Neutrino observatories can characterize cosmic sources and neutrino properties
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Neutrino observatories can characterize cosmic sources and neutrino properties

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Neutrino observatories can characterize cosmic sources and neutrino properties

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Barenboim Szuchman, Gabriela Alejandra Perfil; Quigg, Chris
Aquest document és un/a article, creat/da en: 2003
Neutrino telescopes that measure relative fluxes of ultrahigh-energy nu(e),nu(mu),nu(tau) can give information about the location and characteristics of sources, about neutrino mixing, and can test for neutrino instability and for departures from CPT invariance in the neutrino sector. We investigate the consequences of neutrino mixing for the neutrino flux arriving at Earth, and consider how terrestrial measurements can characterize distant sources. We contrast mixtures that arise from neutrino oscillations with those signaling neutrino decays. We stress the importance of measuring nu(e),nu(mu),nu(tau) fluxes in neutrino observatories.

    Barenboim Szuchman, Gabriela Alejandra Quigg, Chris 2003 Neutrino observatories can characterize cosmic sources and neutrino properties Physical Review D 67 7 073024
http://dx.doi.org/10.1103/PhysRevD.67.073024
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