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It is often assumed that primordial perturbations are statistically isotropic, which implies, among other properties, that their power spectrum is invariant under rotations.
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Cited alongside, same era.
2007
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A. R. Liddle, “Information criteria for astrophysical model selection,” Mon. Not. Roy. Astron. Soc. Lett. 377
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2008
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2008
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2008
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2007
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