Cherenkov Reflections:Gamma-Ray Imaging and the Evolution of Tev Astronomy

切伦科夫反射:伽马射线成像与TeV天文学的演化

空间天文学

原   价:
1351.00
售   价:
1013.00
发货周期:预计3-5周发货
作      者
出  版 社
出版时间
2019年06月27日
装      帧
精装
ISBN
9789813276857
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页      码
300
语      种
英文
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库存 30 本
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图书简介
TeV gamma-ray astronomy is a mature and highly successful discipline with more than 200 established TeV point sources, many of which have been individually probed and studied in great detail. Much of the observational work is done using the now well-established imaging atmospheric Cherenkov technique. Quite how TeV gamma-ray astronomy has evolved to a 4th-generation of sophistication is a very interesting story, one that is neither well documented, nor appreciated across the broader astronomical community. This book documents how TeV gamma-ray astronomy painstakingly emerged from 20th century traditional cosmic-ray physics to become, in time, a keystone feature of contemporary high-energy astrophysics that is central to our understanding of high-energy processes and interactions in the cosmos, linking traditional particle physics to a multitude of astrophysical phenomena. The book tells the story from the perspective of the Whipple Observatory collaboration, the pioneers of the imaging technique. At the same time, the parallel developments in the broader community are constantly referred to, discussed and evaluated, at both TeV and PeV energies. The narrative traces all the contributions of the most important participants active in the field since the mid-1950s and critically evaluates and provides commentary on the progress of research until the first sources were discovered in the late 1980s and early 1990s. The final chapter presents a short summary of the contemporary status of TeV gamma-ray astronomy. The author takes the reader through many decades of exploration and investigation with the use of no more than a few equations. This book is suitable for astronomers, astrophysicists, experimentalists working across a variety of cognate disciplines including astronomy in different wavebands, particle physics, and high energy physics. Key Features: ○The first comprehensive review of the development of high-energy astronomy ○Uniquely puts together many aspects of the story into a coherent single source ○Timely review of the foundations and basic principles upon which CTA and other emerging facilities have been built
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