Confrontation of Cosmological Models with Observations

9319970 Klypin这是一项资助，用于在现代宇宙学模型中对各种天文物体形成的理论研究。其主要目标是在很大范围内对物体和结构进行详细的理论预测，并将这些预测与观测数据相比较。基本上所有可能的宇宙学相关尺度都将被考虑：从微波背景的波动，探测尺度大于100 Mpc，到10-100 Mpc尺度的超星系团和星系团，到1-10 Mpc尺度的星系团，再到亚兆秒差距尺度，这对星系形成的时代很重要。宇宙学模型的综合分析和模型与观测结果的对比是研究的重点，这些模型也涵盖了广泛的大小和不同类型的物体。

9319970 Klypin This is a grant for theoretical research of the formation of various types of astronomical objects in modern cosmological models. The main goal is to make detailed theoretical predictions for objects and structures for a very wide range of scales and to confront these predictions with observational data. Basically all possible cosmologically relevant scales will be considered: from the fluctuations of the microwave background, which probe scales larger then, say 100 Mpc, to superclusters and clusters of galaxies on 10-100 Mpc scales to galaxy clustering at 1-10 Mpc and to submegaparsec scales, which are important for the epoch of galaxy formation. Comprehensive analysis of cosmological models and confrontation of the models with observational results, which also cover a vast range of sizes and different types of objects, are the key points of the research.