报告题目:
1. Gravitational Waves and their detection: Laser-interferometers on Earth
2. GW detection in space: projects of large space-borne laser interferometers
报告人:A. Ruediger教授,Albert-Einstein-Institute Hannover, Germany
摘 要:
1. Gravitational waves are a consequence of Einstein’s General Theory of Relativity. Time-derivatives of the mass quadrupole moment of celestial bodies are the source of such waves. The waves induce tiny strains in space-time, typically of the order 10^{-21} or less.
Michelson-type interferometers with arm-lengths in the km range have been constructed to detect such waves, yet without measuring any events. Therefore, a second generation of such antennas is under construction, with increased sensitivities. The technologies being pursued are discussed that lead to the desired improvements.
2. Gravitational waves of low frequencies (below 1 Hz) cannot be measured by terrestrial detectors, due to many noise contributions in that frequency range. Laser interferometers in space, with huge arm-lengths, have been proposed and are under active study. The most prominent of these, LISA, has been studied in a NASA/ESA collaboration. Its arm-lengths
of 5 million km will allow measuring GWs from cosmological events stemming from distant galaxies and involving massive black holes. The envisaged sensitivities would allow a deep insight into many cosmological questions. Other proposed space-borne GW detectors will also be discussed. The launch of the technology demonstrator mission, the LISA Pathfinder, is within a few years from now. It will verify the key technologies that are crucial for LISA, but also for other space missions using laser interferometry.
时间:
1. 2011年05月16日上午10:00点
2. 2011年05月17日上午10:00点
地点:科研楼五层物理所报告厅。
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详细讲解了LISA
网上的资料:http://bolide.lamost.org/translat/trans58.htm