Though it may initially seem tempting to use the expansion of the universe to assign a direction to time, the potential for re-collapse means that a more robust arrow is drawn from the thermodynamic properties of the evolving universe, effectively uniting the cosmological and thermodynamic arrows. Though we have established that the thermodynamic arrow is caused by the initial low entropy of the universe, there are several conflicting cosmological theories as to why such a state was formed.
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|Fig. 2: Gravitationally bound systems exhibit clumping as their entropy in-
| creases, where a gas with no such forces will evolve in the opposite
| manner.
Modern cosmology has arrived at two basic evolutionary routes which ac-
count for the low initial entropy; either the universe was created in some special, low entropy state, or that from the initial randomness of the universe a dynamical process caused, at least in our observable region, the low entropy we measure. Many contemporary cosmologists argue that the theory of inflation, normally used to explain cosmic geometry and symmetry, can result in such a selection of low entropy regions from a random universe. It has been suggested, however, that the selection of an unlikely region in some initial universe for which inflation will produce the expected results is equivalent to invoking the anthropic principle, and that such a selection would be dwarfed in chance by regions which already resemble our current observable universe. This view has been countered to the satisfaction of some, however the revised theory requires inflation in both time directions to be equally probable.
From controversial statements that there can be no cosmological constant in an inflationary universe, to the baby universes of string theory inheriting an arrow of time from their parent multiverse, recent papers have suggested a plethora of new possibilities which will stimulate research into the cosmological arrow for some time to come.