  In this theoretical study, we report an investigation of the equations of
state (EoSs) ofhyper-nuclear matter and its composition as a function of
density within the framework of effective field theory motivated relativistic
mean field model. We have used G2 force parameter along with various
hyperon-meson coupling ratios by allowing the mixing and the breaking of SU(6)
symmetry to predict the EoSs, keeping the nucleonic coupling constant intact.
We have estimated the properties of non-rotating and rapidly rotating
configuration of compact stars by employing four different representative sets
of equations of state. The obtained results of the mass and radius for the
compact stars are compared with the recent mass observations. Further, we have
studied the stability and sensitivity of rotational frequency (at
sub-millisecond period) on the configuration of the compact stars, because the
angular frequency is significantly smaller than the mass-shedding (Keplerian)
frequency in slow rotation regime. Moreover, the yield of hyperon as a function
of density for various hyperon-meson couplings are also estimated.
