Neutrino Masses from Large Extra Dimensions
ArXiv hep-ph/9811448 (1998)
Authors:
Nima Arkani-Hamed, Savas Dimopoulos, Gia Dvali, John March-Russell
Abstract:
Recently it was proposed that the standard model (SM) degrees of freedom
reside on a $(3+1)$-dimensional wall or ``3-brane'' embedded in a
higher-dimensional spacetime. Furthermore, in this picture it is possible for
the fundamental Planck mass $\mst$ to be as small as the weak scale $\mst\simeq
O(\tev)$ and the observed weakness of gravity at long distances is due the
existence of new sub-millimeter spatial dimensions. We show that in this
picture it is natural to expect neutrino masses to occur in the $10^{-1} -
10^{-4}\ev$ range, despite the lack of any fundamental scale higher than
$\mst$. Such suppressed neutrino masses are not the result of a see-saw, but
have intrinsically higher-dimensional explanations. We explore two
possibilities. The first mechanism identifies any massless bulk fermions as
right-handed neutrinos. These give naturally small Dirac masses for the same
reason that gravity is weak at long distances in this framework. The second
mechanism takes advantage of the large {\it infrared} desert: the space in the
extra dimensions. Here, small Majorana neutrino masses are generated by
breaking lepton number on distant branes.