The specific frequency and the globular cluster formation efficiency in
  Milgromian dynamics
  Previous studies of globular cluster (GC) systems show that there appears to
be a universal specific GC formation efficiency $\eta$ which relates the total
mass of GCs to the virial mass of host dark matter halos, $M_{vir}$ (Georgiev
et al 2010, Spitler & Forbes2009). In this paper, the specific frequency,
$S_N$, and specific GC formation efficiency, $\eta$, are derived as functions
of $M_{vir}$ in Milgromian dynamics, i.e., in modified Newtonian dynamics
(MOND). In Milgromian dynamics, for the galaxies with GCs, the mass of the GC
system, $M_{GC}$, is a two-component function of $M_{vir}$ instead of a simple
linear relation. An observer in a Milgromian universe, who interprets this
universe as being Newtonian/Einsteinian, will incorrectly infer a universal
constant fraction between the mass of the GC system and a (false) dark matter
halo of the baryonic galaxy. In contrast to a universal constant of $\eta$, in
a Milgromian universe, for galaxies with $M_{vir} <= 10^{12}\msun$, $\eta$
decreases with the increase of $M_{vir}$, while for massive galaxies with
$M_{vir}>10^{12}\msun$, $\eta$ increases with the increase of $M_{vir}$.
