U.S.-Hungary Cooperative Science Research in Cosmology

美国-匈牙利宇宙学合作科学研究

• 批准号: 9107499
• 负责人: David Schramm
• 金额: $ 4.5万
• 依托单位: University of Chicago
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 1991
• 资助国家: 美国
• 起止时间: 1991-09-01 至 1995-02-28
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9107499&HistoricalAwards=false
• 关键词: U.S.; Hungary; Cooperative; Science; Research

The primary objective of this US-Hungary Cooperative Science Research Project between Dr. David Schramm of the University of Chicago and Dr. Alex Szalay of Eotos University, Budapest is to continue the collaboration of US and Hungarian researchers working on problems in cosmology and high energy astrophysics. The observational and theoretical research relates to the formation and the statistical description of the structure of the universe and will be applied to problems in many areas such as Biased Galaxy Formation, Fluctuation Spectrum; Pencilbeam Redshift Surveys; Higher Order Correlations and Clusters of Galaxies; Particle Physics and Early Universe; and Gamma Ray Bursters and Gamma Ray Background. The results may provide information on new observations and by extraction from existing unique data. Methodology may be extended by the effort to develop models in which a structure such as a supercluster can be formed from first principles. This project in cosmology fulfills the program objective of advancing scientific knowledge by enabling leading experts in the United States and Eastern Europe to combine complementary talents and pool research resources in areas of strong mutual interest and competence.

芝加哥大学的戴维·施拉姆（David Schramm）博士与布达佩斯Eotos大学的Alex Szalay博士之间的这项US-Hust合作科学研究项目的主要目标是继续美国与匈牙利研究人员的合作，从事宇宙学和高能天文学问题的问题。 观察和理论研究与宇宙结构的形成和统计描述有关，并将应用于许多领域的问题，例如偏见的星系形成，波动谱； 铅笔红移调查；星系的高阶相关和簇；粒子物理和早期宇宙；以及伽马射线汉堡和伽马射线背景。 结果可能会提供有关新观察结果的信息，并通过从现有的唯一数据中提取。 方法可以通过开发模型来扩展方法，在这种模型中可以从第一原理中形成诸如超集群之类的结构。 宇宙学项目实现了计划的目标，即通过使美国和东欧的主要专家能够将互补才能和汇总研究资源结合在一起，以促进科学知识。