OTTER
发表于 2025-3-23 11:35:47
Olusola Olasupo,Christopher Isiket gravitational wave detectors (GW) and now it is proposed for the future generation of the GW interferometers. In the following we summarize the history of GW detectors and we recall some of the basic principles of the cryogenic techniques. Then, we focus on the issues of cooling the mirrors of a GW interferometer.
arrhythmic
发表于 2025-3-23 16:20:49
E. Bauer,K. Kast,S. F. Tantono,W. Cenower levels, therefore the important issue of radiation pressure effects is addressed. Finally, a brief introduction to the topic of diffraction limited beams and high order transverse electromagnetic modes is included.
过份好问
发表于 2025-3-23 19:39:58
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易受骗
发表于 2025-3-24 01:32:28
https://doi.org/10.1057/9780230508361 limited by the Heisenberg Uncertainty Principle, giving rise to the interferometric Standard Quantum Limit for 40 kg test masses. This chapter will give a basic outline of the concepts currently under consideration for surpassing the Standard Quantum Limit.
Dungeon
发表于 2025-3-24 04:43:57
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conjunctiva
发表于 2025-3-24 08:51:25
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烧烤
发表于 2025-3-24 11:01:58
E. Bauer,K. Kast,S. F. Tantono,W. Cenaser interferometers. This chapter introduces the working principles of the different optical configuration that were and will be used in gravitational wave detectors: Michelson interferometer, Fabry-Perot resonant cavity, power and signal recycling techniques. Advanced detectors will feature high p
Substance
发表于 2025-3-24 18:47:53
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腐败
发表于 2025-3-24 21:32:03
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anatomical
发表于 2025-3-25 00:56:38
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