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by zmgsabst
1100 days ago
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There’s a debate over if the whole universe is rotating, called rotational anisotropy. At every scale below that you’re definitely rotating: cosmic filaments, clusters, and galaxies are all observed to rotate. As the theory goes, we’re seeing the small perturbations/rotations from when the universe was tiny inflated to cosmic scale. |
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Wait, debate ? Or am I failing to understand what you mean ?
\Lambda-CDM at the linear level requires the decay of vector-mode perturbations associated with vorticity; at the very least, the small scalar perturbations must totally dominate. This motivated a couple decades of searches for vector (and tensor) perturbations encoded in the CMB. Post-WMAP/Planck polarization data, aren't vector modes dead as a doornail in the linear theory ? (e.g. <https://journals.aps.org/prl/abstract/10.1103/PhysRevLett.11...> | <https://link.aps.org/accepted/10.1103/PhysRevLett.117.131302> aka astro-ph/1605.07178 which kills off early-time vorticity imho, conflicting with your final paragraph.)
I also know of some work on late-time vorticity, proposing studies of CMB lensing curl, kinetic SZ and moving-lens tomography, galaxy rotation planes and so forth, but isn't practically all of this work explicitly generating null-tests of \Lambda-CDM, rather than a cosmology where "the whole universe is rotating", Bianchi or otherwise ?
Finally, I also know of some work trying to use large N-body simulations to look at scales where predictions from the linear theory become unreliable (~ Mpc). However, I don't think this is what you mean.
If there is a published review of "a debate over if the whole universe is rotating" that you could direct me to, I would be grateful. I got nowhere with "rotational anisotropy" as a search term, and seem to lack the capacity to imagine possible synonyms other than as above. Don't spare me, I'm prepared to admit and embrace the consequences of my ignorance.