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The dynamics of a (3 + 1) dimensional homogeneous anisotropic universe ismodified by Loop Quantum Cosmology and, consequently, it has generically a bigbounce in the past instead of a big-bang singularity. This modified dynamicscan be well described by effective equations of motion. We generalise theseeffective equations of motion empirically to (d + 1) dimensions. Thegeneralised equations involve two functions and may be considered as a class ofLQC -- inspired models for (d + 1) dimensional early universe cosmology. As aspecial case, one can now obtain a universe which has neither a big bangsingularity nor a big bounce but approaches asymptotically a `Hagedorn like'phase in the past where its density and volume remain constant. In a fewspecial cases, we also obtain explicit solutions.

A Class of LQC--inspired Models for Homogeneous, Anisotropic Cosmology in Higher Dimensional Early Universe