Gravitational Waves: Prevalence Across the Universe

In summary, gravitational waves of the magnitude currently detected by LIGO and similar detectors are prevalent throughout the known universe, with one detection every 2 months before reaching maximum sensitivity and potentially one per week after. These events are not heavily attenuated by distance or passing through galaxies, and there is no evidence for concentration in the Milky Way.
  • #1
roineust
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Would it be correct to say, that gravitational waves of the magnitude that is currently detected by LIGO and similar detectors, are prevalent to the extent that there is no single location in the known universe, that such magnitude of gravitational waves, don't pass through at least several times a year?
 
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  • #3
roineust said:
Would it be correct to say, that gravitational waves of the magnitude that is currently detected by LIGO and similar detectors, are prevalent to the extent that there is no single location in the known universe, that such magnitude of gravitational waves, don't pass through at least several times a year?
We are a single point in the Universe. How many events per year does LIGO report with high confidence?
 
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  • #4
LIGO lists its detections by year
https://www.ligo.caltech.edu/page/detection-companion-papers

https://www.ligo.caltech.edu/page/faq
"On average, over its first two observing runs, LIGO's detections have been made at a rate of one every 2 months, and this is before we reach so-called "design sensitivity" (which we expect to reach in 2020). The eleven confirmed detections made so far suggest that these kinds of events are relatively common. Once LIGO's detectors reach their maximum sensitivity, they could be detecting gravitational waves at a rate of one per week. The only way to refine the estimates of how often detectable gravitational waves pass, is to keep making detections! "
 
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More importantly, all known Ligo detections appear to come from distant extragalactic sources (like gamma ray bursts).
Since gravitational waves are not heavily attenuated either by distance or by passing through galaxies, only by inverse square spreading, we can guess that an observer in our general vicinity, but in an intergalactic void, would still see roughly the same number of gravitational wave events.
With just 11 confirmed detections, there is no statistical evidence for concentration in Milky Way disc or away from it, and no such concentration is expected.
Note that if most observed gravitational waves came from Milky Way, observers in intergalactic space would see less. But as stated, this is not the case.
 
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Related to Gravitational Waves: Prevalence Across the Universe

1. What are gravitational waves?

Gravitational waves are ripples in the fabric of spacetime caused by the acceleration of massive objects. They were first predicted by Albert Einstein's theory of general relativity.

2. How are gravitational waves detected?

Gravitational waves are detected using highly sensitive instruments called interferometers, which measure tiny changes in the distance between two objects caused by passing gravitational waves.

3. What is the significance of detecting gravitational waves?

The detection of gravitational waves provides evidence for the existence of black holes and other massive objects, and allows us to study the behavior of objects in extreme environments. It also confirms Einstein's theory of general relativity and opens up new avenues for studying the universe.

4. How prevalent are gravitational waves in the universe?

Gravitational waves are constantly being produced by a wide range of objects, from colliding black holes to the motion of planets and stars. However, they are very weak by the time they reach Earth, making them difficult to detect.

5. Can gravitational waves be used for communication or travel?

No, gravitational waves cannot be used for communication or travel as they are extremely weak and cannot be manipulated or controlled. They also travel at the speed of light, making them impractical for communication purposes.

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