Interferometric detector

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LIGO tunnel in Hanford
Vacuum pumps and the evacuated tubes of the TAMA300

An interferometric detector is a detector that uses the interference effects of light to detect gravitational waves . The detector consists of two tunnels that meet at an angle of ninety degrees, in which laser beams are sent back and forth and come together again at a photodiode. If a gravitational wave from space hits this tunnel system, according to the general theory of relativity one of the two arms of the interferometer should contract while the other one expands and this should lead to differences in the time of flight of the laser beams. These spatial distortions are extremely small - even the most violent events in the universe would only change the relative length of the tunnels to the 20th place after the decimal point. For this reason, the interferometer arms of all gravitational wave detectors built so far are relatively long (up to four kilometers). However, the changes in length are smaller than the diameter of an atomic nucleus , so the measurements must be very precise.

Work according to this principle:

Under construction or planned are:

Web links

Individual evidence

  1. Cryogenic systems of the Cryogenic Laser Interferometer Observatory  ( page no longer available , search in web archivesInfo: The link was automatically marked as defective. Please check the link according to the instructions and then remove this notice.@1@ 2Template: Dead Link / www.iop.org