Influence of Small-Scale Inhomogeneities on the Cosmological Consistency Tests

Abstract

The current cosmological dark sector (dark matter plus dark energy) is challenging our comprehension about the physical processes taking place in the Universe. Recently, some authors tried to falsify the basic underlying assumptions of such dark matter-dark energy paradigm. In this Letter, we show that oversimplifications of the measurement process may produce false positives to any consistency test based on the globally homogeneous and isotropic LCDM model and its expansion history based on distance measurements. In particular, when local inhomogeneity effects due to clumped matter or voids are taken into account, an apparent violation of the basic assumptions ("Copernican Principle") seems to be present. Conversely, the amplitude of the deviations also probes the degree of reliability underlying the phenomenological Dyer-Roeder procedure by confronting its predictions with the accuracy of the weak lensing approach. Finally, a new method is devised to reconstruct the effects of the inhomogeneities in a LCDM model, and some suggestions of how to distinguish between clumpiness (or void) effects from different cosmologies are discussed.

18 pages, 2 figures. Improved version accepted for publication as a Letter in MNRAS

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Cited by in corpus (5)

• Probing cosmic opacity at high redshifts with gamma-ray bursts
• Light propagation in inhomogeneous and anisotropic cosmologies
• Supernovae as probes of cosmic parameters: estimating the bias from under-dense lines of sight
• Studying light propagation in a locally homogeneous universe through an extended Dyer-Roeder approach
• Impact of small scale inhomogeneities on observations of standard candles