Gravitational Waves and the Expansion of the Universe: Redshift or Not?

In summary, gravitational waves would redshift with the expansion of the universe, meaning their frequency would change as the universe expands. Although we have yet to detect them, the expected answer is yes and the reason for not detecting them may be due to their weak nature. Utilizing the GPS satellite network or the Apollo astronauts' mirrors on the moon as arms for an interferometer is not feasible. However, there is a project called LISA that plans to deploy a space-based GW detector with arms of 5 million km long. Unfortunately, the Lunar Laser Ranging setup is not accurate enough for detecting gravity waves. Gravity waves do carry angular momentum or spin.
  • #1
TEFLing
237
22
would gravitational waves redshift with the expansion of the universe ?
 
Space news on Phys.org
  • #2
Well, I don't know if "redshift" is the right term, but they would certainly change frequency in that way since they propagate at the speed of light and light redshifts.
 
  • #3
TEFLing said:
would gravitational waves redshift with the expansion of the universe ?
I agree with Phinds' conclusion, TEFLing. They would. Incoming wavelengths would be enlarged by the same factor as the distance between the source and us has grown while the waves were on their way here.
I.e. by the ratio a(now)/a(then)
 
  • #4
According to Keith Riles of the Michigan Gravitational Wave Group, the expected answer is yes - re: http://arxiv.org/abs/1209.0667. The answer is expected because we have yet to actually detect gravitational waves. The odds are, however, quite favorable given the outcome of the Hulse-Taylor study.
 
  • Like
Likes TEFLing
  • #5
What do people think the reason is for not detecting them yet? too weak or wrong frequency?
 
  • #6
Tanelorn said:
What do people think the reason is for not detecting them yet? too weak or wrong frequency?
Too weak, I think.
 
  • #7
Tanelorn said:
What do people think the reason is for not detecting them yet? too weak or wrong frequency?

From here: http://en.wikipedia.org/wiki/Gravitational_wave#Ground-based_interferometers

(Talking about the arms of the LIGO detectors, which have arms between 2 and 4 km long)
Even with such long arms, the strongest gravitational waves will only change the distance between the ends of the arms by at most roughly 10−18 meters.

10-18 meters is one attometer. For comparison, the diameter of a proton is about 1700 times this distance (1.755 femtometers).
 
  • Like
Likes Tanelorn
  • #8
Could the GPS satellite network, or something else like that, be utilized as the arms of an interferometer? Are the onboard clocks accurate enough to detect tiny time delays ?
 
  • #9
Didn't the Apollo astronauts leave a mirror on the moon? Could that comprise a nearly 400,000km arm?
 
  • #10
TEFLing said:
Could the GPS satellite network, or something else like that, be utilized as the arms of an interferometer? Are the onboard clocks accurate enough to detect tiny time delays ?

I'm not sure.

TEFLing said:
Didn't the Apollo astronauts leave a mirror on the moon? Could that comprise a nearly 400,000km arm?

One arm isn't enough and the return signal would be extremely weak, so I doubt it's a feasible option.
 
  • Like
Likes TEFLing
  • #11
TEFLing said:
Could the GPS satellite network, or something else like that, be utilized as the arms of an interferometer?

TEFLing said:
Didn't the Apollo astronauts leave a mirror on the moon? Could that comprise a nearly 400,000km arm?

Neither of these will work, because the distance between the ends of each arm (even assuming we could set up two perpendicular arms) has to be constant unless a gravitational wave is passing. Obviously "arms" where one end is the Moon or a GPS satellite and the other end is the Earth don't meet that requirement.

There is a project to deploy a space-based GW detector, called LISA; see here:

http://lisa.nasa.gov/

Its arms are planned to be about 5 million km long.
 
  • Like
Likes wabbit, berkeman and TEFLing
  • #12
Unfortunately the Lunar Laser Ranging setup is nowhere near the accuracy of dedicated gravity wave detectors like LIGO. The exact distance to the moon uncertain at any given instant due to a variety of factors. Orbital eccentricities, tidal flexture of both bodies, and even the weather affect its true distance. LLR instrument sensitivity is also an issue. The best achievable accuracy with the LLR setup is in the 2-3 cm range. These combined uncertainties are huge compared to the threshold accuracy required to measure gravitational wave amplitude. Note that there is a satellite version of LISA recently proposed, and discussed here, that could have an effective arm length of around 8 light minutes.
 
  • Like
Likes TEFLing
  • #13
Do gravity waves carry angular momentum / spin ?
 
  • #14
Yes, gravity waves are spin 2.
 
  • Like
Likes TEFLing and Tanelorn
  • #15
thanks dude :)
 
  • Like
Likes bapowell

Related to Gravitational Waves and the Expansion of the Universe: Redshift or Not?

1. What are gravity waves?

Gravity waves are ripples in the fabric of space-time caused by the acceleration of massive objects, such as stars or black holes.

2. How are gravity waves different from electromagnetic waves?

Gravity waves are fundamentally different from electromagnetic waves in that they are a result of the curvature of space-time, while electromagnetic waves are caused by oscillations in electric and magnetic fields.

3. What is redshift?

Redshift is a phenomenon in which light or other electromagnetic radiation from an object appears to have a longer wavelength, or shift towards the red end of the spectrum, due to the object's relative motion away from the observer.

4. How does gravity waves redshift occur?

Gravity waves redshift occurs when the source of the waves is moving away from the observer, causing the waves to appear to have a longer wavelength and lower frequency. This is similar to the Doppler effect seen with sound waves.

5. What implications does gravity waves redshift have?

Gravity waves redshift can provide valuable information about the distance and speed of the source object, as well as the strength and direction of the gravitational force acting on it. This can help scientists better understand the nature of the universe and how it evolves over time.

Similar threads

Replies
3
Views
1K
Replies
14
Views
851
Replies
1
Views
1K
Replies
0
Views
653
Replies
4
Views
1K
Replies
12
Views
876
Replies
2
Views
824
Replies
3
Views
1K
Replies
0
Views
596
Replies
9
Views
886
Back
Top