Gravitational Wave Detection: Understanding Interferometers

In summary, interferometers work by detecting gravitational waves through the alteration of distance between two mirrors as they pass through. This is achieved by using the wavelength of a laser beam passing through the space. Despite initial confusion and claims that gravitational waves were not observable, it has been proven that there are solutions in general relativity that are not just coordinate waves. This can be compared to the observable expansion of the universe, where the spaces between galaxies expand, leading to an increase in the overall size of the universe.
  • #1
jeebs
325
4
My understanding of how interferometers work is that they detect gravitational waves because they alter the distance between two mirrors as they pass through. They do this by using the wavelength of a laser beam passing through this space.
However, shouldn't this always fail to detect anything, because the wave would always make the same fractional alteration to the photon wavelength as it does to the distance the light has to travel?
Why/how does this work?
thanks.
 
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  • #2
Yeah, we found gravitational waves.

(We need more funding. :wink: ) LOL! JK.
 
  • #3
Historically there was a lot of confusion on this issue. At one point, Einstein published a paper claiming that gravitational wave solutions in GR were in fact not observable. GR allows any kind of change of coordinates you like, including changes of coordinates that make the metric look oscillatory when written down on paper, without introducing any change in the actual physical properties of spacetime, such as curvature. This is known as a coordinate wave. However, it turns out that Einstein was wrong, and there really are gravitational wave solutions to GR that are not just coordinate waves. This may be helpful: http://en.wikipedia.org/wiki/Sticky...ents_on_the_properties_of_gravitational_waves

This is similar to the question of why cosmological expansion is observable, and IMO the cosmological expansion version is the easier one to understand. Rulers, solar systems, and galaxies don't expand, but the spaces between galaxies do. Therefore the size of the universe becomes bigger as measured by a ruler. More on this topic here: http://www.lightandmatter.com/html_books/genrel/ch08/ch08.html#Section8.2 (see subsection 8.2.5).
 
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Related to Gravitational Wave Detection: Understanding Interferometers

1. What are gravitational waves?

Gravitational waves are ripples in the fabric of space-time caused by the acceleration of massive objects. They were first predicted by Albert Einstein's theory of general relativity and were finally detected in 2015, confirming their existence.

2. How are gravitational waves detected?

Gravitational waves are detected using instruments called interferometers. These devices use lasers to measure tiny changes in the distance between two mirrors caused by passing gravitational waves.

3. What is an interferometer?

An interferometer is a scientific instrument that measures the interference pattern of two or more waves. In the case of gravitational wave detection, the waves being measured are laser beams reflecting off of mirrors that are affected by passing gravitational waves.

4. Why are interferometers important for detecting gravitational waves?

Interferometers are crucial for detecting gravitational waves because they are sensitive enough to measure the tiny changes in distance caused by these waves. They are also able to filter out other sources of interference, such as vibrations and background noise.

5. What is the significance of detecting gravitational waves?

The detection of gravitational waves has been hailed as one of the most significant scientific discoveries of the 21st century. It has opened up a new window into the universe, allowing us to study and understand phenomena that were previously inaccessible. It also confirms and further supports the theory of general relativity, paving the way for new advancements in our understanding of the universe.

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