使用“传统”技术，推动ET灵敏度
Pushing towards the ET sensitivity using 'conventional' technology
摘要：
最近，“爱因斯坦引力波望远镜”的设计研究在欧洲FP 7框架内得到了资助。该项目的宏伟目标是提供一个探测器的概念设计，其灵敏度比目前运行的仪器高出一百倍。预计这将需要开发和实施新技术，这些技术将超越第一代和第二代探测器所采用的概念。然而，想象一个迈克耳孙干涉仪是一个非常有趣和有教育意义的练习，在这个干涉仪中，传统技术已经被推到--或者可能超越--它们的极限，以达到爱因斯坦望远镜所设想的灵敏度。在本文中，我们提出了第一个粗略的分析，什么修改和改进是必要的，一步一步，从第二代引力波探测器的爱因斯坦望远镜。
英文摘要：
Recently, the design study `Einstein gravitational wave Telescope' (ET) has been funded within the European FP7 framework. The ambitious goal of this project is to provide a conceptual design of a detector with a hundred times better sensitivity than currently operating instruments. It is expected that this will require the development and implementation of new technologies, which go beyond the concepts employed for the first and second detector generations. However, it is a very interesting and educational exercise to imagine a Michelson interferometer in which conventional technologies have been pushed to - or maybe beyond - their limits to reach the envisaged sensitivity for the Einstein Telescope. In this document we present a first sketchy analysis of what modifications and improvements are necessary to go, step-by-step, from second generation gravitational wave detectors to the Einstein Telescope.
机构、总结、中文摘要均由AI分析而来，可能存在错误，请以论文正文为准。
