable backgrounds from astrophysical neutrinos (solar, atmospheric and diffuse supernova neutrinos), the so-called neutrino floor. In this talk I will discuss very basic aspects of the physics challenges that the neutrino floor gives and of the opportunities that it provides. I will mention the importance that neutrino non-standard-interactions have on the determination of the background.
University of Liège >
Faculty of Sciences >
Department of Astrophysics, Geophysics and Oceanography :
CoWebAGO, Juin 2009.