2009 Fiscal Year Final Research Report
Cosmological scenario based on inhomogeneous models
Project/Area Number |
19540279
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Research Category |
Grant-in-Aid for Scientific Research (C)
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Allocation Type | Single-year Grants |
Section | 一般 |
Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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Research Institution | Nagoya University |
Principal Investigator |
NAMBU Yasusada Nagoya University, 大学院・理学研究科, 准教授 (40212112)
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Project Period (FY) |
2007 – 2009
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Keywords | 非一様宇宙 / 平均化ボイド / 光度距離 / ダークエネルギー |
Research Abstract |
Void models provide a possible explanation of the "accelerated expansion" of the Universe without dark energy. To make the conventional void models more realistic, we allow the void, an under-dense region around us, to be anisotropic and consider an average of the distance-redshift relations over the solid angle subtended at the observer. We first show that after taking the average of a form of the optical scalar equation (distance equation), the effective distance equation we obtain coincides with the one for the Lema^itre-Tolman- Bondi universe with a Dyer-Roeder-like extension. We then numerically solve the equation to compare with observational data of Type Ia supernovae. We find that anisotropy allows smaller size of void and larger Ωm.
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Research Products
(6 results)
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[Remarks] [プレプリント] M. Tanimoto and Y. Nambu and K. Iwata“The role of anisotropy in the void models without dark energy"arXiv:0906.4857 [astro-ph.CO] (2009)
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[Remarks] [他大学でのセミナー]東京工業大学宇宙理論グループセミナー“The role of anisotropy in the void models without dark energy"2009年5月12日講演者:南部保貞