In this work we have investigated the emergent scenario of the universe
described by Loop quantum cosmology model, DGP brane model and Kaluza-Klein
cosmology. Scalar field along with barotropic fluid as normal matter is
considered as the matter content of the universe. In Loop quantum cosmology it
is found that the emergent scenario is realized with the imposition of some
conditions on the value of the density of normal matter in case of normal and
phantom scalar field. This is a surprising result indeed considering the fact
that scalar field is the dominating matter component. In case of Tachyonic
field, emergent scenario is realized with some constraints on the value of
ρ1 for both normal and phantom tachyon. In case of DGP brane-world
realization of an emergent scenario is possible almost unconditionally for
normal and phantom fields. Plots and table have been generated to testify this
fact. In case of tachyonic field emergent scenario is realized with some
constraints on H˙. In Kaluza-Klein cosmology emergent scenario is
possible only for a closed universe in case of normal and phantom scalar field.
For a tachyonic field realization of emergent universe is possible for all
models(closed, open and flat).Comment: 13 pages, 16 figures, 1 table. arXiv admin note: text overlap with
arXiv:1105.109