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Universal Journal of Applied Mathematics Vol. 2(2), pp. 99 - 103
DOI: 10.13189/ujam.2014.020204
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Homotopy Perturbation Method for Solving a Spatially Flat FRW Cosmological Model


Victor Shchigolev *
Department of Theoretical Physics, Ulyanovsk State University, 42 L. Tolstoy Str., Ulyanovsk 432000, Russia

ABSTRACT

In the present paper, we study a homogeneous cosmological model in Friedmann-Robertson- Walker (FRW) space-time by means of the so-called Homotopy Perturbation Method (HPM). First, we briefly recall the main equations of the cosmological model and the basic idea of HPM. Next we consider the test example when the exact solution of the model is known, in order to approbate the HPM in cosmology and present the main steps in solving by this method. Finally, we obtain a solution for the spatially flat FRW model of the universe filled with the dust and quintessence when the exact solution cannot be found. A comparison of our solution with the corresponding numerical solution shows that it is of a high degree of accuracy.

KEYWORDS
Cosmological Model, Exact and Approximate Solutions, Homotopy Perturbation Method

Cite This Paper in IEEE or APA Citation Styles
(a). IEEE Format:
[1] Victor Shchigolev , "Homotopy Perturbation Method for Solving a Spatially Flat FRW Cosmological Model," Universal Journal of Applied Mathematics, Vol. 2, No. 2, pp. 99 - 103, 2014. DOI: 10.13189/ujam.2014.020204.

(b). APA Format:
Victor Shchigolev (2014). Homotopy Perturbation Method for Solving a Spatially Flat FRW Cosmological Model. Universal Journal of Applied Mathematics, 2(2), 99 - 103. DOI: 10.13189/ujam.2014.020204.