Undergrad Doppler Gravity: Does it Exist? Why or Why Not?

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    Doppler Gravity
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SUMMARY

The discussion centers on the concept of whether gravity exhibits a Doppler-like effect, specifically if gravitational intensity varies based on the approach or recession of a massive object. Participants argue that while light and sound exhibit frequency shifts due to Doppler effects, gravity operates differently, governed by the stress-energy tensor rather than relativistic mass. The consensus is that gravity does not become stronger from an approaching object compared to a receding one, as gravitational waves require specific conditions, such as a non-zero second derivative of the quadrupole moment, to manifest.

PREREQUISITES
  • Understanding of the stress-energy tensor in general relativity
  • Familiarity with gravitational waves and their generation conditions
  • Knowledge of relativistic physics, particularly the effects of velocity on mass
  • Basic grasp of the Doppler effect in wave phenomena
NEXT STEPS
  • Study the mathematical framework of the stress-energy tensor in general relativity
  • Research the conditions necessary for generating gravitational waves
  • Explore the Aichelburg-Sexl ultraboost and its implications in relativistic physics
  • Examine the gravitational slingshot effect in Newtonian and relativistic contexts
USEFUL FOR

Physicists, students of general relativity, and anyone interested in the nuances of gravitational interactions and wave phenomena.

  • #31
.Scott said:
Let's have a flat universe with many stationary (in their frame) gravitation sources (perhaps galaxies) evenly disbursed.

Do you mean spatially flat (as in our best current model of our universe)? If there are gravitation sources present, spacetime can't be flat.

(Strictly speaking, isolated gravitating bodies, even if they are evenly distributed, won't lead to a spatially flat spacetime. But it could be spatially flat on average.)

.Scott said:
Taking this galaxy as our frame, will this galaxy accelerate?

Since you are assuming that all of the other gravitating bodies are evenly distributed, my answer would be no.

.Scott said:
If it does not, then gravity is doing something that I don't understand. Somehow it isn't really propagating at the speed of light - because our moving galaxy isn't "running into" this propagation and causing it to "bunch up".

I don't understand this reasoning; I don't know what you mean by "bunch up" or why you think this would happen. I suspect you have a confused concept of how gravity in GR works. Rather than try to use that confused intuition to try to analyze a scenario, you should try to retrain your intuition. The best way to do that is to work through a good textbook on GR. (Carroll's online lecture notes are a good start.)
 
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  • #32
PeterDonis said:
I don't know what you mean by "bunch up" or why you think this would happen.

The OP has prompted me to ask a very B level question -

Why is it invalid to compare a moving mass and its radiation of gravity to a moving light-bulb and its radiation of photons? Doesn't all matter emit gravitons all the time, and don't these gravitons move at c?
 
  • #33
Grinkle said:
Why is it invalid to compare a moving mass and its radiation of gravity to a moving light-bulb and its radiation of photons? Doesn't all matter emit gravitons all the time, and don't these gravitons move at c?
That's mixing classical and quantum pictures. And we have no quantum theory of gravity.

But, here is a simple question: Does a charge that is moving radially inward toward a stationary charged body encounter a different Coulomb force than a charge that is moving radially outward from that stationary body?
 
  • #34
Grinkle said:
Why is it invalid to compare a moving mass and its radiation of gravity to a moving light-bulb and its radiation of photons?

It's not invalid as a heuristic; the fact that moving charge emits EM radiation does make it reasonable to hypothesize that moving stress-energy emits gravitational radiation.

However, once you dig into the details, you find that there are significant differences. The Carlip paper I linked to in post #21 discusses the key ones, which can be summarized as:

(1) EM radiation is dipole at lowest order, whereas gravitational radiation is quadrupole. In other words, EM radiation is produced by any accelerating charge--i.e., when the second time derivative is nonzero--since that is sufficient to produce a time-varying dipole moment; but to produce gravitational radiation you need a time-varying quadrupole moment, which requires the third time derivative to be nonzero. (This is connected to the fact that the EM force is spin 1 while gravity is spin-2, and to the constraints imposed by conservation of momentum, which leads to the next point.)

(2) EM sources can be accelerated without having to add any further charges or currents to the system. However, gravitational sources (stress-energy) cannot be accelerated without adding further gravitational sources to the system, the sources of whatever energy is being used to produce the acceleration. This drastically constrains the kinds of scenarios you can consistently set up to test how gravity propagates; for example, as has already been commented, you can't just have a gravitating body like the sun disappear and ask how long it takes us to notice here on Earth.
 
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  • #35
jbriggs444 said:
Does a charge that is moving radially inward toward a stationary charged body encounter a different Coulomb force than a charge that is moving radially outward from that stationary body?

If both particles are the same distance away, I think no since the Coulomb force is a function of the distance.
 
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  • #36
.Scott said:
So light will blue shift (higher energy) and sound is louder and at a higher pitch.
So does that mean that you have or have not read up on gravitational redshift?
 
  • #37
MikeGomez said:
So does that mean that you have or have not read up on gravitational redshift?
That's a different topic.
 
  • #38
.Scott said:
the total change in momentum applied to the observer from the gravitational force
Umm, in general relativity there is no gravitational force, and the four momentum of an object in free fall does not change. The only way to get any of these quantities is to introduce a coordinate system and then you can look at the three momentum and the Christoffel symbols. That will be the closest you can get, but to do that you will have to specify the coordinates fully.
 

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