Please use this identifier to cite or link to this item: https://hdl.handle.net/11147/5578
Title: Bianchi I model: An alternative way to model the present-day Universe
Authors: Russell, Esra
Kılınç, Can Battal
Pashaev, Oktay
Keywords: Early Universe
Large-scale structure of Universe
Cosmology
Issue Date: Aug-2014
Publisher: Oxford University Press
Source: Russell, E., Kılınç, C.B., and Pashaev, O. (2014). Bianchi I model: An alternative way to model the present-day Universe. Monthly Notices of the Royal Astronomical Society, 442(3), 2331-2341. doi:10.1093/mnras/stu932
Abstract: Although the new era of high-precision cosmology of the cosmic microwave background (CMB) radiation improves our knowledge to understand the infant as well as the presentday Universe, it also leads us to question the main assumption of the exact isotropy of the CMB. There are two pieces of observational evidence that hint towards there being no exact isotropy. These are: first, the existence of small anisotropy deviations from isotropy of theCMB radiation and secondly, the presence of large angle anomalies, although the existence of these anomalies is currently a huge matter of debate. These hints are particularly important since isotropy is one of the two main postulates of the Copernican principle on which the Friedmann Robertson Walker (FRW) models are built. This almost-isotropic CMB radiation implies that the universe is almost an FRW universe, as is proved by previous studies. Assuming that the matter component forms the deviations from isotropy in the CMB density fluctuations when matter and radiation decouples, we here attempt to find possible constraints on the FRW-type scale and Hubble parameter by using the Bianchi type I (BI) anisotropic model which is asymptotically equivalent to the standard FRW. To obtain constraints on such an anisotropic model, we derive average and late-time shear values that come from the anisotropy upper limits of the recent Planck data based on a model independent shear parameter of Maartens, Ellis & Stoeger and from the theoretical consistency relation. These constraints lead us to obtain a BI model which becomes an almost-FRWmodel in time, and which is consistent with the latest observational data of the CMB.
URI: https://doi.org/10.1093/mnras/stu932
http://hdl.handle.net/11147/5578
ISSN: 0035-8711
1365-2966
0035-8711
Appears in Collections:Mathematics / Matematik
Scopus İndeksli Yayınlar Koleksiyonu / Scopus Indexed Publications Collection
WoS İndeksli Yayınlar Koleksiyonu / WoS Indexed Publications Collection

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