ar X iv : h ep - p h / 97 08 44 5 v 1 2 4 A ug 1 99 7 Concerning the Differences Between Zero Mass Dirac and Majorana Neutrinos

نویسنده

  • A. Widom
چکیده

That a Majorana neutrino theory is different from a Dirac neutrino theory (even in the zero mass limit) is proved in two sentences. Fermion Statistics For the reactions (Dirac) e + e − → ν ¯ ν and (Majorana) e + e − → νν wherein the two final particles are presumed to have opposite helicity, in the Dirac case the neutrino and anti-neutrino are different particles so that Ψ Dirac (p 1 , λ 1 ; ¯ p 2 , ¯ λ 2) (in momentum-helicity) has no particular particle anti-particle exchange symmetry, while in the Majorana case the two neutrinos are identical fermion particles with an exchange anti-symmetric wave function in the center of mass frame[1] Thus, for the Dirac case with a fixed angle of scattering, the probability of having a left helicity neutrino can and does differ from the probability for having a right helicity anti-neutrino dσ dΩ Dirac ν Lef t = dσ dΩ Dirac ¯ ν Right (in general) (2) and for the Majorana case with a fixed angle of scattering, the probability of having a left helicity neutrino is identical to the probability of having a right helicity neutrino dσ dΩ M ajorana ν Lef t = dσ dΩ M ajorana ν Right. (3) This non-perturbative difference (transcending particular parity violating Lagrangian models) between the Dirac and Majorana cases is true even in the zero mass limit. We disclaim responsibility for work purporting to describe more than one Majorana fermion without employing a properly anti-symmetric neutrino wave function. Finally, we have greatly benefited by reading recent debates[2-6].

برای دانلود 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

ar X iv : h ep - p h / 97 08 25 4 v 1 5 A ug 1 99 7 SUPERGRAVITY UNIFIED MODELS

The development of supergravity unified models and their implications for current and future experiment are discussed.

متن کامل

ar X iv : h ep - p h / 96 11 38 3 v 3 8 A pr 1 99 7 Can we distinguish Majorana and Dirac neutrinos in solar neutrino experiments ?

If neutrino conversions within the Sun result in partial polarization of initial solar neutrino fluxes then a new opportunity to distinguish Majorana and Dirac neutrinos by measuring the differential ν e e-scattering cross section in solar neutrino detectors arises. The experiment like HELLAZ would be preferable in testing of recoil electron spectra differences initiated by Majorana and Dirac n...

متن کامل

ar X iv : h ep - p h / 97 08 46 3 v 1 2 6 A ug 1 99 7 Colour reconnection and Bose - Einstein effects ∗

Final-state interactions and interference phenomena that could affect the value of the W mass reconstructed from hadronic WW decays at LEP2 are reviewed, and possible areas for future investigation are identified.

متن کامل

ar X iv : h ep - p h / 96 08 32 5 v 1 1 4 A ug 1 99 6 HIGGS MASS PREDICTION

In this talk the Higgs boson effects in electroweak precision observables are reviewed and the possibility of indirect information on the Higgs mass from electroweak radiative corrections and precision data is discussed.

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

برای دانلود 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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1997