Special Relativity & Non-Instantaneous Force Equations

In summary, the gravitational force is described by the equation F = Gm1m2/r^2 in classical mechanics, but this equation is not compatible with special relativity. In general relativity, gravity is not a force but is instead described by the curvature of spacetime. Attempts to modify the Newtonian force equation to make it compatible with special relativity have been unsuccessful, leading to the development of general relativity. The field concept, introduced by Faraday, is key to understanding the fundamental difference between Newtonian gravity and electromagnetism, which is already consistent with relativity.
  • #1
Fascheue
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In classical mechanics, the gravitational force is described by the equation:

F = Gm1m2/r^2

What would this equation - or other similar equations - look like in special relativity? This equation cannot be correct because it implies that the force acts instantaneously.
 
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Fascheue said:
What would this equation - or other similar equations - look like in special relativity?

You can't describe gravity using special relativity. You have to use general relativity. In GR, gravity is not a force, it's spacetime curvature, so there is no "force equation" for gravity except in particular solutions where a Newtonian approximation can be used.
 
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  • #3
Fascheue said:
This equation cannot be correct because it implies that the force acts instantaneously.

You are correct, and the obvious way to try to fix the Newtonian force equation for gravity is to add retardation, i.e., to make the gravitational force on body B due to body A depend, not on where body A is "now", but where body A was on body B's past light cone. Unfortunately, this theory makes predictions that are grossly contrary to observation (for example, there would be no stable orbits in such a theory), and attempting to fix it up by adding more corrections eventually leads you to General Relativity.
 
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As you note, Newtonian gravity is incompatible with special relativity. I believe several attempts were made to construct a Lorentz covariant version of Newtonian gravity after special relativity was developed, but they all made completely wrong predictions. For a relativistic theory of gravity you need General Relativity, but in this theory gravity is not a force and there is no equivalent to Newton's formula. Instead you derive the effects of gravity from the geometry of curved spacetime.
 
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  • #5
PeterDonis said:
You are correct, and the obvious way to try to fix the Newtonian force equation for gravity is to add retardation, i.e., to make the gravitational force on body B due to body A depend, not on where body A is "now", but where body A was on body B's past light cone. Unfortunately, this theory makes predictions that are grossly contrary to observation (for example, there would be no stable orbits in such a theory), and attempting to fix it up by adding more corrections eventually leads you to General Relativity.
I see. Is this only true for the gravitational force?

Does the light cone modification work for the very similar Coulomb’s law equation?
 
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  • #6
Fascheue said:
I see. Is this only true for the gravitational force?

Does the light cone modification work for the very similar Coulomb’s law equation?
The fundamental difference between Newtonian gravity and electromagnetism is that electromagnetism includes electric effects (similar to Newtonian gravity in the static case, as you say) and magnetic effects (for which there is no analog in Newtonian gravity). In short, if you move an electric charge you get a magnetic field, and that turns out to produce mathematics that is consistent with relativity. If you move a mass, there is no such thing as a Newtonian "gravitational magnetic field", and the apparent analogy with electromagnetism breaks down.

You can, in certain weak field limits, derive something called a gravitomagnetic field from general relativity. It's an exact analogy to electromagnetism and is governed by an exact analog of Maxwell's equations. It's only an approximation to relativity, though.
 
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  • #7
Fascheue said:
Is this only true for the gravitational force?

Is what only true?

The gravitational force is the only force (in the pre-GR sense of "force") that obeys the equivalence principle, so it is the only force that has a straightforward interpretation in terms of spacetime geometry, as GR does it.

Fascheue said:
Does the light cone modification work for the very similar Coulomb’s law equation?

Yes; what you get when you do that is Maxwell's Equations, which are the classical field equations for electromagnetism. In other words, classical electromagnetism, as embodied in Maxwell's Equations, is already "relativistic". This is usually described as Maxwell's Equations already being Lorentz invariant, whereas Newton's laws and Newtonian gravity are not; they are Galilean invariant.
 
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I think to answer this question concerning gravitation one should argue not with the final result that gravitational interaction (and inertia) can be reinterpreted as spacetime geometry a la general relativity, though this is of course a correct an important interpretation but conceptually the question is answered by the introduction of the field concept.

Interestingly already Newton had his quibbles with his action-at-a-distance law for gravity, which however is the only way to make the interaction between distant bodies compatible with the third law (actio=reactio). Already Newton was a bit quibbled by this action at a distance but since it worked so well with the celestial mechanics he just abandoned his quibbles by his famous statement "hypotheses non fingo" ("I don't make hypotheses").

The resolution of this quibble was the idea of the field concept, which is due to Faraday in connection with the electromagnetic interaction. Though he couldn't formulate this most important fundamental concept since Newton's mechanics in a mathematical way, he had a very good intuition. Then of course Maxwell with his mathematical realization of Faraday's field idea got it right as a relativistic local field theory though of course he had no idea about relativity.

The important feature of the field-theoretical view in connection with your question of consistency with relativistic causality (i.e., with the existence of a limiting speed of causal signal propagation) is that it is a local theory, i.e., the action of the electromagnetic force on a charged point particle is due to the presence of the electromagnetic field at the location of this point charge, and the electromagnetic field is taking part in the dynamics of a closed system as does the charged particles, i.e., the field is a fundamental dynamical degree of freedom, and Maxwell's equations tell how the field is created due to the presence of charges and currents and Lorentz's force tells the charges how to move (though this is a bit too optimistic a view concerning point particles, because there are serious problems with classical point particles in any relativistic field theory, and the solution of this is to describe the matter in terms of (relativistic) continuum mechanics in the classical realm or in terms of a relativistic QFT when quantum effects become important), and thus through the "mediation of the forces" through a dynamical field everything is consistent with the "fundamental speed limit".

Now the gravitational interaction is different from all other interactions in the sense that the socalled equivalence principle holds. This means that for a sufficiently small region in space, where the gravitational field acting on a point particle (caused by other matter creating this field) can be considered as homogeneous you can always find a reference frame where there is no gravitational force (you can realize it by a sufficiently small box in free fall, like the International Space Station, where you have only very little gravity inside, because it's freely falling). This is the socalled "weak equivalence principle". You can now also impose the "strong equivalence principle", i.e., you extend the possibility to find, in a sufficiently small region (more precisely spacetime region) always a frame of reference, where all the physical laws hold as if there's no gravitational field. If you think this to the end you end up with the conclusion that Lorentz invariance, which is a global symmetry in special relativity must be made a local symmetry. This opens all the mathematical machinery to make all kinds of models for matter and in addition you get a (pseudo-)metric and what's called a connection on a differentiable manifold. Further it turns out that in the macrocopic realm, where you can describe matter in terms of continuum mechanics and with electromagnetism as the only relevant interaction besides gravity, that the connection is torsion free and thus you end up with Einstein's general relativity, which is completely equivalent to say that gravity can be reinterpreted as a curved spacetime geometry, and also it turns out that everything is compatible with the "relativistic speed limit", i.e., what appears as a gravitational force acting on a freely falling test body in Newtonian mechanics is within GR just a force-free motion in the curved spacetime, and again the trajectory of the body is completely determined by local laws, namely that the trajectory of the freely falling body must be a geodesic of spacetime. How the spacetime geometry looks like in detail is described by Einstein's field equations, which tell "spacetime how to curve" (Wheeler), and thus the spacetime structure (described by the pseudometric of the Lorentz space) becomes a dynamical entity, and causal changes propagate with the same limiting as in special relativity which, to the best of our knowledge, is just the speed of light, because the electromagnetic field is with high accuracy massless. Quantitatively the upper bound of the related photon mass is ##m_{\gamma}<10^{-18} \text{eV}##.
 
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1. What is special relativity?

Special relativity is a theory developed by Albert Einstein that explains the relationship between space and time in the presence of gravity. It is based on the idea that the laws of physics are the same for all observers, regardless of their relative motion.

2. How does special relativity differ from classical mechanics?

Special relativity differs from classical mechanics in that it takes into account the effects of high speeds and strong gravitational fields. It also introduces the concept of spacetime, where space and time are not separate entities but are interconnected.

3. What are the implications of special relativity?

Special relativity has several implications, including the famous equation E=mc^2, which states that mass and energy are equivalent and can be converted into one another. It also explains the phenomenon of time dilation, where time appears to pass slower for objects that are moving at high speeds.

4. What are non-instantaneous force equations?

Non-instantaneous force equations are equations that take into account the time it takes for a force to act on an object. In classical mechanics, forces are assumed to act instantaneously, but in special relativity, the finite speed of light means that forces take time to propagate through space.

5. How do non-instantaneous force equations relate to special relativity?

Non-instantaneous force equations are a crucial part of special relativity because they allow us to accurately calculate the effects of forces on objects moving at high speeds. Without taking into account the finite speed of light, our understanding of motion and forces would be incomplete.

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