Gravitational waves are distortions in space-time caused by massive objects accelerating, such as black holes colliding. They travel at the speed of light and stretch and compress space perpendicular to their direction of motion. This phenomenon was predicted by Einstein's theory of general relativity, which describes gravity as the curvature of space-time.
The detection of gravitational waves by LIGO in 2015 confirmed a major prediction of Einstein's theory of general relativity and opened a new way to observe the universe. It provided direct evidence of black holes and their collisions, offering insights into cosmic events that were previously undetectable.
LIGO uses laser interferometry to detect gravitational waves. It measures tiny changes in the distance between mirrors placed kilometers apart, caused by the stretching and compressing of space as gravitational waves pass through. These changes are on the order of a thousandth of the width of a proton.
When two black holes collide, they merge into a single, more massive black hole. During the collision, they emit gravitational waves, which carry away energy. For example, in the first detected event, two black holes of about 30 solar masses each merged, resulting in a black hole of 57 solar masses, with the remaining mass converted into gravitational waves.
Gravitational waves from distant events, like black hole collisions, are too weak to affect humans or Earth. However, if such an event occurred very close to Earth, the stretching and compressing of space could be felt, but this is highly unlikely given the vast distances involved.
Gravitational waves are not sound waves, but LIGO converts the detected signals into sound for analysis. The frequencies of these waves fall within the range of human hearing, making it possible to 'listen' to the universe. However, gravitational waves are distortions of space-time, not vibrations in air.
Gravitational waves travel through space at the speed of light, passing through matter without being significantly absorbed or scattered. They are highly penetrating and can traverse the entire universe, making them a powerful tool for observing cosmic events.
Rainer Weiss was one of the original architects of LIGO and a key figure in its development. He proposed the basic design of the interferometer used to detect gravitational waves and played a crucial role in advancing the project over several decades, culminating in the first detection in 2015.
LIGO faced skepticism, funding issues, and technical challenges in its early development. Many doubted the feasibility of detecting gravitational waves, and initial prototypes were small and limited in sensitivity. It took decades of innovation and collaboration to build the large-scale, highly sensitive detectors that eventually succeeded.
Future advancements include the development of space-based detectors like LISA, which will be sensitive to lower-frequency gravitational waves. This will allow the observation of events like the early stages of black hole mergers and other cosmic phenomena that are currently undetectable.
What is a gravitational wave? Janna Levin and comedian Matt Kirshen sit down with physicist Rainer Weiss to discuss LIGO, black holes, and the physics of gravitational waves.
(Originally Aired October 4, 2016)
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