Spatial correlations of primordial density fluctuations in the standard cosmological model
David H. Oaknin

TL;DR
This paper challenges standard assumptions about the origin of primordial density fluctuations, proposing that causality constraints during the radiation era naturally produce scale-invariant anisotropies over large scales, altering the understanding of structure formation.
Contribution
The study revises the analysis of primordial density fluctuations by removing an unjustified approximation, revealing that causality during the radiation era leads to scale-invariant anisotropies over large volumes.
Findings
Density anisotropies are produced by standard physics during radiation domination.
Scale invariance arises from causality constraints at decoupling.
Amplitude of anisotropies is set by sub-horizon modes at decoupling.
Abstract
We revisit the {\it origin of structures problem} of standard Friedmann-Robertson-Walker cosmology to point out an unjustified approximation in the prevalent analysis. We follow common procedures in statistical mechanics to revise the issue without the disputed approximation. Our conclusions contradict the current wisdom and reveal and unexpected scenario for the origin of primordial cosmological structures. We show that standard physics operating in the cosmic plasma during the radiation dominated expansion of the universe produce at the time of decoupling scale invariant density anisotropies over cosmologically large comoving volumes. Scale invariance is shown to be a direct consequence of the causality constrains imposed by the short FRW comoving horizon at decoupling, which strongly suppress the power spectrum of density fluctuations with cosmologically large comoving wavelength.…
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Taxonomy
TopicsCosmology and Gravitation Theories · Relativity and Gravitational Theory · Dark Matter and Cosmic Phenomena
