AbstractSeesaw models with a small lepton number breaking can naturally accommodate electroweak-scale pseudo-Dirac neutrinos with a sizable mixing with the active neutrinos, while satisfying the light neutrino oscillation data. Due to the smallness of the lepton number breaking parameter, the ‘smoking gun’ collider signature of same-sign dileptons is suppressed, and the heavy neutrinos in these models would manifest at the LHC dominantly through lepton number conserving trilepton final states. Using the recent CMS results for anomalous production of multilepton events at the s=8 TeV LHC with an integrated luminosity of 19.5 fb−1, we derive direct upper bounds on the light-heavy neutrino mixing parameter as a function of the heavy Dirac neut...
Presented at the XXXI International Conference of Theoretical Physics, “Matter to the Deepest”, Ustr...
Heavy neutrinos (N) remain one of most promising explanations for the ori-gin of neutrinos' tiny mas...
Heavy neutrinos (N) remain one of most promising explanations for the ori-gin of neutrinos' tiny mas...
Seesaw models with a small lepton number breaking can naturally accommodate electroweak-scale pseudo...
AbstractSeesaw models with a small lepton number breaking can naturally accommodate electroweak-scal...
Seesaw models with a small lepton number breaking can naturally accommodate electroweak-scale pseudo...
Large colliders are not sensitive to light neutrino masses and character, but they can produce new h...
The existence of the neutrino mass has been established by the neutrino oscillation experiments. The...
The observation of lepton flavor violating processes at colliders could be a clear signal of a non-m...
Neutrinos can be pseudo-Dirac in Nature - they can be Majorana fermions whilebehaving effectively as...
Models of neutrino mass generation constitute well motivated scenarios of Beyond-the-Standard-Model ...
The recent discovery of nonzero θ13 (equal to Cabbibo angle θC up to a factor of 2‾√ ), the masses o...
AbstractThe recent discovery of nonzero θ13 (equal to Cabbibo angle θC up to a factor of 2), the mas...
The neutrino masses and flavor mixings, which are missing in the Standard Model (SM), can be natural...
In this work, by using the machine learning methods, we study the sensitivities of heavy pseudo-Dira...
Presented at the XXXI International Conference of Theoretical Physics, “Matter to the Deepest”, Ustr...
Heavy neutrinos (N) remain one of most promising explanations for the ori-gin of neutrinos' tiny mas...
Heavy neutrinos (N) remain one of most promising explanations for the ori-gin of neutrinos' tiny mas...
Seesaw models with a small lepton number breaking can naturally accommodate electroweak-scale pseudo...
AbstractSeesaw models with a small lepton number breaking can naturally accommodate electroweak-scal...
Seesaw models with a small lepton number breaking can naturally accommodate electroweak-scale pseudo...
Large colliders are not sensitive to light neutrino masses and character, but they can produce new h...
The existence of the neutrino mass has been established by the neutrino oscillation experiments. The...
The observation of lepton flavor violating processes at colliders could be a clear signal of a non-m...
Neutrinos can be pseudo-Dirac in Nature - they can be Majorana fermions whilebehaving effectively as...
Models of neutrino mass generation constitute well motivated scenarios of Beyond-the-Standard-Model ...
The recent discovery of nonzero θ13 (equal to Cabbibo angle θC up to a factor of 2‾√ ), the masses o...
AbstractThe recent discovery of nonzero θ13 (equal to Cabbibo angle θC up to a factor of 2), the mas...
The neutrino masses and flavor mixings, which are missing in the Standard Model (SM), can be natural...
In this work, by using the machine learning methods, we study the sensitivities of heavy pseudo-Dira...
Presented at the XXXI International Conference of Theoretical Physics, “Matter to the Deepest”, Ustr...
Heavy neutrinos (N) remain one of most promising explanations for the ori-gin of neutrinos' tiny mas...
Heavy neutrinos (N) remain one of most promising explanations for the ori-gin of neutrinos' tiny mas...