Large 1-3 leptonic mixing and Renormalization Group Effects

نویسنده

  • Srubabati Goswami
چکیده

Starting from tri-bimaximal mixing at high scale, we investigate if it is possible to generate a sizable value of |Ue3|, while at the same time keeping solar neutrino mixing near its measured value, which is close to sin θ12 = 1 3 through renormalization group corrections. Generation of indicated values of |Ue3| ≈ 0.1 via this effect requires the neutrinos to be quasidegenerate in mass. If we consider Standard Model (SM) as the low energy effective theory then the required value of the mass scale is beyond 2.3 eV which is the current constraint from tritium β-decay. On the other hand considering the Minimal Supersymmetric Standard Model (MSSM) as the effecitve theory at low energy it is possible to generate the non-zero Ue3 values hinted by the current global analysis for lower m0 values. The consistency with the allowed range of sin θ12 together with large running of |Ue3| forces one of the Majorana phases to be close to π. This implies large cancellations in the effective Majorana mass governing neutrino-less double beta ((ββ)0ν -)decay, constraining it to lie near its minimum allowed value of m0 cos 2θ12, where m0 >∼ 0.1 eV.

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

The LMA Solution from Bimaximal Lepton Mixing at the GUT Scale by Renormalization Group Running

We show that in see-saw models with bimaximal lepton mixing at the GUT scale and with zero CP phases, the solar mixing angle θ12 generically evolves towards sizably smaller values due to Renormalization Group effects, whereas the evolution of θ13 and θ23 is comparatively small. The currently favored LMA solution of the solar neutrino problem can thus be obtained in a natural way from bimaximal ...

متن کامل

Renormalization Group Evolution of Dirac Neutrino Masses

There are good reasons why neutrinos could be Majorana particles, but there exist also a number of very good reasons why neutrinos could have Dirac masses. The latter option deserves more attention and we derive therefore analytic expressions describing the renormalization group evolution of mixing angles and of the CP phase for Dirac neutrinos. Radiative corrections to leptonic mixings are in ...

متن کامل

5 Running Neutrino Masses , Leptonic Mixing Angles and CP - Violating Phases : From M Z to Λ GUT

We derive renormalization group equations for neutrino masses, leptonicmixing angles and CP-violating phases running at energies above the seesawthreshold, both in the Standard Model and in the Minimal SupersymmetricStandard Model extended with three right-handed neutrinos. With theseequations, we carry out a systematic study of the radiative correction that mayarise to ...

متن کامل

Renormalization-Group Effects in the SO(3) Gauge Model With Nearly Degenerate Neutrino Masses and Bi-maximal Mixing

The renormalization-group effects on the scenario with nearly degenerate mass and bi-maximal mixing of neutrinos are analyzed. As a consequence, we explicitly show in the SO(3) gauge model that the renormalization-group effects could modify the fitting values of the relevant basic parameters of the model, but leave the nearly bi-maximal mixing scenario to remain stable for reconciling both sola...

متن کامل

Effective Hamiltonian for Non - Leptonic | ∆ F | = 1 Decays at NNLO in QCD

We compute the effective hamiltonian for non-leptonic |∆F | = 1 decays in the standard model including next-to-next-to-leading order QCD corrections. In particular, we present the complete three-loop anomalous dimension matrix describing the mixing of currentcurrent and QCD penguin operators. The calculation is performed in an operator basis which allows to consistently use fully anticommuting ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009