Evolution of density perturbations in fractional cosmology
S. M. M. Rasouli

TL;DR
This paper studies how matter density perturbations evolve in a fractional cosmology model, deriving exact solutions and constraining the fractional parameter using observational data.
Contribution
It introduces a fractional cosmological framework with non-local effects, deriving the modified growth equation, and constrains the fractional parameter using large-scale structure data.
Findings
The model admits both growing and decaying modes of density perturbations.
A stringent upper bound on the fractional parameter is found: $oxed{ ext{alpha} extless 1.07}$.
The growth of density perturbations shows distinctive fractional signatures.
Abstract
We investigate the evolution of matter density perturbations within a fractional cosmological framework inspired by fractal space-time constructions in field theory, where a deformation of the integration measure induces non-locality and memory effects in the dynamics. Working in the matter-dominated era and adopting a covariant fluid-flow approach, we derive the modified growth equation for the density contrast and obtain exact analytical solutions. The resulting dynamics depends explicitly on the fractional parameter and smoothly reduces to the corresponding standard case in the limit . We show that the model admits both growing and decaying modes, and we identify the parameter range in which structure formation is physically viable. Focusing on the growing mode, we compute the evolution of density fluctuations from recombination to the present epoch. By confronting…
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