Atmospheric neutrino mixing and b-tau Unification

Details Atmospheric neutrino mixing and b-tau Unification Atmospheric neutrino mixing and b-tau Unification

2002-11-22

arxiv.org/abs/hep-ph/0211346v2

Phys.Lett.B556:185-191,2003

Physics

High Energy Physics

High Energy Physics - Phenomenology

11 pages, 2 Postscript figures, ReVTeX4

Scientific paper

10.1016/S0370-2693(03)00132-1

Extrapolating the tau and b masses in the MSSM tends to give for their ratio at the GUT scale a number around 1.2, for most viable values \tan \beta, rather than the minimal SU(5) prediction of 1. We suggest that this may be due to large off-diagonal elements in the charged lepton mass matrix M_L that can also explain the large atmospheric neutrino mixing angle. Several simple models with definite predictions for m_{tau}/m_b(M_{GUT}) are presented.

Affiliated with

Also associated with

No associations

Rating

Atmospheric neutrino mixing and b-tau Unification does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Atmospheric neutrino mixing and b-tau Unification, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atmospheric neutrino mixing and b-tau Unification will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-162249