Does GR reduce gravitational force on a planet's surface?

In summary: words, the force of gravity between two plates is the same whether the plates are at the same altitude or at different altitudes.
  • #1
Shaw
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3
Am I correct in thinking that the force of gravity between 2 test objects at rest on a planet's surface is less than it would be for the same objects at rest in deep space? I understand that this occurs because in GR gravitational potential has a mass value which is lost on the surface, while the mass's themselves still retain the same value. If this is correct, does it require a difficult GR calculation? Thanks
 
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  • #2
I don't understand your question, but gravity is not a force in GR (as it is in Newtonian classical physics), it is a simple consequence of spacetime geometry.
 
  • #3
Shaw said:
Am I correct in thinking that the force of gravity between 2 test objects at rest on a planet's surface is less than it would be for the same objects at rest in deep space?

As phinds pointed out, in GR gravity is not a force; it's spacetime curvature. But if spacetime curvature is weak enough, and objects are moving slow enough, we can approximate the effects of gravity as a Newtonian force, which can be measured by a Cavendish experiment. If we consider running such an experiment with two objects in deep space, and then moving the two objects to a planet's surface and running the experiment again, the results would be the same in both cases. So in this sense, I think the answer to your question is "no".
 
  • #4
PeterDonis said:
As phinds pointed out, in GR gravity is not a force; it's spacetime curvature. But if spacetime curvature is weak enough, and objects are moving slow enough, we can approximate the effects of gravity as a Newtonian force, which can be measured by a Cavendish experiment. If we consider running such an experiment with two objects in deep space, and then moving the two objects to a planet's surface and running the experiment again, the results would be the same in both cases. So in this sense, I think the answer to your question is "no".
Thanks for this. The opinion I received from a prof. of Engineering, who also has a degree in mathematical physics, was that there would be a discrepancy for the reasons I mentioned, so I was just trying to nail that down. It sounded right to me, but I can't find any information on the subject on the internet.
 
  • #5
PeterDonis said:
If we consider running such an experiment with two objects in deep space, and then moving the two objects to a planet's surface and running the experiment again, the results would be the same in both cases. So in this sense, I think the answer to your question is "no".
Um, but it won't be the same in both cases. The objects will have different potential energy, and that contributes to their gravitational pull. So the answer is "yes".
 
  • #6
georgir said:
The objects will have different potential energy, and that contributes to their gravitational pull. So the answer is "yes".
Gravitational potential energy is a property of the system of objects, not of one particular object. The Equivalence Principle indicates that at least for small separations of the 2 test objects the answer is "no".
 
  • #7
Thanks georgic and A.T. for these replies. I guessed that the force on the surface might be a little less because if we take the grav. potential energy, which equals the kinetic energy at the escape velocity, and use E=mc^2 to convert it into mass, we can plug the values for a particular example, say the Earth, into the equation V^2/V^2max + m1^2/m^2 = 1. V = 11.2 km/sec, m is a test object's mass, let's say 1kg, m1 is 1kg - .62 micrograms (the mass we get from E=mc^2) and Vmax is the highest value for the velocity. If we solve for Vmax we get c, or near enough (we don't need to use E=mc^2; we could just use the experientially derived value.) Any comments about this?
 
  • #8
Let's say we are in an accelerating spaceship. We have two massive plates that stick together gravitationally. The force is large enough to keep plate B hanging on plate A when we lift plate A up.

Now we grab the plate A, and the plate B hanging on plate A, and start climbing down a rope.

Before we have reached the Rindler-horizon, the plates will have been pulled apart. This is easy to calculate.

In a homogeneous gravity field things are exactly the same as in an accelerating spaceship.

Force of gravity between two plates is less when the plates are at a lower position.
 
  • #9
georgir said:
The objects will have different potential energy, and that contributes to their gravitational pull.

"Potential energy" relative to what? Relative to infinity, yes; but we're not measuring their gravitational pull relative to infinity. Relative to each other, since by hypothesis they are both at the same altitude in the field, their gravitational pull is unchanged.

In other words, moving the pair of objects from infinity to some finite altitude in a gravity well does not change the objects locally at all.
 
  • #10
jartsa said:
The force is large enough to keep plate B hanging on plate A when we lift plate A up.

This doesn't make sense. The plates should be separated horizontally, not vertically; otherwise they are not at the same "gravitational potential", which they must be by the OP's hypothesis, at least as I understand it.

If the plates are allowed to be separated vertically, then of course you can change their separation by going to a regime where the change in proper acceleration from one plate to the other is large enough (close enough to the Rindler horizon in the flat spacetime case, or deep enough in the gravity well in the curved spacetime case). But that's not changing the "force of gravity" produced by the plates.
 
  • #11
Thanks for this. Has anyone actually done the experiment comparing the force of gravity between two objects on the surface of the Earth with the force in space? A good test of GR I would think. I can't find any reference to it if it has. The effect would not show up in the orbits of the planets because inertial and gravitational mass would change together.

Another related matter, the time dilation on the surface of a planet equals the time dilation at that planet's escape velocity - generally considered an odd coincidence. Isn't it also a little odd that we can use the mass energy value of the escape velocity, and without reference to E=mc^2 (we only need to use the experimentally derived per unit mass energy value) calculate a value equal to c? Are there several ways to calculate c other than Maxwell's?
 
  • #12
Shaw said:
Has anyone actually done the experiment comparing the force of gravity between two objects on the surface of the Earth with the force in space?

I don't know that anyone has done a Cavendish experiment in space, which would be the definitive test.
 
  • #13
jartsa said:
Let's say we are in an accelerating spaceship. We have two massive plates that stick together gravitationally. The force is large enough to keep plate B hanging on plate A when we lift plate A up.

Now we grab the plate A, and the plate B hanging on plate A, and start climbing down a rope.

Before we have reached the Rindler-horizon, the plates will have been pulled apart. This is easy to calculate.

In terms of a local frame of reference, as you descend down the rope, absolutely nothing happens to the force between the plates, but the proper acceleration needed to hold station on the rope increases. So of course the plates separate. How does this show that "gravity is weaker"?

As long as you use local measurements (local clocks, rulers, and scales), the laws of physics (as modeled by General Relativity, at least) don't depend on your location, or the gravitational potential of your location.
 
  • #14
PeterDonis said:
This doesn't make sense. The plates should be separated horizontally, not vertically; otherwise they are not at the same "gravitational potential", which they must be by the OP's hypothesis, at least as I understand it.

If the plates are allowed to be separated vertically, then of course you can change their separation by going to a regime where the change in proper acceleration from one plate to the other is large enough (close enough to the Rindler horizon in the flat spacetime case, or deep enough in the gravity well in the curved spacetime case). But that's not changing the "force of gravity" produced by the plates.

I'm so lazy that I copy-paste and edit:

If the plates are allowed to be separated vertically, then of course you can change their separation by going to a regime where the proper acceleration is large enough (close enough to the Rindler horizon in the flat spacetime case, or deep enough in the gravity well in the curved spacetime case).

We might say that the "force of gravity" produced by the plates changed. Or we might say the "force of gravity" produced by the acceleration changed.I happen to like the first alternative. Because ... a mountain climber causes a constant tension on a rope, when he climbs down the rope in a uniform gravity field. I mean the anchor does not break away from the rock, no matter how far the climber descends. Right?
 
  • #15
jartsa said:
That might be changing the "force of gravity" produced by the plates. Or it might be changing the "force of gravity" produced by the acceleration.

No, it can only be the second. The first alternative won't work. See below.

jartsa said:
a mountain climber causes a constant tension on a rope, when he climbs down the rope in a uniform gravity field

What is a "uniform gravity field"? If by that you mean "proper acceleration does not change with height", then the thought experiment you describe is not a "uniform gravity field"; the Rindler horizon is associated with a congruence of Rindler observers, and their proper acceleration varies with height above the horizon. So the tension in the rope caused by the climber won't be constant.

If, OTOH, you insist on a congruence of observers whose proper acceleration is constant, then this is the Bell congruence, and they are not at rest relative to each other. (More precisely, the expansion scalar of the Bell congruence is nonzero, which means it is not rigid.) So you can't use that congruence to model a static "gravitational field" in your thought experiment. The rope that the mountain climber is climbing down will be stretched further and further as time goes on, even if the climber is not there.
 
  • #16
In SR we see time and mass changing together, so if time changes in a gravitational field isn't it worth checking to see if there's some kind of mass change as well? It just seems like due diligence to me. I may be naive about this but 2 test objects at rest in deep space have more energy than the same objects at rest on the surface of a planet. E = mc^2, therefore we have the equivalent of mass loss, and therefore a reduction in the force of gravity between them compared to what it would be in space. By the way, the forum has not addressed my observation about c. A comment or two would be appreciated.
 
  • #17
Shaw said:
In SR we see time and mass changing together

More precisely, we see time dilation and relativistic mass changing together. But relativistic mass is not the source of gravity in GR; the stress-energy tensor is.

Shaw said:
but 2 test objects at rest in deep space have more energy than the same objects at rest on the surface of a planet.

Energy relative to what? "Energy" is not an absolute quantity; it's relative. And once again, the "energy" you are talking about is not the source of gravity in GR; the stress-energy tensor is. The stress-energy tensor that describes these "test objects" (technically that's not a good term because that term is usually used to describe objects whose own mass is negligible, so they don't act as sources of gravity) is what determines the gravity they produce, and that's different from the "energy" you are talking about.

In short, you are reasoning from a mistaken assumption about what property of the test objects determines the gravity they produce. When you use the correct property, the stress-energy tensor of the objects, you get the answer I and others have already given several times in this thread: the gravity between the two objects is the same when they are in a gravity well and when they are out in empty space far from all other bodies.
 
  • #18
pervect said:
In terms of a local frame of reference, as you descend down the rope, absolutely nothing happens to the force between the plates, but the proper acceleration needed to hold station on the rope increases. So of course the plates separate. How does this show that "gravity is weaker"?

As long as you use local measurements (local clocks, rulers, and scales), the laws of physics (as modeled by General Relativity, at least) don't depend on your location, or the gravitational potential of your location.
First let's use a clock and a ruler to measure acceleration. The clock is affected by time dilation. So our accelerometer is affected by time dilation.

Then let's try to probe acceleration at various altitudes using a fishing rod, a fishing line and a weight, the amount of bending of the fishing rod tells us something about the acceleration at the position of the weight.

The second accelerometer is actually just a force meter. Multiplying the force by the time dilation factor at the position of the weight yields the proper weight of the weight at the position of the weight. Proper acceleration can be calculated from proper weight.

If we put the part that measures the force at the lower end of the fishing line, then the fishing line accelerometer agrees with the clock and ruler accelerometer about acceleration increasing when moving down in uniform gravity field. The two gravitating disks that break apart at some height is same kind of accelerometer as this one. It is affected by time dilation.What if an accelerating spaceship tows a weight with force-meters at both ends of the towing line? Do we agree that the lower force-meter's reading is higher? (towing line is massless, or we subtract its weight)
 
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  • #19
Thanks again for the replies. You know vastly more about GR than I do, so I accept what you've told me. But experiment trumps theory, and as I've pointed out, there is a simple experiment available to put GR's interpretation to the test. My feeling is that you agree. Saying that the experiment is unnecessary because we have the GR solution is not good science. Good science puts theory to the test whenever possible. I don't understand why this experiment has never been done, unless the Cavendish experiment lacks enough sensitivity, but it's my understanding that it's extremely sensitive, so it's likely to be able to do the job. Cheers
 
  • #20
PeterDonis said:
What is a "uniform gravity field"? If by that you mean "proper acceleration does not change with height", then the thought experiment you describe is not a "uniform gravity field"; the Rindler horizon is associated with a congruence of Rindler observers, and their proper acceleration varies with height above the horizon. So the tension in the rope caused by the climber won't be constant.

If, OTOH, you insist on a congruence of observers whose proper acceleration is constant, then this is the Bell congruence, and they are not at rest relative to each other. (More precisely, the expansion scalar of the Bell congruence is nonzero, which means it is not rigid.) So you can't use that congruence to model a static "gravitational field" in your thought experiment. The rope that the mountain climber is climbing down will be stretched further and further as time goes on, even if the climber is not there.

By uniform gravity field I mean the "gravity field" inside an arbitrarily large accelerating spaceship, or the gravity field inside sufficiently small room on a planet. OTOH I use the term correctly. :)

When a climber climbs down a rope in an uniform gravity field, the force of gravity that he feels increases, because he is affected by increasing time dilation. The force pulling the upper end of the rope is the force felt by the climber divided by time dilation factor at climber's position, so it's constant.
 
  • #21
jartsa said:
The clock is affected by time dilation.

Not locally. And pervect was talking about a local measurement. So was the OP.

You are talking about a different scenario, where you are measuring the "redshifted" force at the top of the fishing line, and measuring the "proper" force on the weight at the bottom of the line, and comparing the two. Nobody is disputing that these two measurements will give different results. And nobody is disputing that time dilation will also be measured between the two locations. But none of that has anything to do with the OP's question.

jartsa said:
The two gravitating disks that break apart at some height is same kind of accelerometer as this one.

No, it isn't. Your other accelerometers measure non-gravitational force, which can be present in flat spacetime. The two gravitating disks only have gravitational "force" between them; so spacetime at the very least between them cannot be flat. If you are trying to evaluate whether "gravitational force" measured locally between two objects changes with altitude in a global gravitational field, you can't handwave away that difference.

jartsa said:
By uniform gravity field I mean the "gravity field" inside an arbitrarily large accelerating spaceship, or the gravity field inside sufficiently small room on a planet.

Um, what? If the spaceship is "arbitrarily large", it can't possibly be the same as a "sufficiently small" room on a planet.

jartsa said:
When a climber climbs down a rope in an uniform gravity field, the force of gravity that he feels increases

Yes.

jartsa said:
because he is affected by increasing time dilation.

No. Time dilation is a measure of the gravitational potential; proper acceleration felt is a measure of the gradient of the potential. They're two different things.

jartsa said:
The force pulling the upper end of the rope is the force felt by the climber divided by time dilation factor at climber's position

Yes.

jartsa said:
so it's constant.

For Rindler observers in flat spacetime, yes, it does work out that way. But not for the case of curved spacetime, i.e., a planet. So you can't use your "uniform gravity field" to model what happens on a planet in this respect.
 
  • #22
Shaw said:
Saying that the experiment is unnecessary because we have the GR solution is not good science.

Who said the experiment shouldn't be done? Of course it should be done, when time and resources permit.

But not having done the experiment is not the same as not being pretty sure about the outcome. GR has been tested in many other ways, and it has passed every test. Also, alternative theories of gravity have been constructed which predict different results for this scenario (i.e., that Cavendish experiments will give different results in a gravity well vs. in empty space); but every such theory that has been constructed also makes other predictions which have been falsified. So every indication we have is that, if and when we run the experiment under discussion, the results will match the GR prediction.

That doesn't mean we shouldn't do the experiment; but it also doesn't mean we should go around saying that GR isn't "really proven" until we've done every single experiment that could possibly test it. No scientific theory will ever be able to meet that standard; there will always be other experiments that could in principle be run but haven't yet been run.

Shaw said:
I don't understand why this experiment has never been done

Probably because it's a low priority compared to other experiments that could be run in space. Also possibly because doing such an experiment in free fall might present difficulties.
 
  • #23
PeterDonis said:
Not locally. And pervect was talking about a local measurement. So was the OP.

You are talking about a different scenario, where you are measuring the "redshifted" force at the top of the fishing line, and measuring the "proper" force on the weight at the bottom of the line, and comparing the two. Nobody is disputing that these two measurements will give different results. And nobody is disputing that time dilation will also be measured between the two locations. But none of that has anything to do with the OP's question.
As the OP was interested about force of gravity inside a gravity well, I made a Cavendish apparatus out of two plates, then I made an experimenter to carry the apparatus downstairs, then the experimenter saw the plates to become pulled apart, then I said the plates were pulled apart either because of stronger gravity pulling the plates apart, or because of weaker gravity pulling the plates together.
No, it isn't. Your other accelerometers measure non-gravitational force, which can be present in flat spacetime. The two gravitating disks only have gravitational "force" between them; so spacetime at the very least between them cannot be flat. If you are trying to evaluate whether "gravitational force" measured locally between two objects changes with altitude in a global gravitational field, you can't handwave away that difference.

What happens locally is simple and boring: locally nothing changes.

This might be somewhat interesting:

Let's say that inside an accelerating spaceship there are two winches that are lowering down two magnets. As the magnets descend, the magnetic force between the magnets becomes red shifted, so it becomes easier for a person inside the spaceship to move the winches apart, with the magnets still hanging on them.

In order to gravitational potential to not have any locally observable effects this must also happen:

Let's say inside an accelerating spaceship there are two winches that are lowering down two masses. As the masses descend, the gravitational force between the masses becomes red shifted, so it becomes easier for a person inside the spaceship to move the winches apart, with the masses still hanging on them.And people inside said spaceship can not tell whether they are inside an accelerating spaceship or inside a spaceship sitting on the surface of a large planet.
 
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  • #24
georgir said:
Um, but it won't be the same in both cases. The objects will have different potential energy, and that contributes to their gravitational pull. So the answer is "yes".
Wrong, that would be a violation of local position invariance. See:

http://relativity.livingreviews.org/Articles/lrr-2014-4/articlese2.html#x5-20002

[since it is a gravitational experiment, it would under the rubric of the SEP rather than the EEP, which is described in the next chapter from the one I linked].
 
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  • #25
jartsa said:
I made a Cavendish apparatus out of two plates

Two plates do not a Cavendish apparatus make. You can't measure "the force of gravity" by measuring how far apart two gravitating objects are and whether it changes as you move them about. That doesn't cleanly separate "the force of gravity" from other things. Please look up how a Cavendish apparatus actually works.

jartsa said:
What happens locally is simple and boring: locally nothing changes.

In other words, locally a Cavendish apparatus gives the same result, no matter how deep in a gravity well it is. Yes, I agree. And that's the answer to the question the OP was asking.

But if that's the case, then how can your plates move farther apart? Obviously because, whatever your two plates are measuring, it isn't "local". In other words, your two plates aren't measuring what you think they're measuring.

jartsa said:
As the magnets descend, the magnetic force between the magnets becomes red shifted, so it becomes easier for a person inside the spaceship to move the winches apart, with the magnets still hanging on them.

But this isn't a local experiment, at least, not by the definition of "local" you were using earlier in your post, when you said that locally nothing changes. A person descending with the magnets would find no change at all in the force he had to exert, at the magnets, to move them apart. That's the local experiment, by your definition of "local".

jartsa said:
people inside said spaceship can not tell whether they are inside an accelerating spaceship or inside a spaceship sitting on the surface of a large planet.

As long as the spaceship is small enough compared to the inverse of the acceleration or the size of the planet, yes. But this is a different definition of "local"--it is "local" in the sense of the equivalence principle, i.e., a "local" region is one in which no changes to the magnitude or direction of the "acceleration due to gravity" are observed. In your spaceship example, accurate enough measurements could detect gravitational redshift (for example, a redshift in the force required at the winches to move the magnets apart, because of time dilation) even if no change in proper acceleration was detectable from the top to the bottom of the spaceship (for example, the proper acceleration could be the same, to the accuracy of measurement, at the winches and at the magnets).

This point is often unclear in discussions of "redshifted force" experiments, because they implicitly assume a large enough different in altitude that the proper acceleration itself is very different. But there is a regime in which there is enough separation for gravitational redshift to be detected, even though there is not enough separation for a difference in proper acceleration to be detected. Note that Einstein's thought experiment deriving gravitational redshift using the equivalence principle does not require any difference in acceleration.
 
  • #26
The situation of distinguishing a tall accelerating rocket from a Schwarzschild field even more delicate than Peter implied in his last post. As I'm sure he knows, the most reasonable model of tall rocket with steady thrust is the Rindler metric, which does have decreasing acceleration with altitude. This is necessary to preserve local spatial relationships (technically, make the expansion tensor vanish). Thus, one must have sensitivity to distinguish Rindler from SC metric. For purely one dimensional tidal detection, this would require either extreme precision or a very 'tall' experiment. Easier is if at least two spatial dimensions are used to detect tidal deviation from Rindler (which of course, has no tidal forces, as it is flat spacetime).
 
  • #27
PAllen said:
the most reasonable model of tall rocket with steady thrust is the Rindler metric, which does have decreasing acceleration with altitude.

Yes, this is true. But you can run Einstein's argument for gravitational redshift using a small enough difference in altitude that the acceleration difference is not detectable. This regime is even smaller than the regime in which the difference between the Rindler and Schwarzschild metric is not detectable (since detecting that difference requires, not just detecting a difference in acceleration, but detecting the spatial behavior of the difference precisely enough to distinguish the absence or presence of tidal gravity). In other words, "locality" in the sense of not detecting a gravitational redshift is a more stringent condition than "locality" in the sense of the EP (not detecting tidal gravity).
 
  • #28
Let me add this since it's not personal theory. I have no means of contributing anything directly to relativity theory, it's way beyond my ability, but I do have a set of skills I can apply to the problem of creating a model of spacetime. We have 2 at the moment: the marble rolling on a flexible membrane, and the embedding diagram of the geometry of space around a large mass. The membrane is essentially useless since it relies on gravity to explain gravity so it can't be used in space. It doesn't show curved space in 3 dimensions + the forth I believe is needed. The embedded model can't assign any physical reality to the higher dimensioned space in which the surface is modeled.

I decided I could do better than this and I came up with a 3 dimensional model of the space surround mass, with time as the added dimension. I don't know much about GR, but I'm very good at this sort of thing. The model pointed to 2 predictions. Time would slow down on the surface of a planet and the slowing would equal that for an object moving at the escape velocity. I believe this is correct and it wasn't predicted by GR. The model also predicted a mass reduction to accompany the time change, and if we extrapolated this mass change from a specific example until it approached zero, we would have a velocity very near the speed of light. So the model suggests a testable divergence from GR theory, and that test has never been performed. I agree with PeterDonis that it probably wouldn't work in orbit.
 
  • #29
Shaw said:
Let me add this since it's not personal theory.

It is if you are claiming your model makes predictions different from GR, which you are. (You happen to be at least partly incorrect in this claim, as far as I can see--see below--but that's not relevant to the question of whether it's a personal theory.)

Shaw said:
Time would slow down on the surface of a planet and the slowing would equal that for an object moving at the escape velocity. I believe this is correct and it wasn't predicted by GR.

Why do you think that? GR certainly predicts gravitational time dilation of exactly this magnitude for the case of a planet.

Shaw said:
The model also predicted a mass reduction to accompany the time change

If by "mass reduction" you mean a change in a local measurement, then yes, you are right that GR does not predict this.

If you mean a change "as seen from a distance", then GR does predict that; if you take an object at rest at infinity, and lower it to the surface of a planet, bringing it to rest on that surface, making sure to let any energy released during the process escape to infinity, then the final mass of planet + object, as measured from far away, will be less than the mass of the planet + the original rest mass of the object, as measured at infinity, before you started to lower it. And the difference will be given by the same time dilation factor referred to above.

Shaw said:
So the model suggests a testable divergence from GR theory

If this is true (see above), then it's a personal theory, unless you can give a mainstream reference for it. Which means it's off limits for discussion. So I am closing this thread. If you do have a mainstream reference, PM me.
 

1. What is GR and how does it relate to gravitational force on a planet's surface?

GR, or General Relativity, is a scientific theory proposed by Albert Einstein that describes the relationship between gravity and the curvature of spacetime. It explains how the presence of massive objects, like planets, can affect the curvature of spacetime and thus influence the force of gravity on a planet's surface.

2. Does GR actually reduce the gravitational force on a planet's surface?

Yes, according to the theory of General Relativity, the presence of massive objects, such as planets, can cause a curvature in spacetime which results in a reduction of the gravitational force on a planet's surface compared to what would be predicted by Newton's Law of Universal Gravitation.

3. How does GR differ from Newton's Law of Universal Gravitation?

Newton's Law of Universal Gravitation states that the gravitational force between two objects is directly proportional to the product of their masses and inversely proportional to the square of the distance between them. However, GR takes into account the curvature of spacetime and explains how the presence of massive objects can affect the force of gravity.

4. Are there any real-world examples that support the concept of GR reducing gravitational force on a planet's surface?

Yes, there have been several observations and experiments that support the concept of GR reducing gravitational force on a planet's surface. One example is the phenomenon of gravitational lensing, where the light from distant objects is bent by the gravity of massive objects, confirming the curvature of spacetime predicted by GR.

5. Is GR the only theory that explains the relationship between gravity and the curvature of spacetime?

No, there are other theories such as Modified Newtonian Dynamics (MOND) and Scalar-Tensor-Vector Gravity (STVG) that attempt to explain the relationship between gravity and spacetime curvature. However, GR is the most widely accepted and experimentally supported theory in this regard.

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