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Brian, hope it's OK to interject. I think the main agenda here is to resolve the cosmological singularity and provide either for inflation or for a substitute mechanism.
Renaldi, in the invited review article I mentioned, mentions string cosmology, loop cosmology, Horava, Jacobson's Einstein-aether, and various others. He gives a brief historical account of the earlier attempts which preceded and led up to these approaches---particularly the first two. In one form or another, most of these involve a bounce.
You might want to glance at the relevant section, which is just 2 pages long. It is section 2 "Lines of Research" and begins on page 2. Here's an excerpt.
==Rinaldi review article http://arxiv.org/abs/1201.4543 page 3==
There are several other models that offer alternatives to the direct quantization of gravity. Recently, Horava has proposed a power-counting renormalizable theory of gravity, based on an anisotropic scaling at high energy 20. Essentially, the fundamental hypothesis is that time and space do not scale in the same way, according to the scheme t → bzt, xi → bxi, where z is called critical (Lifschitz) exponent and b is an arbitrary constant. By adding higher spatial curvature terms to the standard Einstein-Hilbert action, one can construct a model where, at high energy z ≥ 3, which makes the theory power-counting renormalizable, while at low energy z = 1. Local Lorentz invariance is preserved in the infrared (IR), and it is broken in the UV. The original formulation of this model suffered from un unwanted ghost scalar field, that persisted also in the IR 21,22. To remove this anomalous degree of freedom one needs to add new terms in the action, that are basically formed by combination of a vector field, orthogonal to constant time surfaces, and its derivatives 23. In this form, the Hoˇrava-Lifschitz theory becomes very similar to the “Einstein-aether” theory proposed by Jacobson many years before as a vector-tensor theory of gravity 24. Both theories offer non-singular solution to the cosmological equations 25,26 and the horizon problem is solved without recurring to inflation 27.
==endquote==
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