Are gravitational waves bent by gravity?

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Discussion Overview

The discussion revolves around whether gravitational waves are bent by gravity, particularly in the context of massive objects like black holes. Participants explore the implications of gravitational lensing, the behavior of gravitational waves near event horizons, and the relationship between gravity and light in curved spacetime.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants propose that gravitational waves, like light, travel at the speed of light and may bend around massive objects, suggesting that the gravitational effect of a distant star could be altered by the presence of another star in between.
  • Others argue that if a massive object falls into a black hole, the gravitational waves it emits would also be affected by time dilation, leading to questions about when the event horizon actually expands from an outside observer's perspective.
  • A participant mentions that gravitational waves and light both travel in straight lines, but in curved space, this results in gravitational lensing, which could affect how we perceive gravitational influences.
  • There is a discussion about the nature of gravity and whether it can escape a black hole, with one participant questioning the apparent contradiction between gravity being able to influence the curvature of spacetime while light cannot escape.
  • Some participants suggest that the superposition principle might imply that gravitational waves should remain unaffected by other gravitational waves, depending on whether the discussion is framed classically or within a quantum gravity context.
  • One participant notes that any wave affected by gravitational time dilation will be bent, indicating a potential relationship between time dilation and the behavior of gravitational waves.

Areas of Agreement / Disagreement

Participants express a range of views on the bending of gravitational waves and the implications of black holes, with no clear consensus reached. The discussion remains unresolved regarding the specifics of how gravitational waves interact with massive objects and the nature of gravity in relation to black holes.

Contextual Notes

Participants highlight various assumptions, such as the definitions of gravitational waves and the effects of time dilation, which may influence their arguments. The discussion also touches on unresolved questions about the behavior of gravity and gravitational waves in extreme conditions.

michelcolman
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Gravitational waves travel at the speed of light. So do they also bend around massive objects? If we had an extremely sensitive differential accelerometer, would we "feel" a distant star to be where we saw it? This would seem logical if you consider the curved path of light to really be a straight line in a curved universe.

Also, what happens when a massive object passes the event horizon of a black hole? Nothing can escape from behind the event horizon, including gravity waves, so if we would fly around the black hole to map its gravitational field, the object would seem to remain forever at the event horizon. That's where it sent out its last gravitational wave with an update of its position to adjust space-time curvature around the black hole. And as more objects fell in later, the event horizon would expand so that successive objects would appear stuck at different distances, at least as felt by measuring their gravitational effect on the surrounding space.

So much for a black hole with no hair... OK, it would "really" have no hair, but it would feel like it did when you're outside. Right?
 
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1. Yes. If we could magically remove the sun out of space, the last of it's light would arrive at the same time as the last gravitational tug.

2. I know that time dilation shifts light from objects falling into a black hole to the red end of the spectrum the further they fall. I would expect that the gravitational waves would do the same thing: smooth over the event horizon asymptotically. It does seem to beg the question: At what time does the event horizon actually expand? As an outside observer, when does an object pass over the event horizon, if time dilation makes the object seem to approach stand-still. I don't know the answer.
 
gendou2 said:
1. Yes. If we could magically remove the sun out of space, the last of it's light would arrive at the same time as the last gravitational tug.
Yes, but would it also bend around a massive object in between? For example, suppose we would measure the gravity from a star, and then place another star in between, about halfway but slightly to the left from our point of view. Of course nothing will appear to change until the light of the new star reaches us. At that time, we will both see and feel the new star, while the old star will appear to be displaced to the right because of the curvature of light around the new star. But will the old star also "feel" more to the right if we could measure its gravity? Or in other words, will the combined gravity match the observed locations of the two stars rather than what we would ordinarily tend to consider their "real" location (even though "real" is really ill-defined, obviously)?
gendou2 said:
2. I know that time dilation shifts light from objects falling into a black hole to the red end of the spectrum the further they fall. I would expect that the gravitational waves would do the same thing: smooth over the event horizon asymptotically. It does seem to beg the question: At what time does the event horizon actually expand? As an outside observer, when does an object pass over the event horizon, if time dilation makes the object seem to approach stand-still. I don't know the answer.
I have to read up on black holes, I didn't know objects approached a standstill as they approached the event horizon. Of course in the reference frame of the falling object it will keep going, but I didn't know time dilation was strong enough to bring them to a halt in an outside reference frame.

I'm just guessing now, but if objects indeed slow down to an asymptotic crawl as they approach the event horizon, and at the same time the event horizon expands because of the added mass, that would be what tips them over the horizon. It's sort of tied to how you define the black hole: as soon as you start considering the new mass to be part of the black hole, it's suddenly inside the event horizon. But with the mass considered to be a foreign mass outside the black hole, it's still outside the event horizon. Or in yet other words, it could escape from the black hole, but parts of it can't escape from the combination of black hole + new object.

Weird things, those black holes. I hope I never meet one...
 
michelcolman said:
Yes, but would it also bend around a massive object in between?
Light and gravitational both waves travel in a strait line. Strait lines drawn in curved space result in gravitational lensing, which I think was your example. So, yes, we feel the lensed tug of gravity, just like we see the lensed shape of a distant galaxy.

michelcolman said:
... I didn't know objects approached a standstill as they approached the event horizon.
I originally heard this stated in "The Black Hole Wars" by Leonard Susskind
http://en.wikipedia.org/wiki/Black_hole#Before_the_falling_object_crosses_the_event_horizon

michelcolman said:
I'm just guessing now, but if objects indeed slow down to an asymptotic crawl as they approach the event horizon, and at the same time the event horizon expands because of the added mass, that would be what tips them over the horizon. It's sort of tied to how you define the black hole: as soon as you start considering the new mass to be part of the black hole, it's suddenly inside the event horizon. But with the mass considered to be a foreign mass outside the black hole, it's still outside the event horizon. Or in yet other words, it could escape from the black hole, but parts of it can't escape from the combination of black hole + new object.
You grasp what I have come to understand as an unsolved conceptual problem.
 
If gravity was lensed by gravity like light, how come gravity can excape a black hole to make it a black hole, but light can not?
 
Basically, when we say gravity moves at the speed of light, this really means that changes in gravity travel at the speed of light.

The actual field of gravity (the curvature of space-time) was created while the black hole was forming, and new matter falling in keeps updating this field until it reaches the event horizon.

The universe around the black hole simply remains "bent" the way it is, there's no need for any new gravity to escape the black hole and "feed" the field.
 
Correct me if I'm wrong, but doesn't the superposition principle means the answer is no? In other words, if a gravitational wave is truly just a vibration of the gravitational field, should it not remain unaffected by other gravitational waves?

I suppose this is affected by whether we look at gravity classically or whether your question is incorporated into a potential quantum gravity framework.
 
any wave affected by gravitational time dilation will be bent.
 
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