These corrections are responsible for a surprising variety of phenomena, which all improve the behavior in classical cosmology. Nevertheless, they were not motivated by phenomenology but were derived through background-independent quantization. In most models and applications the corrected equations introduce different geometrical effects separately, rather than proceeding with complete effective equations including all quantum corrections. In this sense, such studies are phenomenological since they isolate specific effects. While some situations have already been supported by the rigorous effective equations discussed in Section 6, such a justification remains to be worked out in general; see  for a general discussion. Once all corrections are included, one has complete effective equations in a strict sense. This has been achieved so far only in one class of models; see Section 6.3. Most currently available models are incomplete but provide a wide range of perturbative calculations and have passed several non-trivial tests for consistent behavior.
Details of the derivation in cosmological models and of their technical origin will now be reviewed in Section 5, before we come to precise effective equations in Section 6 and a discussion of the link to the full theory in Section 7.
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