Scalar dark matter and radiative Dirac neutrino mass in an extended \(U(1)_{B-L}\) model
DOI10.1016/j.nuclphysb.2022.115855zbMath1498.83019arXiv2112.12569OpenAlexW4281902682MaRDI QIDQ2155263
Subhasmita Mishra, Narendra Nimmala, Prafulla Kumar Panda, Nirakar Sahoo
Publication date: 15 July 2022
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2112.12569
Unified quantum theories (81V22) Other elementary particle theory in quantum theory (81V25) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Weak interaction in quantum theory (81V15) Motion of charged particles (78A35) Nonselfadjoint operator theory in quantum theory including creation and destruction operators (81Q12) Dark matter and dark energy (83C56) Particle decays (81U90)
Cites Work
- Unnamed Item
- LanHEP -- a package for automatic generation of Feynman rules from the Lagrangian. Version 3.2
- Freeze-in production of FIMP dark matter
- Dirac or inverse seesaw neutrino masses with \(B - L\) gauge symmetry and \(S_3\) flavor symmetry
- Alternative minimal \(\mathrm{U}(1)_{\mathrm{B}-\mathrm{L}}\)
- Unbroken \(B-L\) symmetry
- Scotogenic \(\mathrm U(1)_\chi\) Dirac neutrinos
- Gauge \(B\)-\(L\) model with residual \(Z_3\) symmetry
- Pathways to naturally small Dirac neutrino masses
- Simplest radiative Dirac neutrino mass models
- Neutrino Mass and Spontaneous Parity Nonconservation
- Neutrino decoupling including flavour oscillations and primordial nucleosynthesis
- A precision calculation of relic neutrino decoupling
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