# General relativity and tidal forces

## Main Question or Discussion Point

Tides on earth are described with newton's theory of gravitation. Relativistic effects on tides theoretically become measurable on very strong gravitational fields, possibly becoming twice as strong as tides predicted by newtonian gravity: http://adsabs.harvard.edu/abs/1983ApJ...264..620N

Tides are presumably outcomes of gravitational forces. Einstein ditched forces and the concept of inertia in GR (http://archive.org/stream/TheBornEinsteinLetters/Born-TheBornEinsteinLetters_djvu.txt). So how is GR used to calculate tidal forces? If different parts of the body travel different geodesics, this would cause the body to tear apart over time. How can tides be described with the geometry of space-time?

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Nugatory
Mentor
So how is GR used to calculate tidal forces? If different parts of the body travel different geodesics, this would cause the body to tear apart over time. How can tides be described with the geometry of space-time?
If the forces holding the body together are strong enough, they will accelerate the different parts of the body off their geodesics and onto non-geodesic worldlines that stay close enough that the body doesn't tear apart. The center of mass of the object follows a geodesic and the other parts of the body experience fictitious forces that tend to pull the body apart and are resisted by whatever forces hold the body together.

These fictitious forces are tides.

pervect
Staff Emeritus
Tides on earth are described with newton's theory of gravitation. Relativistic effects on tides theoretically become measurable on very strong gravitational fields, possibly becoming twice as strong as tides predicted by newtonian gravity: http://adsabs.harvard.edu/abs/1983ApJ...264..620N

Tides are presumably outcomes of gravitational forces. Einstein ditched forces and the concept of inertia in GR (http://archive.org/stream/TheBornEinsteinLetters/Born-TheBornEinsteinLetters_djvu.txt). So how is GR used to calculate tidal forces? If different parts of the body travel different geodesics, this would cause the body to tear apart over time. How can tides be described with the geometry of space-time?
Tidal forces, when suitably defined, can be identified as being components of the Riemann curvature tensor.

Under most circumstances, taking the tidal force as one would measure it via Newtonian means ( a couple of accelerometers separated by a rigid rod) is an excellent approximation to (one of the) geometric definitions, which is related to the apparent relative acceleration of nearby geodesics which are initially parallel.

In fact, you write earlier (this is a very good insight)

If different parts of the body travel different geodesics, this would cause the body to tear apart over time.
The point is that when you measure the forces needed to hold a rigid body together, to keep it rigid, you are indirectly measuring "how fast" the geodesics would expand (accelerate away from each other) if said restoring forces did not exist.

MTW's textbook "Gravitation", and a number of other textbooks, take this approach, though MTW is perhaps the textbook which invites the reader to take it most seriously.

The full Riemann curvature can, given a local description of time (a frame of reference, for instance, more formally a timelike congruence of worldlines) be decomposed by the Bel Decomposition http://en.wikipedia.org/w/index.php?title=Bel_decomposition&oldid=512613685 into three parts. One part, called the electrogravitic tensor, describes static gravity, and givenby the above "tidal forces", so the Newtonian tidal tensor can be pretty much directly be linked to the electrogravitic part of the Riemann tensor.

Another part, called the magnetogravitic tensor, described frame-dragging effects (which affect moving bodies, but don't directly affect static bodies). A third part, the topogravitic tensor, describes spatial curvature.

The Bel decomposition, unfortunately, is usually given short shrift in textbooks, so it may be hard to find a formal treatment I was introduced to it rather informally here on PF, for instance.

All right, so I think I understand the basis of how GR creates tides, even though I have a minor issue with fictitious forces counteracted by real forces in this particular case, but that's a subject for another thread, I don't want to get into this here.
My problem with this analysis is that different parts of the body are not only trying to travel different geodesics, but also, in order to stay rigid, the outer parts of the rotating orbiter must have a faster tangential component than the inner parts. This is a bigger problem when you consider a body in tidal lock, such as the moon. Different geodesics would tend to rip the body apart radially, but different velocities would tend to shear te body in the line of orbit. In all gravitational theories, the tangential component of the velocity can't be caused by the gravitational field and is a constant. Newton called it the body's innate velocity.

Think of it this way: a body is at a constant linear velocity, so all parts of the body travel at the same linear speed. Then it is captured by a gravitational field. It starts to orbit that planet and the linear velocity is not changed, but the body is accelerated into a curved motion (or continues to have a constant velocity in curved spacetime). The tangential component must still be the same for all parts of the body since gravity imparts no (fictitious) forces tangentially. This would tend to cause shearing, especially in a body in tidal lock. If it doesn't start to shear, presumably the tangential velocities are different on different parts of the body, with the far side faster then the near side (this would be true for all bodies, not only the ones in tidal lock), but how can that be? What forces act on the body to change the tangential (innate) velocities if gravity has no way to do so neither with Newton nor with GR? Are tides capable of changing tangential velocities in either GR or Newton's theory?

pervect
Staff Emeritus
While "centrifugal" forces, i.e. forces due to rotation, do contribute to the strain on a rigid bar, they do not contribute to the Riemann curvature tensor, which is ultimately based on how fast geodesics separate (or converge). The "force-on-a-bar" idea is very useful, but it can only be used if/when the bar isn't rotating.

So in your orbiter example, either you'd need to imagine that your spacecraft was not rotating (in which case in 1/2 an orbit the outer side would be the inner side, assuming no frame dragging effects), or if your space-craft is tide-locked, you'd have to manually subtract the forces due to its absolute rotation (once per orbit, again assuming no frame dragging) from the measured strain on the bar to get the tensor components.

The Electrogravitic component of the Riemann tensor must be traceless. The centrifugal forces on a rotating sphere are not traceless, this is one way you can tell if a system is rotating.

Accurate measurements of the gravity tensor, typically using rather exotic means such as superconductors and SQUID's for the detectors, are an expensive, but semi-routine, part of modern prospecting. Some interesting references are http://www.physics.umd.edu, http://www.bellgeo.com/tech/technology_theory_of_FTG.html [Broken], and http://www.dtic.mil/cgi-bin/GetTRDoc?AD=ADA496707/GRE/NASA_SGG.pdf [Broken]. These papers describe some of the modern techniques that are actually used to measure the gravity tensor. The last has some discussion of the physics as well, though it's oriented mostly towards Newtonian gravity.

The Wiki article is also mildly helpful, http://en.wikipedia.org/w/index.php?title=Gravity_gradiometry&oldid=508813691, giving a list of some of the basic systems that have been implemented.

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While "centrifugal" forces, i.e. forces due to rotation, do contribute to the strain on a rigid bar, they do not contribute to the Riemann curvature tensor, which is ultimately based on how fast geodesics separate (or converge). The "force-on-a-bar" idea is very useful, but it can only be used if/when the bar isn't rotating.
I'm not sure i follow. Forces due to rotation cause strain, but can only be used if the bar is not rotating??????

So in your orbiter example, either you'd need to imagine that your spacecraft was not rotating (in which case in 1/2 an orbit the outer side would be the inner side, assuming no frame dragging effects), or if your space-craft is tide-locked, you'd have to manually subtract the forces due to its absolute rotation (once per orbit, again assuming no frame dragging) from the measured strain on the bar to get the tensor components.
If the orbiter does not rotate on its axis, as in your first example, everything is fine, because there's no variation in tangential speeds. But if the body is in tidal lock, then how does the tangential velocities adjust to maintain the body in position? Or, if they don't adjust, how come there's no shearing?

russ_watters
Mentor
... different velocities would tend to shear te body in the line of orbit.
Why do you say that? Sounds like an issue with geometry to me, like you think that different velocities mean different parts of the object are moving apart. What you're missing is that the object is rotating. Spin a pencil on your desk and you'll see that different parts travel at different speeds, but there is no shear.
But if the body is in tidal lock, then how does the tangential velocities adjust to maintain the body in position? Or, if they don't adjust, how come there's no shearing?
A torque is produced if a body's tidal bulge is not aligned with the source of the bulge: http://en.wikipedia.org/wiki/Tidal_locking

Why do you say that? Sounds like an issue with geometry to me, like you think that different velocities mean different parts of the object are moving apart. What you're missing is that the object is rotating. Spin a pencil on your desk and you'll see that different parts travel at different speeds, but there is no shear. A torque is produced if a body's tidal bulge is not aligned with the source of the bulge: http://en.wikipedia.org/wiki/Tidal_locking
Sorry, I meant to say that equal tangential velocities would tend to cause shearing, not different velocities. I'm making a diagram to clarify.

Ok, I'm having a hard time putting the problem into words so I drew a diagram that may help to clarify the whole thing:
http://www.pictureshoster.com/files/aix43ezq7zp99daihgzu.jpg
http://www.pictureshoster.com/files/aix43ezq7zp99daihgzu.jpg

If different parts of the body have different velocities, there's no shearing. But if all parts of the body have the same linear velocity, then a body in tidal lock should exhibit shearing.

If there's no shearing, it follows that different parts of the body have different tangential components. Suppose that a body is traveling in a straight line at a constant velocity. It passes near a second body and starts to orbit it. If nothing else happens, the body wouldn't start to rotate on it's own axis and in "1/2 an orbit the outer side would be the inner side" just like pervect said. For a body in tidal lock, something seems to affect linear velocities on the near and far side so that the far side orbits faster than the near side.

My question is what causes the changes in these tangential velocities. Or alternatively, why is there no shearing. Since gravity has no tangential component neither in Newton nor in GR, I'm lost.

At first I thought maybe it had something to do with the rigidity of the body and tidal forces. I thought that gravity would accelerate the near and far sides differently and force the body in tidal lock, accelerating the far side more than the near side, but this turned out to be a dead end.

I think the make up of the problem is clearer now with my diagram, and I believe my logic is consistent. A body in this situation must either shear or achieve different tangential velocities on the near and on the far sides. If this is the case, what is the cause of these changes?

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D H
Staff Emeritus
I think the make up of the problem is clearer now with my diagram, and I believe my logic is consistent.

You are looking in the wrong directions. First look at a spec of mass on the orbiting body at the point furthest from the central mass. The velocity of that spec of mass is a function of the radius of the orbiting body and the velocity of the orbiting body's center of mass. Now imagine what would happen if that orbiting body wasn't there; all you have is the spec of mass as an orbiting body. That free particle will follow a different path than would our spec of mass. In particular, it would move outward. The tidal force at this point is radially outward away from the central mass, not tangential. Similarly, the tidal force on the point closest to the central mass is radially inward, toward the central mass. In both cases, the tidal force is away from the center of mass of the orbiting body. There is also a lesser effect (about half as much) for a particle at the leading and trailing points on the orbiting body. A free particle at those leading and trailing points would follow different paths than will a particle fixed to the orbiting body, but now the tidal force is directed toward the center of mass of the orbiting body. The end result is that the tidal forces act to pull the object apart radially, squeeze it together tangentially.

Newtonian mechanics and general relativity agree on the above description so long as the central mass isn't particular massive or the distance to the central mass is sufficiently large. The reason for this agreement is that space-time is locally flat. "Locally" is a fairly large volume in these weak field circumstances, at least as far as physicists are concerned. (Mathematicians will disagree; local means infinitesimally small to them.) Make the central body massive enough or close enough and those weak field approximations become invalid. You'll start seeing effects that result from the curvature of space-time. Newtonian mechanics and relativity diverge at this point. Newtonian mechanics does not properly describe the extreme spaghettification that results from close proximity to extremely massive objects.

pervect
Staff Emeritus
If you connect the "red x"s on the same point on a non-rotating body, you'll get an elliptical orbit more like the one I'll attach, the picture you drew isn't right.

If you go through the math (using just Newtonian theory), you'll get the results DW quoted.

In particular, if the radial Newtonian force is -GM/r^2, differentiating this with respect to r gives the well-known result for the radial tidal force 2GM/r^3. See also the wiki article, http://en.wikipedia.org/w/index.php?title=Tidal_tensor&oldid=332450104.

It takes more work to go through the math to get the compressive tidal forces, the results dW quotes are correct however.

The results for GR are formally similar to the Newtonian results in a local frame-field, if you replace the radial distance "r" with the radial coordinate "r" for the Schwarzschild metric. Local frame fields seem to confuse more readers than they should, the math to compute them is somewhat involved, but the end result is just the forces/fields/tensors that a local observer would measure with local clocks and local rulers.

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First look at a spec of mass on the orbiting body at the point furthest from the central mass. The velocity of that spec of mass is a function of the radius of the orbiting body and the velocity of the orbiting body's center of mass. Now imagine what would happen if that orbiting body wasn't there; all you have is the spec of mass as an orbiting body. That free particle will follow a different path than would our spec of mass. In particular, it would move outward. The tidal force at this point is radially outward away from the central mass, not tangential. Similarly, the tidal force on the point closest to the central mass is radially inward, toward the central mass. In both cases, the tidal force is away from the center of mass of the orbiting body.
I completely agree. But this does not address the problem. In the diagram, I hid the effects of tides, I want to focus on the tangential components of the velocities. I am aware that the specs would move apart, I actually said that explicitly in my first post.

What keeps the near and far side from moving apart, which was answered in the beginning of the post, are the forces holding the body together, so it is clear that tidal forces tend to elongate the body radially, and it is clear that neither tides nor gravity have mechanisms to act tangentially on the near and far sides to change these velocities.

Please be patient since my question has not been answered. Leave tidal forces out for a moment and consider this:

- A body Y moves in a straight line at a constant velocity V.
- All parts of the body have the same linear velocity V.
- This body starts to orbit a central mass M.
- M imparts a centripetal acceleration due to gravity on Y.
- Y feels no tangential forces from M, and no drag.
- Y achieves tidal lock: the far side has a faster tangential velocity than the inner side.

Now, if Y did not achieve tidal lock, and no forces other then gravity from M act on it, we may assume that there is no change in the tangential velocities and there would be no fixed near and far sides, the tides would travel, the body would appear to rotate as seen from M, the body would not be rotating in it's own axis locally (relative to it's own orbit) and everything is fine.

But if Y orbits in tidal lock, the far side orbits faster than the near side, and we must assume a change in the tangential velocities of each sides, namely, a positive acceleration on the far side and a negative one on the near side.

Gravity can't cause these tangential accelerations, so there's no way M causes it. The body Y also cannot impart forces on itself, so again, it cannot be the cause of these changes.

My question is: what causes the changes in the tangential velocities of the near and far sides?

Nugatory
Mentor
The body Y also cannot impart forces on itself, so again, it cannot be the cause of these changes.
The body Y cannot apply forces to itself, but one part of the body can apply forces to another part. Replace the body with a cloud of dust, such that each dust particle is connected to its neighbors with a spring. Now if two of the particles are on diverging geodesics, the spring between them will be stretched, applying a force to both particles that will accelerate them off their inertial path and onto other geodesics. Obviously this process can change the shape of the body/cloud; but it can also change the velocity of one part of the cloud relative to another, as in tidal locking.

Nugatory
Mentor
Gravity can't cause these tangential accelerations
Even though it acts only in a radial direction, gravity can produce tangential accelerations. Consider, for example, dropping a horizontally oriented bar towards the surface of the earth. Each end of the bar will experience a gravitational force pointing towards the center of the earth. These two vectors are not parallel; if I extend them far enough they will intersect at the center of the earth, so they are ever so slightly converging. Thus, both vectors have a small tangential component that is pushing the ends of the rod towards the middle and is resisted by the rigidity of the rod.

It's true that these forces are balanced so they cannot affect the center-of-mass movement of the rod - but that's true of tidal locking of a rotating body as well.

That's a good point, but isn't that one of the reasons the body should resist changes on tangential velocities on the near and far sides? For example, if I try to push only the far side, these internal bonds (rigidity) would tend to transfer forces to the near side (and everywhere else). But the force is only transfered in this case, isn't it? That means that there must be an external force acting on the tangent in this case, and this force would be resisted by rigidity.

You mention tangential accelerations caused by gravity in a rigid rod falling horizontally towards the central mass. But in this case, the body is not in orbit, and if it was (even if slowly falling), the forces would be on the trailing and leading sides, wouldn't they? And this would only help the radial bulging anyway. These tangential components are not capable of altering tangential velocities on the near and far sides. A good analogy would be to hold the same rod vertically wrt earth and throw it straight towards the horizon (ignore drag). Would the far side of the rod start to speed up relative to the near side? Of course not. But that would be a rod in tidal lock.

Since there's no tangential forces in gravity, I don't see where these changes in tangential velocities come from. The stretching you mentioned with the springs, caused by gravity, is only radial, it would cause radial stretching (tidal bulges). Exactly how can this radial force change the tangential velocities of the near and far sides?

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It might be constructive to look at some actual figures. For a test particle in the Schwarzschild vacuum the proper acceleration felt by an observer in a circular path u is

$$\frac{du}{d\tau} = \frac{m\,{\cos\left( \theta\right) }^{2}}{{r}^{2}-2\,m\,r}\ dr -\frac{m\,\cos\left( \theta\right) \,\sin\left( \theta\right) }{r-3\,m}\ d\theta$$
If the particle is entirely in the equatorial plane (EP, θ = π/2) both components are zero, and the orbit is a geodesic. Considering a small sphere in orbit, with its centre following the geodesic we can make some deductions about the forces required to keep the whole body together.

The acceleration in the θ-direction ( the one pointing up and down from the equatorial plane) will change sign between the two halves so it always acts towards the EP causing compressive stress. In the radial direction, leaving the EP in either direction will cause an increase in the acceleration in the +ve r-direction. I don't know what deformation this causes. Both components get smaller as the radius increases so it looks like there is also some stretching in the r and θ-directions.

The acceleration above is calculated from the Schwarzschild circular orbit geodesic in the coordinate basis with 4-velocity
$$u=\frac{\sqrt{r}\,\sqrt{m\,{\sin\left( \theta\right) }^{2}+r-3\,m}}{\sqrt{r-3\,m}\,\sqrt{r-2\,m}}\ \partial_t -\frac{\sqrt{m}}{r\,\sqrt{r-3\,m}}\ \partial_\phi$$
This is only a geodesic if sin(θ) = 1. So any circular path off the EP must apply forces to offset the accelerations engendered.

zonde
Gold Member
But if Y orbits in tidal lock, the far side orbits faster than the near side, and we must assume a change in the tangential velocities of each sides, namely, a positive acceleration on the far side and a negative one on the near side.

Gravity can't cause these tangential accelerations, so there's no way M causes it. The body Y also cannot impart forces on itself, so again, it cannot be the cause of these changes.

My question is: what causes the changes in the tangential velocities of the near and far sides?
Let's say that this body in tidal lock does not have perfect spherical symmetry. Then as it rotates it's gravity affects large mass M differently. Now let's say that body M is not entirely rigid so that there are slightly different responses to small body in different rotation angle positions.
Another possibility. Body in orbit itself is not entirely rigid and then radial stretch elongates the body in different directions as it rotates. If this response to stretch in different directions is different then shouldn't it be possible to dump angular momentum using that radial force?

Nugatory
Mentor
A good analogy would be to hold the same rod vertically wrt earth and throw it straight towards the horizon (ignore drag). Would the far side of the rod start to speed up relative to the near side? Of course not.
When you're holding the rod vertically, it's exactly lined up with the radial gravitational force; both ends of the rod and the center of the earth lie in the same line, and the gravitational force acts along that line. But when you throw the rod it moves off that vertical line. Now the forces acting on the two ends are no longer exactly parallel (extend the vectors and they meet at the center of the earth, therefore are very slightly converging). Furthermore, the forces have very slightly different magnitudes, because the distance to the center of the earth is different for the two ends.

So we have forces of different magnitude acting in different directions on the two ends of the rod. Why shouldn't one end speed up relative to the other?

Mentz114, Thanks for this. Correct me if i'm wrong, i take this to mean that anything above the equatorial plane suffers an accel towards the equatorial plane. That would be the flattening at the poles of tidal theory. As you also pointed out, there should also be stretching in the equatorial plane (i assume only on the near and far sides) which would be the tidal bulges. Still, i see no component that would cause different tangential forces on the near and far sides that could adjust velocities to cause a body to achieve tidal lock, is this correct?

Let's say that this body in tidal lock does not have perfect spherical symmetry. Then as it rotates it's gravity affects large mass M differently. Now let's say that body M is not entirely rigid so that there are slightly different responses to small body in different rotation angle positions.
Another possibility. Body in orbit itself is not entirely rigid and then radial stretch elongates the body in different directions as it rotates. If this response to stretch in different directions is different then shouldn't it be possible to dump angular momentum using that radial force?
I have considered this, and i believe that would tend to cause shearing. If the tangential velocities on the near and far sides remain unchenged, these forces that you mention would work against this stretching, but not overcome it. If a body has almost no rigidity, it could not hold itself together and it would shear (near side ahead of the far side), stretch radially and tear apart.

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When you're holding the rod vertically, it's exactly lined up with the radial gravitational force; both ends of the rod and the center of the earth lie in the same line, and the gravitational force acts along that line. But when you throw the rod it moves off that vertical line. Now the forces acting on the two ends are no longer exactly parallel (extend the vectors and they meet at the center of the earth, therefore are very slightly converging). Furthermore, the forces have very slightly different magnitudes, because the distance to the center of the earth is different for the two ends.

So we have forces of different magnitude acting in different directions on the two ends of the rod. Why shouldn't one end speed up relative to the other?
This is a more thorough analysis. But wouldn't this cause the near side to accelerate more than the far side? Garvity is stronger nearer the central mass than farther away. The rod would actually start to rotate slightly backwards, the near side being faster than the far side, the far side getting behind. Also, these forces still have no tangential component, they are only radial. I don't see these forces accelerating the far side more than the near side in any way, especially tangentially. Agreed?

Nugatory
Mentor
But wouldn't this cause the near side to accelerate more than the far side? Garvity is stronger nearer the central mass than farther away. The rod would actually start to rotate slightly backwards, the near side being faster than the far side, the far side getting behind.
I threw the rod, so it's moving in some direction. The tiny horizontal components of the gravitational forces acting on the ends of the rod are acting against the direction of movement so are slowing the ends. The inner end, subject to the stronger horizontal force, is slowed more so ends up behind.

But that's a detail.... The more important point is

Also, these forces still have no tangential component, they are only radial. I don't see these forces accelerating the far side more than the near side in any way, especially tangentially. Agreed?
No. If one end is getting behind the other, then the speed of one or both has necessarily changed since the moment they were thrown. That's acceleration, by definition.

Also important is that you have to be very careful with the word "radial" and "tangential" when you're dealing with non-point objects, because the directions identified by those words change from point to point, and therefore from one place to another on a non-point object like a planet or a rod or a cloud of dust particles connected by springs. A purely radial force at the center of gravity of an object has a tangential component at another part of the object.

At least in classical mechanics, the net force on the body must sum to being a radial force through the center of mass, but other parts of the body can feel forces that try to move them relative to that center of mass. These can rotate the object (thrown vertical rod), compress it horizontally (stationary horizontal rod), as well as stretch it vertically or change its shape.

I threw the rod, so it's moving in some direction. The tiny horizontal components of the gravitational forces acting on the ends of the rod are acting against the direction of movement so are slowing the ends. The inner end, subject to the stronger horizontal force, is slowed more so ends up behind.
I see what you mean, it is tricky indeed. Let's look at it with GR: the far side follows a larger geodesic than the near side of the rod. There are no forces or accelerations. The tangential velocity of the rod is the same all over, so it would travel the outer geodesic at the same speed as the inner geodesic, and since the inner geodesic is smaller, the near side gets ahead of the far side. Just like two race cars with the same velocity in their speedometers, making a turn in an inner and an outer track lane – the car in the outer lane has to travel a longer distance, and ends up behind the car in the inner lane.

Considering Newton, it's a bit trickier (who would imagine!): in visualizing the rod oriented vertically to the central mass, traveling linearly (trying to describe no curves - curves would be the result of gravity alone) with a constant linear velocity, I see your point. I can also visualize it differently, though: the inner side has a greater pull than the far side, and drags the far side down with it (more than gravity alone would if acted on a particle at the same distance as the far side). That would cause the far side to experience basically the same acceleration down as the near side for a rigid rod. The vector addition of the tangential velocity and the centripetal acceleration would result in vectors with the direction and magnitude for both sides, and since the far side has a longer distance to travel, we end up with the same situation as the analysis above.

Also important is that you have to be very careful with the word "radial" and "tangential" when you're dealing with non-point objects, because the directions identified by those words change from point to point, and therefore from one place to another on a non-point object like a planet or a rod or a cloud of dust particles connected by springs. A purely radial force at the center of gravity of an object has a tangential component at another part of the object.
I agree we have to be very careful. In the diagram I posted, you can see that a change the directions of the tangents precisely the way you propose. But it's very tricky without diagrams, I admit.
But I disagree with your analysis of the tangential components... The tangential component you specified is only apparent, meaning, it is relative to other parts of the body, not relative to the central mass. The centripetal acceleration have no tangential components of its own. You have to consider that all resulting motions are vector additions of a centripetal acceleration and a linear tangential velocity, nothing else. If one side has a different tangential velocity and describes a different curve than the other, it must be due to this vector addition, and the only tangential component is the body's innate linear velocity. Remember that Einstein also claimed that gravity can't work on the tangents in GR.

At least in classical mechanics, the net force on the body must sum to being a radial force through the center of mass, but other parts of the body can feel forces that try to move them relative to that center of mass. These can rotate the object (thrown vertical rod), compress it horizontally (stationary horizontal rod), as well as stretch it vertically or change its shape.
Agreed. Now, none of that can make the far side orbit faster than the near side so a body achieves tidal lock, can it?

The best way to visualize all this, I think, is to consider 2 small bodies with the same linear velocity, one starting to orbit closer to the central mass than the other. The one closer to the central mass would complete a revolution before the one farther away. These forces should be equivalent to the forces experienced by different parts of a large orbiting body, the only difference is the reaction to these forces due to rigidity. But these reactions can't move the far side faster than the near side on a body in tidal lock, so I still can't figure out what creates the tidal lock.

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One more thing: both the centripetal acceleration and the forces due to rigidity take time to travel from the near side to the far side in Newton's theory, so the far side would lag behind the near side. In GR, the same is true for the forces due to rigidity.

Nugatory
Mentor
The best way to visualize all this, I think, is to consider 2 small bodies with the same linear velocity, one starting to orbit closer to the central mass than the other. The one closer to the central mass would complete a revolution before the one farther away.
That's not possible, at least not if the orbits are circular and I'm understanding "linear velocity" correctly as "the speed of the object, which is also its velocity in its tangential direction at a particular moment". The speed needed to keep an object in a circular orbit in an inverse-square field like gravity is a function of the radius of the orbit (compare the acceleration $\frac{v^2}{r}$ with the force producing that acceleration $\frac{K}{r^2}$ to see this) so they can't both have the same linear velocity.

The best way to visualize all this, I think, is to consider 2 small bodies with the same linear velocity, one starting to orbit closer to the central mass than the other....These forces should be equivalent to the forces experienced by different parts of a large orbiting body, the only difference is the reaction to these forces due to rigidity. But these reactions can't move the far side faster than the near side on a body in tidal lock, so I still can't figure out what creates the tidal lock.
OK, back to tidal lock....

Consider your two bodies orbiting at slightly different radii and joined by a spring. The tidal lock problem comes down to explaining how this system ends up oriented vertically so that both objects complete an orbit in the same time - which implies that the ensemble of two objects and a spring is rotating about its own center of mass once per orbital period.

Assume for definiteness that both the orbit and the positive sense of rotation of the body-spring system is counter-clockwise. If the body-spring system is rotating too slowly, less than one rotation per orbit (this also covers the case of zero rotation and clockwise rotation), then the outer object will lag behind the inner object. Conversely if the body-spring system is rotating at more than one rotation per orbit, then the outer object will move ahead of the inner object.

Now look at the torque around the center of mass of the body-spring system when the outer object is leading and when it is lagging; we know that there will be some torque because both the direction and the strength of the forces on the two bodies is different. When the outer body is leading, that torque acts against the rotation, and when the inner body is leading that torque tends to act with the rotation. That is, when the body-spring system is rotating around its center of mass at less than one rotation per orbit, the torque from the different forces on the two ends acts to increase the rotation rate; and when the body-spring system is rotating at more than that rate, the torque acts to reduce it.

Thus, we expect the system to stabilize at exactly one revolution per orbit, and that's tidal lock.
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There are some complexities that I've glossed over. Among them:
- As long as we aren't tidally locked, there will be some points in the orbit when the two objects are at the same distance from the center and the spring is compressed, and other points where they are at different distances and the spring is stretched. Energy is dissipated in the stretching and relaxing of the spring as the body-spring system orbits (or in a real stone-and-rock satellite, as the tidal bulge moves through its crust with the rotation of the satellite) until the stable tidal lock situation is reached. Thus, tidal locking may result in some loss of orbital kinetic energy, and we may end up with a lower orbit post-lock than pre-lock.
- Angular momentum has to be conserved. When locking changes the angular momentum of the body-spring system about its center of mass, something else has to change as well. This will either be the orbital angular momentum of the body-spring system (see above for how it can change) or the rotation of the parent body (so far we've assumed the parent body to be a fixed point source, but of course it's not, so these tidal effects are at work on it as well).

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