We provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for neutrino mass. Taking into account most recent experimental data on <math altimg="si1.gif" xmlns="http://www.w3.org/1998/Math/MathML"><mi>μ</mi><mo stretchy="false">→</mo><mi>e</mi><mi>γ</mi></math> as well as the mixing angle <math altimg="si2.gif" xmlns="http://www.w3.org/1998/Math/MathML"><msub><mrow><mi>θ</mi></mrow><mrow><mn>13</mn></mrow></msub></math> we obtain lower bounds on the masses of the singly and doubly charged scalars of between 1 and 2 TeV, with some dependence on perturbativity and fine-tuning requirements. This makes the scalars difficult to observe at LHC with 14 TeV even with optimistic assumptions on the luminosity, and would ...
Contrary to the see-saw models, extended Higgs sectors leading to radiatively-induced neutrino masse...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
An extension of the Zee model involving a light right handed neutrino, nu_R is considered. We update...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
We provide an updated scan of the allowed parameter space of the two-loop Zee-Babu model for neutrin...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
We update previous analyses of the Zee–Babu model in the light of new data, e.g., the mixing angle <...
AbstractWe update previous analyses of the Zee–Babu model in the light of new data, e.g., the mixing...
AbstractWe investigate non-standard neutrino interactions (NSIs) in the Zee–Babu model. The size of ...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
In this talk we discuss how the Zee-Babu model can be tested combining information from neutrino dat...
Contrary to the see-saw models, extended Higgs sectors leading to radiatively-induced neutrino masse...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
An extension of the Zee model involving a light right handed neutrino, nu_R is considered. We update...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
We provide an updated scan of the allowed parameter space of the two-loop Zee-Babu model for neutrin...
AbstractWe provide an updated scan of the allowed parameter space of the two-loop Zee–Babu model for...
We update previous analyses of the Zee–Babu model in the light of new data, e.g., the mixing angle <...
AbstractWe update previous analyses of the Zee–Babu model in the light of new data, e.g., the mixing...
AbstractWe investigate non-standard neutrino interactions (NSIs) in the Zee–Babu model. The size of ...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
We update previous analyses of the Zee-Babu model in the light of new data, e.g., the mixing angle O...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
AbstractIn this talk we discuss how the Zee-Babu model can be tested combining information from neut...
In this talk we discuss how the Zee-Babu model can be tested combining information from neutrino dat...
Contrary to the see-saw models, extended Higgs sectors leading to radiatively-induced neutrino masse...
The smallness of the observed neutrino masses might have a radiative origin. Here we revisit a speci...
An extension of the Zee model involving a light right handed neutrino, nu_R is considered. We update...