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Renormalization group running of neutrino parameters
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Neutrinos are the most elusive particles in our universe. They have masses at least one million times smaller than the electron mass, carry no electric charge, and very weakly interact with other particles, meaning they are rarely captured in terrestrial detectors. Tremendous efforts in the past two decades have revealed that neutrinos can transform from one type to another as a consequence of neutrino oscillations---a quantum mechanical effect over macroscopic distances---yet the origin of neutrino masses remains puzzling. The physical evolution of neutrino parameters with respect to energy scale may help elucidate the mechanism for their mass generation.
Forward citations
Cited by 3 Pith papers
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Confronting the seesaw mechanism with neutrino oscillations: a general and explicit analytical bridge
The paper provides, for the first time, explicit analytical expressions for the two mass-squared differences, three mixing angles, and effective Dirac CP phase of the canonical seesaw mechanism in terms of its 18 para...
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Disentangle RG Running Parameters with Medium-Baseline Reactor Experiments
RG running beta functions of mixing parameters alter the fast oscillation mode at JUNO and can reduce mass ordering sensitivity, but measurements from the TAO near detector can restore it by constraining the running p...
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RG Running of Multiple Neutrino Mixing Parameters at Oscillation Experiments
Combining DUNE-ND, JUNO-TAO, and FASERν2 data can disentangle multiple model-independent RG running parameters of neutrino mixing and resolve degeneracies.
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