Neutrino mass observables and non-Hermitian version of Type-I seesaw model
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Publication:5029573
DOI10.1088/1475-7516/2021/07/056zbMath1485.83166arXiv1806.06229OpenAlexW3191906109MaRDI QIDQ5029573
Publication date: 14 February 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1806.06229
Relativistic cosmology (83F05) Quantum field theory on curved space or space-time backgrounds (81T20) Gravitational interaction in quantum theory (81V17) Weak interaction in quantum theory (81V15) Matrix models and tensor models for quantum field theory (81T32)
Cites Work
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- \(\mathcal P\mathcal T\)-symmetric quantum electrodynamics
- Dual \(\mathcal P\mathcal T\)-symmetric quantum field theories
- On the consistency of a non-Hermitian Yukawa interaction
- Dynamical Majorana neutrino masses and axions. I.
- Dynamical Majorana neutrino masses and axions. II: Inclusion of anomaly terms and axial background
- On the Fritzsch Texture and Quark-Lepton Complementarity
- \mathcal {P}\mathcal {T} symmetry as a generalization of Hermiticity
- Real Spectra in Non-Hermitian Hamiltonians Having<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="bold-script">P</mml:mi><mml:mi mathvariant="bold-script">T</mml:mi></mml:math>Symmetry
- Neutrino Mass and Spontaneous Parity Nonconservation
- 𝓟𝓣-symmetric quantum mechanics
- Foldy–Wouthuysen transformation for non-Hermitian Hamiltonians
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