Current experimental data guarantees the presence of physics beyond the Standard Model in the neutrino sector. The responsible physical description might show itself through virtual effects on low-energy observables. In particular, massive neutrinos are able to produce contributions to the triple gauge coupling $WW\gamma$. The present paper deals with the calculation, estimation and analysis of one-loop contributions from Majorana neutrinos to the Lorentz-covariant $WW\gamma$ parametrization. Our calculations show that CP-odd effects vanish exactly, whereas CP-even contributions, $\Delta\kappa$ and $\Delta Q$, remain. According to our estimations, the effects from heavy neutrinos with masses in the range of hundreds of GeVs dominate over th...
We investigate the question whether leptogenesis, as a mechanism for explaining the baryon asymmetry...
I summarize the present status of global analyses of neutrino oscillations, including the most recen...
Large colliders are not sensitive to light neutrino masses and character, but they can produce new h...
Confirmed by the measurement of neutrino oscillations, neutrino mass is recognized as a genuine mani...
Journal of High Energy Physics 2015.10 (2015): 130 reproduced by permission of Scuola Internazionale...
The simplest extension of the SM to account for the observed neutrino masses and mixings is the addi...
In this study, we explore the non-standard $\nu\bar{\nu}\gamma \gamma$ couplings parametrized by dim...
We perform a detailed analysis of the one-loop corrections to the light neutrino mass matrix within ...
The recent CDF-II measurement of the $W$-boson mass shows a strong tension with the corresponding St...
A variety of new physics scenarios allow for neutrinos to up-scatter into a heavy neutral lepton sta...
We analyse the effects of Dirac and Majorana neutrinos on leptonic decays of muon and tau leptons us...
Heavy Majorana neutrinos beyond the standard model can simultaneously explain the origin of tiny neu...
AbstractA general feature of TeV-scale radiative seesaw models, in which tiny neutrino masses are ge...
Journal of High Energy Physics 2011.5 (2011): 063 reproduced by permission of Scuola Internazionale ...
Massive neutrinos open up the possibility for a variety of new physical phenomena. Among them are os...
We investigate the question whether leptogenesis, as a mechanism for explaining the baryon asymmetry...
I summarize the present status of global analyses of neutrino oscillations, including the most recen...
Large colliders are not sensitive to light neutrino masses and character, but they can produce new h...
Confirmed by the measurement of neutrino oscillations, neutrino mass is recognized as a genuine mani...
Journal of High Energy Physics 2015.10 (2015): 130 reproduced by permission of Scuola Internazionale...
The simplest extension of the SM to account for the observed neutrino masses and mixings is the addi...
In this study, we explore the non-standard $\nu\bar{\nu}\gamma \gamma$ couplings parametrized by dim...
We perform a detailed analysis of the one-loop corrections to the light neutrino mass matrix within ...
The recent CDF-II measurement of the $W$-boson mass shows a strong tension with the corresponding St...
A variety of new physics scenarios allow for neutrinos to up-scatter into a heavy neutral lepton sta...
We analyse the effects of Dirac and Majorana neutrinos on leptonic decays of muon and tau leptons us...
Heavy Majorana neutrinos beyond the standard model can simultaneously explain the origin of tiny neu...
AbstractA general feature of TeV-scale radiative seesaw models, in which tiny neutrino masses are ge...
Journal of High Energy Physics 2011.5 (2011): 063 reproduced by permission of Scuola Internazionale ...
Massive neutrinos open up the possibility for a variety of new physical phenomena. Among them are os...
We investigate the question whether leptogenesis, as a mechanism for explaining the baryon asymmetry...
I summarize the present status of global analyses of neutrino oscillations, including the most recen...
Large colliders are not sensitive to light neutrino masses and character, but they can produce new h...