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dc.contributor.authorLai, Kwang-Changen_US
dc.contributor.authorLai, Wei-Haoen_US
dc.contributor.authorLin, Guey-Linen_US
dc.date.accessioned2019-04-03T06:41:31Z-
dc.date.available2019-04-03T06:41:31Z-
dc.date.issued2017-12-26en_US
dc.identifier.issn2470-0010en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevD.96.115026en_US
dc.identifier.urihttp://hdl.handle.net/11536/144285-
dc.description.abstractWe study Lorentz violation effects on flavor transitions of high energy astrophysical neutrinos. It is shown that the appearance of a Lorentz-violating Hamiltonian can drastically change the flavor transition probabilities of astrophysical neutrinos. Predictions of Lorentz-violation effects on flavor compositions of astrophysical neutrinos arriving on Earth are compared with IceCube flavor composition measurement which analyzes astrophysical neutrino events in the energy range between 25 TeV and 2.8 PeV. Such a comparison indicates that the future IceCube-Gen2 will be able to place stringent constraints on a Lorentz-violating Hamiltonian in the neutrino sector. We work out the expected sensitivities by IceCube-Gen2 on dimension-3 CPT-odd and dimension-4 CPT-even operators in a Lorentz-violating Hamiltonian. The expected sensitivities can improve on the current constraints obtained from other types of experiments by more than two orders of magnitudes for certain ranges of the parameter space.en_US
dc.language.isoen_USen_US
dc.titleConstraining the mass scale of a Lorentz-violating Hamiltonian with the measurement of astrophysical neutrino-flavor compositionen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevD.96.115026en_US
dc.identifier.journalPHYSICAL REVIEW Den_US
dc.citation.volume96en_US
dc.citation.issue11en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000418657500014en_US
dc.citation.woscount2en_US
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