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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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dc.contributor.author Barenboim Szuchman, Gabriela Alejandra
dc.contributor.author Quigg, Chris
dc.date.accessioned 2015-04-28T07:26:24Z
dc.date.available 2015-04-28T07:26:24Z
dc.date.issued 2003
dc.identifier.citation Barenboim Szuchman, Gabriela Alejandra Quigg, Chris 2003 Neutrino observatories can characterize cosmic sources and neutrino properties Physical Review D 67 7 073024
dc.identifier.uri http://hdl.handle.net/10550/43446
dc.description.abstract 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.
dc.language.iso eng
dc.relation.ispartof Physical Review D, 2003, vol. 67, num. 7, p. 073024
dc.subject Física
dc.title Neutrino observatories can characterize cosmic sources and neutrino properties
dc.type journal article es_ES
dc.date.updated 2015-04-28T07:26:24Z
dc.identifier.doi 10.1103/PhysRevD.67.073024
dc.identifier.idgrec 030680
dc.rights.accessRights open access es_ES

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