TL;DR
This paper introduces a double power series method based on the FSN approach to analytically approximate solutions for cosmological perturbations, achieving high accuracy and providing a complete set of sub-horizon solutions.
Contribution
It adapts the FSN double power series method to cosmological perturbation theory, offering a new analytical approximation technique for sub-horizon scales.
Findings
Achieves ~1% accuracy compared to numerical solutions.
Provides a complete set of oscillating and non-oscillating solutions.
Includes a Mathematica implementation for practical use.
Abstract
We introduce a double power series method for finding approximate analytical solutions for systems of differential equations commonly found in cosmological perturbation theory. The method was set out, in a non-cosmological context, by Feshchenko, Shkil' and Nikolenko (FSN) in 1966, and is applicable to cases where perturbations are on sub-horizon scales. The FSN method is essentially an extension of the well known Wentzel-Kramers-Brillouin (WKB) method for finding approximate analytical solutions for ordinary differential equations. The FSN method we use is applicable well beyond perturbation theory to solve systems of ordinary differential equations, linear in the derivatives, that also depend on a small parameter, which here we take to be related to the inverse wave-number. We use the FSN method to find new approximate oscillating solutions in linear order cosmological perturbation…
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