>>1134Rotation is around an axis: it is inhomogeneous and anisotropic. Dark energy is both homogeneous and isotropic. It doesn't fit.
Dark energy is an energy density. You could tie the value to a spin-like state of a particle in an n+1-dimensional box with a field that couples to spin to give the value of energy density we observe. The simplest field would be a scalar V, for an energy density of V*S, where S is the spin.
Because total radiation energy decreases as the universe expands, universe particles experience a force proportional to -V*S*dV/dx, where d/dx is the vector derivative along each of the box' n dimensions. This pushes positive S universes towards local absolute value minima, explaining the value more neatly than inflation which pushes towards regular minima, requiring anthropic reasoning to explain why we aren't negative-valued. Negative S universe are pushed towards local maxima.
Since our universe has been stable, we are either alone, or spin-spin interactions are rare. If we were to get hit, however, a number of things could happen:
1. Our spin changes, our position stays the same. The energy density suddenly, globally, instantaneously changes. For the universe to be a point particle with a time dimension equivalent to ours, locality is already broken, tough luck.
2. Our spin flips sign.
The universe suddenly starts shrinking, and shrinking increasingly rapidly until a local maximum is reached. Destruction of the universe in anywhere between 10 billion years and an hour.
3. We are pushed out of the local mimimum, and fall back. A sudden increase in dark energy density which slowly returns to present values.
4. We are pushed to another local minimum. Weirdly continuously varying dark energy densities, slowly decreasing in rate of change, finally stabilizing at some other minimum. Could be zero, could be negative (contraction), or positive. Could be big enough to have a big crunch or heat death rapidly.
5. We are pushed, and spin flips. Similar to above, except a maximum is reached and doom comes considerably quicker as a result.
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