https://www.selleckchem.com/pr....oducts/AZD2281(Olapa
The next generation interferometric gravitational wave detectors require arm lengths measured in tens of kilometers, with each cavity storing megawatts of optical power. The beams are contained in ultrahigh vacuum pipes. Scattered interferometer light in the pipes may reenter the cavities and inject extra noise. The pipes are, therefore, provided with optical baffles necessary to eliminate the scattered light. The design of the vacuum pipes and of the optical baffles is tightly intertwined. We present a thorough discussion tha
Like
Comment
Share
