Tidal Forces in Accelerating Frames

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Discussion Overview

The discussion revolves around the effects of tidal forces and brightness of stars as experienced by an observer in an accelerating spaceship. Participants explore concepts related to gravitational effects, the equivalence principle, and the relationship between a star's brightness and its gravitational influence, considering both local and global perspectives in spacetime.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • One participant suggests that as they accelerate, the brightness of stars increases due to their position in a pseudo gravity well, questioning if tidal forces increase with brightness.
  • Another participant clarifies that brightness increases gradually as the ship's velocity relative to the stars increases, and that tidal forces also increase gradually as the observer gets closer to the star.
  • There is a discussion about the relationship between a star's brightness, luminosity, and distance, with some participants noting that brighter stars are not always more massive.
  • A participant proposes that if an observer's clock experiences significant time dilation, they might perceive the gradual brightening of stars as happening quickly, under high acceleration.
  • One participant argues that the gravitational pull of a star is determined by the stress-energy tensor and is not affected by the observer's velocity relative to the star.
  • Another participant challenges the assumption that a star gains potential energy during acceleration, stating that the equivalence principle only applies locally and does not hold in this scenario.

Areas of Agreement / Disagreement

Participants express differing views on the relationship between brightness and tidal forces, the implications of acceleration on gravitational effects, and the validity of assumptions regarding potential energy. No consensus is reached on these points.

Contextual Notes

Participants highlight limitations in applying the equivalence principle over large patches of spacetime and the complexity of relating brightness to gravitational effects, indicating unresolved assumptions and dependencies.

jartsa
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Let's say I'm floating in space in a spaceship, and there are some stars around.

Now I turn on powerful spaceship engines. This causes a huge acceleration, which causes the brightness of some stars to increase a lot. (Those stars that are up in the pseudo gravity well become bright)

Does tidal force from a star increase as much as its brightness?

If the star is able to shine brightly, it contains a lot of energy, so it exerts a large gravitational force on those observers that say that it's a bright star, right?
 
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jartsa said:
Now I turn on powerful spaceship engines. This causes a huge acceleration, which causes the brightness of some stars to increase a lot. (Those stars that are up in the pseudo gravity well become bright)

Not immediately. They will only become brighter as your ship's velocity relative to them increases. This is an example of how the equivalence principle only works locally: in a small patch of spacetime, you can equate acceleration with being at rest in a gravitational field, but globally, you can't.

jartsa said:
Does tidal force from a star increase as much as its brightness?

The brightness does not increase at once, as above. The tidal force from the star doesn't increase at once, either; it will increase gradually as you get closer to the star. Also, your acceleration has no effect on the tidal force you experience from the star.

jartsa said:
If the star is able to shine brightly, it contains a lot of energy, so it exerts a large gravitational force on those observers that say that it's a bright star, right?

The brightness of the star is a function of its luminosity and your distance from it. There is a relationship between mass and luminosity, but it's not the simple one you appear to be implicitly assuming; brighter stars are more massive in some cases, but not all.
 
PeterDonis said:
Not immediately. They will only become brighter as your ship's velocity relative to them increases. This is an example of how the equivalence principle only works locally: in a small patch of spacetime, you can equate acceleration with being at rest in a gravitational field, but globally, you can't.

Oh yes. Gradual change of brightness seems to spoil my simple idea.

The brightness does not increase at once, as above. The tidal force from the star doesn't increase at once, either; it will increase gradually as you get closer to the star. Also, your acceleration has no effect on the tidal force you experience from the star.

I would like to eliminate the effect of the change of distance. If observer's clock becomes quickly time dilated, then the observer will say that the gradual brightening of the star happens quickly, and the star does not have time to move much during that time. This is the situation when the acceleration is sufficiently high.

The brightness of the star is a function of its luminosity and your distance from it. There is a relationship between mass and luminosity, but it's not the simple one you appear to be implicitly assuming; brighter stars are more massive in some cases, but not all.

I just want to assume that the star gains potential energy when I start to accelerate, and I can feel the gravitational force of that extra energy.
 
jartsa said:
If the star is able to shine brightly, it contains a lot of energy, so it exerts a large gravitational force on those observers that say that it's a bright star, right?
If the increased brightness is a consequence of the star moving towards the observer in the observer's rest frame then presumably the star dims by the same amount in the opposite direction in that frame. If so then the amount of energy being emitted by the star, measured in the observer's rest frame, may not have changed, and hence there is no reason to expect observer to perceive the gravitation of the star as having increased.

But a cleaner way to look at it is that the 'gravitational pull' of the star is a function of the stress-energy tensor, which is a coordinate-independent item, not of a coordinate-dependent measurement of mass-energy. So the observer's perception of the gravitation of the star via phenomena such as tidal effects cannot be affected by the observer's velocity relative to the star.
 
jartsa said:
If observer's clock becomes quickly time dilated,

It doesn't.

jartsa said:
I just want to assume that the star gains potential energy when I start to accelerate, and I can feel the gravitational force of that extra energy.

You may want to assume this, but that doesn't mean it's correct. It isn't.

Once again: the EP only works locally. Your scenario is not local; it covers a large patch of spacetime, including your ship and the star. A "pseudo-gravity" field due to acceleration is not equivalent to a real gravitational field over this large patch of spacetime; suddenly accelerating your ship does not instantly create the effects you are talking about.
 

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