Particle Astrophysics with VERITAS

使用 VERITAS 进行粒子天体物理学

• 批准号: 0102786
• 负责人: Simon Swordy
• 金额: $ 26万
• 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: 2003
• 资助国家: 美国
• 起止时间: 2003-08-15 至 2005-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=0102786&HistoricalAwards=false
• 关键词: Particle; Astrophysics; VERITAS

Some of the most astounding recent discoveries about our universe have been made by telescopes and instruments collecting forms of natural radiation from space, that are invisible to the human eye. For example, the 2002 Nobel Prize in Physics was awarded to scientists who worked in collecting astrophysical X-rays and solar neutrinos. This proposal is to support groups at the University of Chicago and the University of California, Los Angeles (UCLA) for participation in the exploration of the next frontier in astronomy, the observation of high-energy gamma rays from space. The VERITAS (Very Energetic Radiation Imaging Telescope Array System) telescope is an array of collectors that detect the small light flashes produced by high-energy gamma rays interacting in the upper atmosphere. Several sources of this high-energy radiation have been discovered with earlier pathfinder telescopes. These sources apparently exist both within our galaxy and in energetic extragalactic objects. VERITAS can detect much fainter and more distant objects than existing telescopes, and is expected to discover many new sources of high-energy gamma rays.VERITAS is a collaboration of 10 institutions in the USA, Canada and Europe. The construction of the project is managed by the Smithsonian Astrophysical Observatory, with the project office located near Tucson, Arizona.Apart from an active involvement in the development of the science of this new astronomy, Chicago and UCLA have key roles in the construction of the VERITAS array hardware and software supported by this proposal. These activities include building key components of the camera at the focus of each VERITAS collector, and designing the way in which the data will be collected and recorded. The VERITAS array is at present under construction for completion in 2006. The first scientific results are expected to appear in 2005.

最近关于宇宙的一些最令人震惊的发现是通过望远镜和仪器收集来自太空的自然辐射形式而获得的，这些辐射是人眼看不见的。 例如，2002年诺贝尔物理学奖被授予致力于收集天体物理X射线和太阳中微子的科学家。 该提案旨在支持芝加哥大学和加州大学洛杉矶分校 (UCLA) 的团体参与探索天文学的下一个前沿，即从太空观测高能伽马射线。 VERITAS（高能辐射成像望远镜阵列系统）望远镜是一个收集器阵列，用于探测高能伽马射线在高层大气中相互作用产生的小闪光。 早期的探路望远镜已经发现了这种高能辐射的几个来源。 这些来源显然既存在于我们的银河系内，也存在于高能的河外天体中。 VERITAS 可以探测到比现有望远镜更暗、更远的天体，并有望发现许多新的高能伽马射线源。VERITAS 是美国、加拿大和欧洲 10 个机构的合作项目。该项目的建设由史密森天体物理观测站管理，项目办公室位于亚利桑那州图森附近。除了积极参与这一新天文学的科学发展之外，芝加哥和加州大学洛杉矶分校在该提案支持的 VERITAS 阵列硬件和软件的建设中发挥着关键作用。 这些活动包括在每个 VERITAS 收集器的焦点上构建相机的关键组件，以及设计数据收集和记录的方式。 VERITAS 阵列目前正在建设中，预计于 2006 年完工。第一个科学结果预计将于 2005 年出现。