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Inhomogeneity-Induced Cosmic Acceleration in a Dust Universe

Chia-Hsun Chuang, Je-An Gu, W-Y. P. Hwang

astro-pharXiv:astro-ph/0512651

Abstract

It is the common consensus that the expansion of a universe always slows down if the gravity provided by the energy sources therein is attractive and accordingly one needs to invoke dark energy as a source of anti-gravity for understanding the cosmic acceleration. To examine this point we find counter-examples for a spherically symmetric dust fluid described by the Lemaitre-Tolman-Bondi solution without singularity. Thus, the validity of this naive consensus is indeed doubtful and the effects of inhomogeneities should be restudied. These counter-intuitive examples open a new perspective on the understanding of the evolution of our universe.

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