Construction of theoretical models of dark energy and their observational constraints
| Project/Area Number |
20740148
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | Tokyo University of Science |
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Principal Investigator |
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| Project Period (FY) |
2008 – 2011
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| Project Status |
Completed (Fiscal Year 2011)
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| Budget Amount *help |
¥4,290,000 (Direct Cost: ¥3,300,000、Indirect Cost: ¥990,000)
Fiscal Year 2011: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
Fiscal Year 2010: ¥1,040,000 (Direct Cost: ¥800,000、Indirect Cost: ¥240,000)
Fiscal Year 2009: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
Fiscal Year 2008: ¥1,170,000 (Direct Cost: ¥900,000、Indirect Cost: ¥270,000)
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| Keywords | 暗黒エネルギー / 一般相対論 / インフレーション / 超弦理論 / 宇宙背景輻射 / 密度揺らぎ / 宇宙の大規模構造 / 暗黒物質 / 粒子生成 |
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| Research Abstract |
Observations such as supernova type Ia suggest that about 70% of the energy density of the Universe today consists of dark energy responsible for cosmic acceleration. The development of both theoretical and observational sides is required to approach the origin of dark energy. From the theoretical side I discriminated between many models of dark energy by studying the background cosmological dynamics, the evolution of density perturbations, and local gravity constraints. Moreover we placed constraints on theoretical models of dark energy from a number of independent observational data.
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Report
(6 results)
Research Products
(58 results)
