Geometrical Origin of Growth of Matter Perturbations

S S De; Farook Rahaman; Antara Mapdar

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arXiv · 2204.09490

Geometrical Origin of Growth of Matter Perturbations

S S De·Farook Rahaman·Antara Mapdar

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Abstract

The density perturbation of the universe has been considered in the framework of a Finslerian cosmological model in which the background spacetime of the universe is taken as the spatially flat FLRW spacetime with a Finslerian perturbation. The inhomogeneity in the matter(energy) density arises naturally in this consideration of gravity in the $( \alpha, \beta)$ - Finsler space for the background spacetime of the universe. The resulting inhomogeneous matter density indicates matter perturbation departing from the uniform density, and it is caused by the Finslerian perturbation in the Riemannian spacetime, thus ascertaining the geometrical origin of the growth of matter perturbation.

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S S De, Farook Rahaman, Antara Mapdar. 2022-04-19. Geometrical Origin of Growth of Matter Perturbations. https://arxiv.org/abs/2204.09490

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