Can we distinguish Majorana and Dirac neutrinos in solar neutrino experiments ?

Details Can we distinguish Majorana and Dirac neutrinos in solar neutrino experiments ? Can we distinguish Majorana and Dirac neutrinos in solar neutrino experiments ?

1996-11-21

arxiv.org/abs/hep-ph/9611383v3

Nucl.Phys. B498 (1997) 39-54

Physics

High Energy Physics

High Energy Physics - Phenomenology

17 pages, LaTex, 3 Postscript figures, the cross-section Eq. (12) corrected in accordance with the new reference [24], section

Scientific paper

10.1016/S0550-3213(97)00289-7

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 $\nu_ee$-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 neutrinos since low energy recoil electrons ($T\geq 100 keV$) can be detected and electron energy and direction can be determined with good precision.

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