  In this work, Emergent Universe scenario has been developed in general
homogeneous anisotropic model and for the inhomogeneus LTB model. In the first
case, it is assumed that the matter in the universe has two components - one is
perfect fluid with barotropic equation of state $p=\omega\rho$ ($\omega$, a
constant) and the other component is a real or phantom (or tachyonic) scalar
field. In the second case, the universe is only filled with a perfect fluid and
possibilities for the existence of emergent scenario has been examined.
