The Fate of No-Scale Supergravity
No-Scale SU(5) Supergravity Models were long time considered to be ruled
out. However, they had not been analyzed with precise detail and recent
considerations of the achievement of the EWSB conditions opened up a
possibility to obtain realistic phenomenology. They are attractive due to
the relatively few free parameters with respect to a general MSSM.
One of the characteristics of these kind of models is the necessity of
supersymmetric spectra with masses around the few TeV region. The LHC
will be a good way to kill or to give hopes to realize them. I will
make a description of these models and explain the phenomenology that
could be accessed at the LHC.