Neutrino Mass and the SU (2)R Breaking Scale

نویسنده

  • Ernest Ma
چکیده

The neutrino sector in a left-right extension of the Standard Model depends on how SU(2)R is broken. I list all possible scenarios, including the ones where the Majorana νR mass is naturally much smaller than the SU(2)R breaking scale, which is desirable for generating the proper baryon asymmetry of the Universe. The best such choice is identified and discussed. In the Standard Model of particle interactions, the neutrino is part of a left-handed doublet (ν, l)L under SU(2)L × U(1)Y . Whereas the charged lepton must have a righthanded singlet counterpart lR, the singlet νR is not mandatory [because it is trivial under SU(2)L × U(1)Y ] and is absent in the minimal version of the model. On the other hand, its existence is usually assumed so that νL may acquire a naturally small Majorana mass as νR gets a large Majorana mass [again because it is trivial under SU(2)L × U(1)Y ] in the famous canonical seesaw mechanism [1, 2]. Where does νR come from? and what is the magnitude of its Majorana mass? The simplest answer [2] is that U(1)Y is actually a remnant of SU(2)R × U(1)B−L under which (ν, l)R is a doublet, and the large Majorana νR mass comes from the vacuum expectation value (vev) of a scalar SU(2)R triplet, which also breaks SU(2)R × U(1)B−L to U(1)Y . This scenario has dominated the thinking on neutrino mass for over 20 years, but it is not the only possibility, even if the existence of νR is conceded. (Mechanisms without νR are also possible and just as natural [3].) It may not even be the best possibility as far as leptogenesis [4] is concerned, because the SU(2)R gauge interactions will tend to diminish the νR number density in the early Universe. Under SU(3)C × SU(2)L × SU(2)R × U(1)B−L, the quarks and leptons transform as: qL = (u, d)L ∼ (3, 2, 1, 1/3), (1) qR = (u, d)R ∼ (3, 1, 2, 1/3), (2) lL = (ν, e)L ∼ (1, 2, 1,−1), (3) lR = (ν, e)R ∼ (1, 1, 2,−1), (4) where the electric charge is given by Q = I3L + I3R + 1 2 (B − L). (5) To break SU(2)R × U(1)B−L to U(1)Y , there are two possibilities. One is to use the scalar

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 Neutrino Mass and Other Possible Signals of Lepton-number Violation in Supersymmetric Theories * Nir Polonsky

We review a recently proposed framework in which the neutrino mass is a signal of supersymmetry breaking and is suppressed dynamically. In addition, we briefly comment on some possible consequences of general lepton-number violation in supersymmetric theories, e.g., dijet and multijet signals and jj → llγγ. 1. Lepton number violation in supersymmetric models is only mildly constrained (see, e.g...

متن کامل

Threshold effects on the mass-scale predictions in SO(10) models and solar-neutrino puzzle.

We compute the threshold uncertainties due to unknown masses of the Higgs bosons on the predictions for the intermediate and unification scales, MI and MU respectively in SO(10) models.We focus on models with separate breaking scales for Parity and SU(2)R symmetries since they provide a natural realization of the seesaw mechanism for neutrino masses. For the two step symmetry breaking chains ,w...

متن کامل

δT/T and Neutrino Masses in SU(5)

We implement inflation in a supersymmetric SU(5) model with U(1)R symmetry such that the cosmic microwave anisotropy δT/T is proportional to (M/MPlanck) 2, where M ∼ MGUT = 2 − 3 × 1016 GeV, the SU(5) breaking scale, and MPlanck = 1.2 × 1019 GeV. The presence of a global U(1)X symmetry, spontaneously broken also at scale MGUT , provides an upper bound M2 GUT /MPlanck ∼ 1014 GeV on the masses of...

متن کامل

New Jarlskog Determinant from Physics above the GUT Scale

We study the Planck scale effects on Jarlskog determiant. Quantum gravitational (Planck scale) effects lead to an effective SU(2) × U(1) invariant dimension-5 Lagrangian involving neutrino and Higgs fields, which give rise to additional terms in neutrino mass matrix on electroweak symmetry breaking. We assume that gravitational interaction is flavor blind and compute the Jarlskog determiant due...

متن کامل

Right-handed-neutrino Majorana mass at the SUSY GUT scale and the solution of the solar-neutrino problem.

In the SUSY GUT scenario, it is natural to assume the right-handed-neutrino Majorana-mass scale to be 10 GeV. This will in principle lead, by the seesaw mechanism, to a mass of order m 2 t =(10GeV ) 3 10 3 eV . This suggests that the solution of the solar-neutrino puzzle should be either the MSW e ect in e{ oscillations, with m 2 10 5 eV 2, or long-wavelength e{ oscillations, with m 10 10 eV 2....

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 2003