Cosmological Constant and the Evolution of the Universe

宇宙常数和宇宙的演化

• 批准号: 07304033
• 负责人: SATO Katsuhiko
• 金额: $ 4.1万
• 依托单位: The University of Tokyo
• 依托单位国家: 日本
• 项目类别: Grant-in-Aid for Scientific Research (A)
• 财政年份: 1995
• 资助国家: 日本
• 起止时间: 1995 至 1996
• 项目状态: 已结题
• 来源: https://kaken.nii.ac.jp/grant/KAKENHI-PROJECT-07304033/
• 关键词: Cosmological Constant; Inflation; Cosmic Microwave; Large Scale Structure; Chemical Evolution; Gravitational Leusing; de Sitter Space-Time; Age of the Universe; ハッブル定数; 相転移; 元素合成

1) Neutrino Background Radiation due to Supernove ExplosionRecently Superkamiokande project has started and it can observe the relic neutrino through supernove explostion. We investigated carefuly the spectrum of relic neutrino using the model for the chemical evolution of galaxies. The total flux depends strongly on the Hubble parameter, but weakly on the cosmological constant. We found that in the same flat universe model the flux in lambda=0 is smaller than that in lambda*o.2) Primordial NucleosynthesisThe primordial nucleosynthesis is best tool for deciding the baryon density. Recently, associated with the progress of techonology in obsevational field, the obsevational result pointed out that the simple model for cosmology has a trouble point. Some of people call the problem as 'crisis' in the universe. Hence, we taken account of the theoretical error in the lepton asymmetry universe and estimeted statistically the final fraction of the light elements by Monte Calro simulation. The result is that the best values for the degenerate parameter and the baryon density are 0.043(]SY.+-。[)0.040 and 0.015(]SY.+-。[)0.006-0.003 (CL.95 percent).

1)超新星爆炸的中微子背景辐射最近启动了超新星探测计划，它可以通过超新星探测来观测遗迹中微子。我们利用星系化学演化模型对残存中微子的光谱进行了详细的研究。总通量强烈地依赖于哈勃参数，而弱地依赖于宇宙常数。我们发现，在相同的平坦宇宙模型中，λ=0的通量比λ*0的通量小。2)原始核合成是决定重子密度的最好工具。近年来，随着宇宙学技术的进步，观测结果指出，简单的宇宙学模型存在一个问题。一些人把这个问题称为宇宙中的“危机”。因此，我们考虑了轻子不对称宇宙中的理论误差，并通过蒙特卡罗模拟对轻元素的最终分数进行了统计估计。结果表明，简并参数和重子密度的最佳值是0.043(]sy.+-。[)0.040和0.015()SY+-。[)0.006-0.003(CL.95%)。

项目成果

戸谷 友則: "Effects of neutrino oscillation on the Supernova Relic" International Journal Modern Physics D. 5. 519-527 (1996)

Tomonori Toya：“中微子振荡对超新星遗迹的影响”国际期刊现代物理学 D. 5. 519-527 (1996)

佐々木 節: "Can the Simplest Two-Field Model of Open Infation Survive?" Physical Review D. 54. 4705-4708 (1996)

Setsu Sasaki：“开放式膨胀的最简单的两场模型能够生存吗？物理评论 D. 54. 4705-4708 (1996)

K. Sato, T. Totani: "Spectrun of velic neutrino background from past supernovae and cosmological models" Astro particle Physus. 3. 367-376 (1995)

K. Sato，T. Totani：“来自过去超新星和宇宙学模型的速度中微子背景的光谱”天体粒子Physus。

Hideo Kodama: General Relativity. Bai-hu-kan, (1997)

儿玉秀夫：广义相对论。

戸谷反則: "Effects of neutrillo oscillation on the Superrora Relic" International Journal Modem Physics D. 5. 519-527 (1996)

Foul Toya：“中微子振荡对 Superrora Relic 的影响”国际期刊现代物理学 D. 5. 519-527 (1996)