The Physics of Massive Neutrinos
By C. Gonzalez-Garcia. 2009
150 citations recorded by the source corpus.
In this talk I review the present status of neutrino masses and mixing and some of their implications for particle physics phenomenology.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/20263c4a30b0dcd7a418d037f24e89e27133f51c
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Citations in the corpus
- Sensitivity and discovery potential of the proposed nEXO experiment to neutrinoless double- β decay (2017, methodology): “Generation of 2νββ decays is performed using the algorithm in [45], validated in the EXO-200 analysis.”
- Flavor structures of charged fermions and massive neutrinos (2019, background): “Such a Majorana neutrino mass term is possible because the neutrino fields (ναL) c = (νc α)R are actually right-handed [169].”
- The EXO-200 detector, part I: detector design and construction (2012, background): “Zero-neutrino double beta decay (0νββ ), on the other hand, is a lepton-number violating decay that can occur only if neutrinos are massive Majorana particles [2, 3].”
- Nuclear matrix elements for double- β decay (2013, background): “Similarly for a factor of 4 included in some definition of G 0ν [2] and not in others [57].”
- Lepton Flavor and Number Conservation, and Physics Beyond the Standard Model (2013, background): “The phase space factors G and G can be found in [51].”
- Phase space factors for double-$\beta$ decay (2012, background): “5 where they are compared with previous calculations [21].”