  We consider the modifications to squark production in the presence of a
naturally heavier Dirac gluino. First generation squark production is highly
suppressed, providing an interesting but challenging signal find or rule out.
No dedicated searches for supersymmetry with a Dirac gluino have been
performed, however a reinterpretation of a "decoupled gluino" simplified model
suggests the bounds on a common first and second generation squark mass is much
smaller than in the MSSM: $\lsim 850$ GeV for a massless LSP, and no bound for
an LSP heavier than about 300 GeV. We compare and contrast the squark
production cross sections between a model with a Dirac gluino and one with a
Majorana gluino, updating earlier results in the literature to a $pp$ collider
operating at $\sqrt{s} = 14$ and 33 TeV. Associated production of squark+gluino
is likely very small at $\sqrt{s} = 14$ TeV, while is a challenging but
important signal at even higher energy $pp$ colliders. Several other salient
implications of Dirac gauginos are mentioned, with some thought-provoking
discussion as it regards the importance of the various experiments planned or
proposed.
