Accelerated expansion from structure formation

dc.creatorRasanen, Syksy
dc.date2006-07-27
dc.date2006-11-09
dc.date.accessioned2026-07-07T10:39:40Z
dc.date.available2026-07-07T10:39:40Z
dc.descriptionWe discuss the physics of backreaction-driven accelerated expansion. Using the exact equations for the behaviour of averages in dust universes, we explain how large-scale smoothness does not imply that the effect of inhomogeneity and anisotropy on the expansion rate is small. We demonstrate with an analytical toy model how gravitational collapse can lead to acceleration. We find that the conjecture of the accelerated expansion being due to structure formation is in agreement with the general observational picture of structures in the universe, and more quantitative work is needed to make a detailed comparison.
dc.description44 pages, 1 figure. Expanded treatment of topics from the Gravity Research Foundation contest essay astro-ph/0605632. v2: Added references, clarified wordings. v3: Published version. Minor changes and corrections, added a reference
dc.identifierhttps://arxiv.org/abs/astro-ph/0607626
dc.identifierhttp://arxiv.org/abs/astro-ph/0607626
dc.identifierJCAP0611:003,2006
dc.identifierdoi:10.1088/1475-7516/2006/11/003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/181111
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleAccelerated expansion from structure formation
dc.typetext

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