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dc.contributor.authorMaltoni, Michele-
dc.contributor.authorWinter, Walter-
dc.date.accessioned2008-07-02T12:38:36Z-
dc.date.available2008-07-02T12:38:36Z-
dc.date.issued2008-03-13-
dc.identifier.citationarXiv:0803.2050v1 [hep-ph]en_US
dc.identifier.urihttp://hdl.handle.net/10261/5539-
dc.description28 pages, 7 figures, 4 tables.-- A number of corresponding movies can be found at: http://theorie.physik.uni-wuerzburg.de/~winter/Resources/AstroMovies.html.en_US
dc.description.abstractWe discuss the interplay of neutrino oscillation and decay properties at neutrino telescopes. Motivated by recent unparticle scenarios, which open the possibility of new neutrino decay modes over astrophysical distances, we perform a complete classification of possible decay schemes, and we illustrate how different scenarios can be identified. Moreover, we show that the sensitivity of neutrino telescopes to standard neutrino properties, such as the mass hierarchy or δ_CP, is greatly enhanced in specific decay scenarios. In particular we discuss the impact of an astrophysical neutrino detection on terrestrial experiments, such as on the mass hierarchy measurement at NOvA. For example, we find that the scenario where only v_1 is stable can be uniquely identified against all the other decay schemes, and that in this case CP violation can be established (for large Θ_13) by the combination of Double Chooz with the track-to-shower ratio at a neutrino telescope, even if the flavor composition at the source is unknown. Our statements are based on a complete analysis of all the present solar, atmospheric, reactor and accelerator neutrino data, as well as on realistic simulation of future terrestrial neutrino oscillation experiments.en_US
dc.description.sponsorshipMM is supported by MEC through the Ramón y Cajal program and through the national project FPA2006-01105, by the Comunidad Autónoma de Madrid through the HEPHACOS project P-ESP-00346, and by the European Union through the ENTApP network of the ILIAS project RII3-CT-2004-506222. WW acknowledges support from the Emmy Noether program of Deutsche Forschungsgemeinschaft.en_US
dc.format.extent459891 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoengen_US
dc.relation.ispartofseriesIFT-UAM/CSIC-08-16en_US
dc.relation.isversionofPreprint-
dc.rightsopenAccessen_US
dc.subjectNeutrino oscillationsen_US
dc.subjectNeutrino decayen_US
dc.subjectNeutrino telescopesen_US
dc.subjectHigh Energy Physics - Phenomenologyen_US
dc.subjectAstrophysicsen_US
dc.subjectHigh Energy Physics - Experimenten_US
dc.titleTesting neutrino oscillations plus decay with neutrino telescopesen_US
dc.typepreprinten_US
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