Has inflation really solved the problems of flatness and absence of relics?
Richard Lieu

TL;DR
The paper critically examines inflation theory's ability to solve flatness and relic problems, finding that classical density fluctuations challenge its effectiveness unless highly fine-tuned initial conditions are assumed.
Contribution
It provides a classical analysis of pre-inflationary density fluctuations, highlighting limitations and the need for fine-tuning in inflationary explanations of cosmological problems.
Findings
Density fluctuations on thermal scales hinder linear growth during inflation.
More than ~60 e-folds lead to larger fluctuations, causing false starts.
Super-homogeneous initial conditions are required to address flatness and relic issues.
Abstract
Among the three cosmological enigma solved by the theory of inflation, {\it viz.} (a) large scale flatness, (b) absence of monopoles and strings, and (c) structure formation, the first two are addressed from the viewpoint of the observed scales having originated from very small ones, on which the density fluctuations of the curvaton and relics are {\it inevitably} of order unity or larger. By analyzing strictly classically (and in two different gauges to ensure consistency) the density evolution of the smoothest possible pre-inflationary component -- thermal radiation -- it is found that the O(1) statistical fluctuations on the thermal wavelength scale present formidable obstacles to the linear theory of amplitude growth by the end of inflation. Since this wavelength scale exited the horizon at an early stage of inflation, it severely limits the number of e-folds of perturbative…
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