Structured FRW universe leads to acceleration: a non-perturbative approach
Reza Mansouri

TL;DR
This paper presents a non-perturbative, exact general relativistic model of a structured universe that explains the observed acceleration and supernova dimming without dark energy by considering local inhomogeneities within a FRW background.
Contribution
It introduces a novel inhomogeneous cosmological model using LTB metrics embedded in FRW, with exact junction conditions, to mimic dark energy effects without modifying fundamental physics.
Findings
Structured universe explains supernova dimming without dark energy
Backreaction influences the global Hubble parameter
Exact relativistic treatment shows inhomogeneities can mimic acceleration
Abstract
We propose a model universe in the matter dominated phase described by a FRW background with local inhomogeneities, like our local patch, grown out of the primordial fluctuations. Our sub-horizon local patch consisting of different structures is approximated as an inhomogeneous cosmic fluid described by a LTB metric embedded in a background FRW universe, in which the observer could be located anywhere. Within the exact general relativistic formulation, the junction conditions for the only possible matching without a thin shell at the boundary, neglected so far in the literature, constrains the model in such a way that the luminosity distance-red shift relation mimics a FRW universe with dark energy. Therefore, the dimming of SNIa is accounted for in such a {\it structured} FRW universe. We have also calculated the exact general relativistic backreaction term and shown how it influences…
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Taxonomy
TopicsCosmology and Gravitation Theories · Galaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research
