Conservation of angular momentum in GR

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SUMMARY

Total angular momentum is not conserved in general relativity (GR) due to the lack of spacetime spherical symmetry, which necessitates the radiation of angular momentum from the quadrupole moment as gravitational radiation. In the Earth-moon system, tidal torques from both the moon and the sun alter the Earth's spin angular momentum, yet the total angular momentum is effectively conserved as the moon's orbit expands by approximately 4.5 cm/year. This conservation occurs because the gravitational field of the Earth-moon system is asymptotically flat, allowing for angular momentum conservation in this specific context. The Kerr spacetime, while asymptotically flat, exhibits an axisymmetric metric, leading to the conclusion that total angular momentum is not conserved in such configurations.

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  • Understanding of general relativity (GR) principles
  • Familiarity with angular momentum concepts in physics
  • Knowledge of tidal forces and their effects on celestial bodies
  • Basic comprehension of asymptotic flatness in spacetime
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  • Study the conservation of angular momentum in asymptotically flat spacetimes
  • Examine the role of tidal forces in the Earth-moon system
  • Learn about the Kerr metric and its implications in GR
  • Explore gravitational radiation and its effects on angular momentum
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Astrophysicists, theoretical physicists, and students of general relativity seeking to deepen their understanding of angular momentum conservation and its implications in gravitational systems.

  • #31
Loinger is a kook with academic credentials. In addition to the kookery discussed by PAllen, Loinger and his coauthor Marsico believe that there is something wrong with the standard analysis of black holes: http://arxiv.org/abs/1011.2600 Basically they make a big deal out of the fact that an observer at infinity sees infalling matter take an infinite amount of time to reach the event horizon. They treat this as having Dramatic Physical Implications, and they criticize other authors: "Now, if we take into account the decisive role of the Hilbertian gravitational repulsion, which is neglected by [Broderick et al.][...]" This is stupid and misleading, since Broderick hasn't made a mistake by ignoring some relevant effect. The "repulsion" isn't really a repulsion; it's just a *coordinate* acceleration with no intrinsic physical significance. An observer at infinity sees infalling material as taking infinite time to reach the event horizon, and since the Schwarzschild t coordinate is the time measured by an observer at infinity, the coordinate acceleration d2r/dt2 has an outward direction.
 
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  • #32
Sam Gralla said:
I think probably all that is going on here is that the earth-moon system analysis you read about is in a non-relativistic (i.e., Newtonian) limit, where there is no gravitational radiation. In reality it will radiate a bit of angular momentum, but my guess is this is tiny and simply being neglected in whatever you read about. In a binary pular, on the other hand, there is a lot of gravitational radiation.
Yes, I also think that's all.
I guess in a Newtonian-limit non-relativistic analysis of the binary pulsar, you do have total angular momentum conservation with no gravitational radiation, with the orbit angular momentum (shortening of the orbital period) compensated by the spin angular moment of the pulsar (acceleration of spin) just like in the earth-moon system Newtonian treatment the slowing of the Earth spin is compensated by the enlarging of the orbit and therefore total angular momentum is conserved.

Sam Gralla said:
Whether to use angular momentum defined at null or spatial infinity is just a choice. If you want to see how much angular momentum escapes as radiation, you use null infinity. If you want to see that angular momentum is always conserved, as long as the angular momentum in the radiation is included, you use spatial infinity. Both are well defined for any asymptotically flat spacetime (although the definitions of asymptotic flatness people give in the respective cases can be a little bit different). I didn't really make this comment in response to your original question; it's just I noticed some people were saying "angular momentum is conserved" and some people were saying "no, you can radiate it away", and the different definitions of angular momentum are probably the cause there.
Yeah, there is some confusion about asymptotically flat spacetimes, it is not an easy theme for non-experts at least. Part is derived from the fact that this and many other common themes in GR have a lot to do with the concepts of "conformal infinity" and "null infinity" that are not usually treated with depth in introductory texts but that are vital to give a sound theoretical basis to GW, black holes etc.
Here is a pretty informative site about this: http://relativity.livingreviews.org/Articles/lrr-2004-1/

Also as I read angular momentum in GR is a thorny subject, or it has been until relatively recently.
 
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  • #33
PAllen said:
Real, massive bodies closely approximate geodesics, but the difference cannot be ignored for a system like two orbiting pulsars. Thus I immediately suspect the whole body of work.
Most likely this guy's work is flawed, but not for this reason.
If we are limiting the analysis to bodies trajectories is perfectly licit to talk about geodesics for anybody trajectory, the fact that in the surface of a massive body test particles at rest are not following geodesic motion is not relevant in this case. The fact is curvature of spacetime (gravity) manifests thru the convergence-divergence of geodesic trajectories.
 
  • #34
TrickyDicky said:
PAllen said:
Real, massive bodies closely approximate geodesics, but the difference cannot be ignored for a system like two orbiting pulsars. Thus I immediately suspect the whole body of work.
Most likely this guy's work is flawed, but not for this reason.
If we are limiting the analysis to bodies trajectories is perfectly licit to talk about geodesics for anybody trajectory, the fact that in the surface of a massive body test particles at rest are not following geodesic motion is not relevant in this case. The fact is curvature of spacetime (gravity) manifests thru the convergence-divergence of geodesic trajectories.
No, PAllen was correct, and he wasn't saying anything about surfaces. Bodies with nonnegligible mass don't follow geodesics because they radiate gravitational waves.
 
  • #35
TrickyDicky; said:
If we are limiting the analysis to bodies trajectories is perfectly licit to talk about geodesics for anybody trajectory, the fact that in the surface of a massive body test particles at rest are not following geodesic motion is not relevant in this case. The fact is curvature of spacetime (gravity) manifests thru the convergence-divergence of geodesic trajectories.
Can't argue the specifics, but agree 100% it's not proper to dismiss anyone who makes a serious argument without presenting their entire rationale first. While no doubt PAllen in #29 meant only the best, it would have been a bit kinder to A.Loinger to have quoted the remainder of the intro "..If we add non-gravitational forces, the conclusion remains the same, because the new trajectories do not possesses kinematical elements (velocity, acceleration,
time derivative of the acceleration, etc.) different from those of the geodesic motions."
Not saying the final conclusion in the full course of time would be different, but, inadvertently or not, excising aspects of his pov paints a particularly simplistic 'straw man' picture. Likewise, bcrowell's costic assessment in #31 to my mind doesn't address the fact that while 'Hilbertian repulsion' may be a poor way of labelling things, is it truly 'of no physical significance' that in Schwarzschild coords a distant observer finds infalling matter will decelerate to zero velocity on approach to the nominal EH of a nominal stationary BH? Isn't this a legitimate 'physically meaningful' perspective, even if the terminology 'repulsion' is somewhat misguided? I'm not the only one to have pointed out that 'infinite redshift' is more than mere 'optical illusion' in this setting -it has a genuine physical meaning, imho at least. And honestly, it may be true Loinger is ultimately off the mark, but is it right to label such folks with terms like 'kook', 'nutter'. 'fringe', 'weirdo', [insert your own pejorative and demonizing term(s) here..]? More reasonable surely to just say 'mistaken', 'minority view' etc. Can't help but see parallels with a particularly intolerant and 'huge vote of hands' religious movement that has just one word for dissenters - 'infidel'.
One last thing here. Notwithstanding TrickyDicky's accepting stance, fact is I have created a 2-stream thread here, and am officially 'pulling' my part of that at this point. Will be in due time be reformulating and starting as new thread - who knows, I might even get some decent feedback (exempting two participants from that observation!).
 
  • #36
Q-reeus said:
Can't argue the specifics, but agree 100% it's not proper to dismiss anyone who makes a serious argument without presenting their entire rationale first. While no doubt PAllen in #29 meant only the best, it would have been a bit kinder to A.Loinger to have quoted the remainder of the intro "..If we add non-gravitational forces, the conclusion remains the same, because the new trajectories do not possesses kinematical elements (velocity, acceleration,
time derivative of the acceleration, etc.) different from those of the geodesic motions."

I stopped quoting where I did for a very specific reason - the point at which a statement was made that differed with 70 years of virtually all other researcher's conclusions going back to Einstein and Infeld. Further, it is, in fact, pretty obvious that if all massive bodies follow geodesics exactly, there is no GW. So this is the fundamental starting point which must be disputed. And the way it is disputed is as I described: derive motion from the field equations rather than a-priori assuming the geodesic hypothesis.

Deriving motion from the field equations is a complex prodedure, but it has been done now dozens of different ways by many researcher's over decades, reaching common conclusions. There is no need to bring in non-gravitational forces to dispute the erroneous starting point.
 
  • #37
PAllen said:
I stopped quoting where I did for a very specific reason - the point at which a statement was made that differed with 70 years of virtually all other researcher's conclusions going back to Einstein and Infeld. Further, it is, in fact, pretty obvious that if all massive bodies follow geodesics exactly, there is no GW. So this is the fundamental starting point which must be disputed. And the way it is disputed is as I described: derive motion from the field equations rather than a-priori assuming the geodesic hypothesis.

Deriving motion from the field equations is a complex prodedure, but it has been done now dozens of different ways by many researcher's over decades, reaching common conclusions.
Thanks for that clarification. As I say I can merely comment on the sidelines at that level. If I recall it right though Einstein himself was a doubter of GW's some twenty odd years after publishing the final version of GR. Lucky I believe to have his reputation saved by an anonymous journal referee who knocked back his 'rebuttal' of GW's as physically real. Subsequently someone persuaded him otherwise no doubt. And to his dying day refused to believe BH's were possible - maybe a sad case of pupil's supplanting teacher; don't know myself.
 
  • #38
Q-reeus said:
Thanks for that clarification. As I say I can merely comment on the sidelines at that level. If I recall it right though Einstein himself was a doubter of GW's some twenty odd years after publishing the final version of GR. Lucky I believe to have his reputation saved by an anonymous journal referee who knocked back his 'rebuttal' of GW's as physically real. Subsequently someone persuaded him otherwise no doubt. And to his dying day refused to believe BH's were possible - maybe a sad case of pupil's supplanting teacher; don't know myself.

Yes, it is well known that Einstein never accepted that Black holes could form by realisitic physical processes. However, he didn't live to see the work of Chandresekhar, Penrose, and Hawking. I expect he would have been swayed.
 
  • #39
PAllen said:
I stopped quoting where I did for a very specific reason - the point at which a statement was made that differed with 70 years of virtually all other researcher's conclusions going back to Einstein and Infeld. Further, it is, in fact, pretty obvious that if all massive bodies follow geodesics exactly, there is no GW. So this is the fundamental starting point which must be disputed. And the way it is disputed is as I described: derive motion from the field equations rather than a-priori assuming the geodesic hypothesis.
So would you argue that the adimensional point that is the center of gravity of a massive body is not following a geodesic motion no matter how massive, is it not following an inertial path (in GR terms)?
 
  • #40
TrickyDicky said:
So would you argue that the adimensional point that is the center of gravity of a massive body is not following a geodesic motion no matter how massive, is it not following an inertial path (in GR terms)?

Yes, massive, non-singular bodies do not exactly follow geodesics. Out of curiosity, I researched a little when this was first convincingly shown, and it is even earlier than I thought. Vladimir Fock showed in 1939 that non-singular bodies that are massive enough to have self gravitation (again, no need for any non-gravitational forces to be considered) do not exactly follow geodesics.

[EDIT: And, continuing the historic trend of putting messy calculations on a more rigorous footing, here is a paper by a recent contributor to these forums verifying the main conclusions of Fock:

http://arxiv.org/abs/0806.3293
]
 
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  • #41
PAllen said:
Yes, massive, non-singular bodies do not exactly follow geodesics.

This is IMO an important point worth to clarify. I would say that by the Equivalence principle, the adimensional center of mass of any massive body is considered "a local inertial frame" and must be following exactly a geodesic path. Is this statement not true? Or is the Equivalence principle not stating this? Or is the equivalence principle not valid here?
 
  • #42
TrickyDicky said:
This is IMO an important point worth to clarify. I would say that by the Equivalence principle, the adimensional center of mass of any massive body is considered "a local inertial frame" and must be following exactly a geodesic path. Is this statement not true? Or is the Equivalence principle not stating this? Or is the equivalence principle not valid here?

Why would the inside of massive body be expected to be (precisely) a local inertial frame? I would expect the opposite, in the sense the metric cannot be transformed to Minkowski form over the scale of interest (the massive body).

The principle of equivalence is problematic as a precise rule, rather than a useful guide, as Bcrowell and others here have helped me understand with pointers to various papers.

However, Clifford Will discusses his take on its usage for precisely this scenario of massive self gravitating bodies:

http://relativity.livingreviews.org/Articles/lrr-2006-3/

especially sections 3.1.2, 4.1.1 and 4.1.2
 
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  • #43
PAllen said:
Why would the inside of massive body be expected to be (precisely) a local inertial frame? I would expect the opposite, in the sense the metric cannot be transformed to Minkowski form over the scale of interest (the massive body).

The center of mass is the single point on a structure which characterizes the motion of the object if the object shrinks to a point mass.
In a curved spacetime, obviously the center of mass is not following an SR inertial path, but a geodesic, or the straightes path in a curved space, but now you are saying that a massive enough body's trajectory,(wich can be characterized by that of its center of mass, as if it were a test particle)is not a geodesic, and I just don't understand what the reason is, all books I consult say in the absence of non-gravitational forces a body follows geodesic motion, can you explain with your own words why this is not the case?




PAllen said:
The principle of equivalence is problematic as a precise rule, rather than a useful guide
But it's still valid, right? at the very least in its weak form.
 
  • #44
TrickyDicky said:
The center of mass is the single point on a structure which characterizes the motion of the object if the object shrinks to a point mass.
In a curved spacetime, obviously the center of mass is not following an SR inertial path, but a geodesic, or the straightes path in a curved space, but now you are saying that a massive enough body's trajectory,(wich can be characterized by that of its center of mass, as if it were a test particle)is not a geodesic, and I just don't understand what the reason is, all books I consult say in the absence of non-gravitational forces a body follows geodesic motion, can you explain with your own words why this is not the case?

But it's still valid, right? at the very least in its weak form.

I don't know of any simple justification. When a body must be treated as both a source of gravitation and responding to gravitation, The EFE are are complex, non-linear. I have read through a couple of such analyses of motion from the EFE, most carefully an old one by Synge (1960), and followed that different methods keep coming to the same conclusion. I was under the belief that center of mass is ill defined in GR, but have not really thought much about it. Birkhoff's theorem is only defined for non-rotating spherical bodies, which is what would lead me to think that the ability to treat any other body as equivalent to mass at a point is suspect.

As for the equivalence principle, in its most classic form (indistinguishability of an accelerating lab from a lab sitting on a planet) , it is true only locally, when all tidal effects can be ignored. Will describes 3 other formulations (all different from Einstein's original formulation). He argues that GR is the only known theory, consistent with experiment, that satisfies all of his 3 forms of equivalence principle. His strong one is specifically designed to be tested in the presence of massive self gravitating bodies that radiate and don't follow geodesics exactly.

[Edit: If you're willing to tackle it, I really got the impression the Sam Gralla paper I linked to is much more careful than any prior presentation I've read. Since you seem particularly sensitive to 'ignored details' (not a bad thing at all), this paper might be more satisfying than other treatments. Repeating the link:
http://arxiv.org/abs/0806.3293 ]
 
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  • #45
TrickyDicky said:
The center of mass is the single point on a structure which characterizes the motion of the object if the object shrinks to a point mass.
In a curved spacetime, obviously the center of mass is not following an SR inertial path, but a geodesic, or the straightes path in a curved space, but now you are saying that a massive enough body's trajectory,(wich can be characterized by that of its center of mass, as if it were a test particle)is not a geodesic, and I just don't understand what the reason is, all books I consult say in the absence of non-gravitational forces a body follows geodesic motion, can you explain with your own words why this is not the case?

Amplifying on PAllen's response to this question: --

If the books you are referring to are carefully written, they should not say that "in the absence of non-gravitational forces a body follows geodesic motion." They should say that "in the absence of non-gravitational forces a body with negligible mass follows geodesic motion."

The basic reason is the one I gave in #34.

-Ben
 
  • #46
PAllen said:
[Edit: If you're willing to tackle it, I really got the impression the Sam Gralla paper I linked to is much more careful than any prior presentation I've read. Since you seem particularly sensitive to 'ignored details' (not a bad thing at all), this paper might be more satisfying than other treatments. Repeating the link:
http://arxiv.org/abs/0806.3293 ]

Another rigorous paper is this one: Ehlers and Geroch, http://arxiv.org/abs/gr-qc/0309074v1

It is nontrivial to even formulate what is meant by geodesic motion of a test body, and a lot of the Ehlers and Geroch paper is taken up with that.

Another thing to note is that if energy conditions are violated, you can't necessarily prove geodesic motion of test bodies.

I made an attempt here http://www.lightandmatter.com/html_books/genrel/ch08/ch08.html#Section8.1 (subsection 8.1.3) to explain the Ehlers and Geroch argument in a way that would be accessible to people who are not big-time GR technicians. It's hard to say whether I succeeded, since I'm not a big-time GR technician myself :-)
 
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  • #47
PAllen said:
I don't know of any simple justification. When a body must be treated as both a source of gravitation and responding to gravitation, The EFE are are complex, non-linear. I have read through a couple of such analyses of motion from the EFE, most carefully an old one by Synge (1960), and followed that different methods keep coming to the same conclusion. I was under the belief that center of mass is ill defined in GR, but have not really thought much about it. Birkhoff's theorem is only defined for non-rotating spherical bodies, which is what would lead me to think that the ability to treat any other body as equivalent to mass at a point is suspect.
It is true that the center of mass is ill defined in GR, according to Krasinski "Introduction to general relativity": " In relativity, so far there is not even a generally accepted definition of the centre of mass, although work on this problem is being done. Thus, when we consider the orbits of point bodies in relativity, we are in fact extending the theory into the domain in which it has not been worked out yet. Nevertheless, these results agree with observational tests."
In practice orbits are considered geodesic paths and I haven't found any reason to think this shouldn't apply to the binary pulsar orbit. A reference where this is stated explicitly would help.

PAllen said:
As for the equivalence principle, in its most classic form (indistinguishability of an accelerating lab from a lab sitting on a planet) , it is true only locally, when all tidal effects can be ignored. Will describes 3 other formulations (all different from Einstein's original formulation). He argues that GR is the only known theory, consistent with experiment, that satisfies all of his 3 forms of equivalence principle. His strong one is specifically designed to be tested in the presence of massive self gravitating bodies that radiate and don't follow geodesics exactly.
That is a valuable opinion but it's just C. Will's, not necessarily the consensus in GR.
PAllen said:
[Edit: If you're willing to tackle it, I really got the impression the Sam Gralla paper I linked to is much more careful than any prior presentation I've read. Since you seem particularly sensitive to 'ignored details' (not a bad thing at all), this paper might be more satisfying than other treatments. Repeating the link:
http://arxiv.org/abs/0806.3293 ]
The notion of self-gravitation is not without its own conceptual problems , since the gravitational field can be made to vanish for a free-falling body following a geodesic path or just by choosing the appropriate coordinates.

The bottom-line is much of this seems to be not fully worked out yet, and no generally accepted conclusion has been drawn, in this context, leaning on recent papers not yet fully validated to reject completely a perhaps valid premise is not appropriate IMO.
It just seems unfair to anybody's work, no matter how flawed it seems to dismiss it just by saying that his premise is clearly wrong because it is obvious that GW exist when his purpose is precisely to prove that they don't exist.
 
  • #48
bcrowell said:
I made an attempt here http://www.lightandmatter.com/html_books/genrel/ch08/ch08.html#Section8.1 (subsection 8.1.3) to explain the Ehlers and Geroch argument in a way that would be accessible to people who are not big-time GR technicians. It's hard to say whether I succeeded, since I'm not a big-time GR technician myself :-)
There seems to be some conflating between geodesic in curved spacetime and inertial paths in flat spacetime here. For instance when you assert: "The world-line of a such a body therefore depends on its mass, and this shows that its world-line cannot be an exact geodesic, since the initially tangent world-lines of two different masses diverge from one another, and these two world-lines can't both be geodesics."
First, in flat space parallel inertial paths remain paralle but in curved space all initially parallel geodesics diverge.
Second, I thought all bodies, no matter their mass are affected in the same way by gravity (curvature), isn't that the principle of equivalence between inertial mass and gravitational mass? or the reason a hammer and a feather fall at the same time on the moon's floor.
Also, why can't both be geodesics?, in a sphere longitude lines departing from the poles diverge and they are all geodesics. The divergence of the masses is derived from the fact that in a real setting gravitational fields are not uniform, orbiting bodies have a near spherical shape so when acting as sources of curvature they produce different geodesics for different giving rise to tidal forces, in fact that is the reason we feel the curvature, and what geodesic deviation measures.

Also it is obvious that not all points in a massive body follow a geodesic path,(maybe this is what you and Pallen mean) the further from the center of mass the more so, at the surface of the body, that is going to be rotating, a test particle at rest is not allowed to follow geodesic motion, that is felt as an acceleration that is commonly described "as gravity" but that in fact is due to non-gravitational forces, like the EM forces that keep matter united or the Pauli exclusion principle affecting fermions.

The cited Geroch paper seems to be in agreement with what I'm saying.On the other hand if all massive bodies, (which is the same that saying all bodies) fail to follow geodesic paths that would mean the only type of motion is non-geodesic motion and this doesn't seem to be right in GR.Perhaps it would be interesting to discuss this in a new thread since it is not directly related to the OP.
 
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  • #49
TrickyDicky said:
There seems to be some conflating between geodesic in curved spacetime and inertial paths in flat spacetime here. For instance when you assert: "The world-line of a such a body therefore depends on its mass, and this shows that its world-line cannot be an exact geodesic, since the initially tangent world-lines of two different masses diverge from one another, and these two world-lines can't both be geodesics."
First, in flat space parallel inertial paths remain paralle but in curved space all initially parallel geodesics diverge.
Initially parallel geodesics at a distance from one another diverge. Initially parallel geodesics at the same point are the same geodesic. (This follows from the fact that the geodesic equation is a second-order differential equation, and there are uniqueness theorems for the solutions of such equations.)

TrickyDicky said:
Second, I thought all bodies, no matter their mass are affected in the same way by gravity (curvature), isn't that the principle of equivalence between inertial mass and gravitational mass? or the reason a hammer and a feather fall at the same time on the moon's floor.
This is the same issue we keep coming back to. That is only an approximation for small masses.

TrickyDicky said:
Also, why can't both be geodesics?, in a sphere longitude lines departing from the poles diverge and they are all geodesics.
They aren't parallel at the pole.

TrickyDicky said:
The cited Geroch paper seems to be in agreement with what I'm saying.
No, you've misunderstood the paper.

TrickyDicky said:
On the other hand if all massive bodies, (which is the same that saying all bodies) fail to follow geodesic paths that would mean the only type of motion is non-geodesic motion and this doesn't seem to be right in GR.
Geodesic motion is the limiting case where the body's mass is small. This is standard stuff that you can find in any GR textbook. If you tell us what GR textbook(s) you own, we can point you to the relevant material in them.
 
  • #50
TrickyDicky said:
The bottom-line is much of this seems to be not fully worked out yet, and no generally accepted conclusion has been drawn, in this context, leaning on recent papers not yet fully validated to reject completely a perhaps valid premise is not appropriate IMO.
No, it has been fully worked out, there is a generally accepted conclusion, and it's been a generally accepted conclusion since roughly 1940 (some history here http://en.wikipedia.org/wiki/Sticky_bead_argument#Einstein.27s_double_reversal ).

TrickyDicky said:
It just seems unfair to anybody's work, no matter how flawed it seems to dismiss it just by saying that his premise is clearly wrong because it is obvious that GW exist when his purpose is precisely to prove that they don't exist.
You've misread what PAllen wrote in #29. He didn't assume gravitational waves. He described calculations that assume only the validity of the Einstein field equations.
 
  • #51
bcrowell said:
This is the same issue we keep coming back to. That is only an approximation for small masses.
The Weak Equivalence principle is an approximation for small masses?

bcrowell said:
They aren't parallel at the pole.
Ok change diverge by converge, are they not parallel at the equator?
bcrowell said:
No, you've misunderstood the paper.
Maybe so, but is it not trying to prove that small bodies follow geodesic motion?, how does that disagree with my trying to shed light about why shouldn't any size body's trajectory, which is a unidimensionalline regardless its size, be considered a geodesic motion?.
bcrowell said:
Geodesic motion is the limiting case where the body's mass is small.
I know the standard reason given to assert this is that massive bodies have a self-gravitation that interferes with the background curvature, but this seem counterintuitive when it is also asserted that freefalling bodies gravitational field vanishes at the appropriate coordinates, and that their inertial mass is equivalent to their gravitational mass.
 
  • #52
bcrowell said:
No, it has been fully worked out, there is a generally accepted conclusion, and it's been a generally accepted conclusion since roughly 1940 (some history here http://en.wikipedia.org/wiki/Sticky_bead_argument#Einstein.27s_double_reversal ).

I was referring to the center of mass in GR, what does that have to do with the GW and Einstein story?

bcrowell said:
You've misread what PAllen wrote in #29. He didn't assume gravitational waves. He described calculations that assume only the validity of the Einstein field equations.

In fact I was thinking of your post #34 when I wrote that. I misquoted Pallen.
 
  • #53
TrickyDicky said:
The Weak Equivalence principle is an approximation for small masses?
Here is a reasonably precise statement, with appropriate caveats, from Clifford Will:
"An alternative statement of WEP is that the trajectory of a freely falling “test” body (one not acted upon by such forces as electromagnetism and too small to be affected by tidal gravitational forces) is independent of its internal structure and composition "
TrickyDicky said:
Ok change diverge by converge, are they not parallel at the equator?
Bcrowell was clear that he was talking about parallel at the same point. An easy way to see that this must be true (though Bcrowell already gave you a perfectly clear one) is to use the parallel transport definition of geodesic: a curve that parallel transports its tangent vector. There is one curve for each tangent vector at a given point.
TrickyDicky said:
I know the standard reason given to assert this is that massive bodies have a self-gravitation that interferes with the background curvature, but this seem counterintuitive when it is also asserted that freefalling bodies gravitational field vanishes at the appropriate coordinates, and that their inertial mass is equivalent to their gravitational mass.

Are you saying that the earth, which is free falling around the sun, may be treated as if it has no gravitational field? I've never heard such a claim. Can you justify it or give a reference for what this could mean.
 
  • #54
PAllen said:
Here is a reasonably precise statement, with appropriate caveats, from Clifford Will:
"An alternative statement of WEP is that the trajectory of a freely falling “test” body (one not acted upon by such forces as electromagnetism and too small to be affected by tidal gravitational forces) is independent of its internal structure and composition "
So once again, are you saying that the WEP is not valid for massive bodies? only for idealized test particles? just asking...


PAllen said:
Bcrowell was clear that he was talking about parallel at the same point. An easy way to see that this must be true (though Bcrowell already gave you a perfectly clear one) is to use the parallel transport definition of geodesic: a curve that parallel transports its tangent vector. There is one curve for each tangent vector at a given point.
He also said if they are at the same point they are the same geodesic.

PAllen said:
Are you saying that the earth, which is free falling around the sun, may be treated as if it has no gravitational field? I've never heard such a claim. Can you justify it or give a reference for what this could mean.
We are talking about its path, and I'm saying the Earth's path is a geodesic. The Earth is of course a source of curvature too.
 
  • #55
So in the context of full GR treatment, when talking of 'small body' vs 'large body' re any departure from geodesic motion of co-orbiting masses, is this basically referring to mass as the only important determinant, or spatial extent? If the latter, wouldn't this imply it all hinging on 2nd and higher order extended body correction terms, making the rationale for GW generation quite different from the linearized theory where point masses are assumed?
 
  • #56
TrickyDicky said:
He also said if they are at the same point they are the same geodesic.

No, this is what Bcrowell said, that I was justifying a different way:

"Initially parallel geodesics at a distance from one another diverge. Initially parallel geodesics at the same point are the same geodesic. (This follows from the fact that the geodesic equation is a second-order differential equation, and there are uniqueness theorems for the solutions of such equations.)"

I was saying the parallel transport definition of a geodesic makes it obvious that this must be so.
 
  • #57
Q-reeus said:
So in the context of full GR treatment, when talking of 'small body' vs 'large body' re any departure from geodesic motion of co-orbiting masses, is this basically referring to mass as the only important determinant, or spatial extent? If the latter, wouldn't this imply it all hinging on 2nd and higher order extended body correction terms, making the rationale for GW generation quite different from the linearized theory where point masses are assumed?

I suspect that for an incompressible solid extended body falling in the presence of tidal forces, the COM must follow a geodesic or there will be a torque around the COM, which would violate conservation of angular momentum.

Maybe it's possible to prove this, but I haven't come across it.
 
  • #58
PAllen said:
Are you saying that the earth, which is free falling around the sun, may be treated as if it has no gravitational field? I've never heard such a claim. Can you justify it or give a reference for what this could mean.

I'm guessing he means that the connection can be made to vanish for a body in geodesic motion.
 
  • #59
Mentz114 said:
I suspect that for an incompressible solid extended body falling in the presence of tidal forces, the COM must follow a geodesic or there will be a torque around the COM, which would violate conservation of angular momentum...
OK thanks, but it's all been centering here about small departures from geodesic motion tying in or not with GW emission, and if spatial extent was a prerequisite, seemed very unlikely there would be even close to a match to the linearized GR quadrupole formula. Guessing the Hulse-Taylor system was basically treated as two orbiting point masses re orbital period decline at least - maybe extended bodies approach for more refined calcs. :zzz:
 
  • #60
Mentz114 said:
I suspect that for an incompressible solid extended body falling in the presence of tidal forces, the COM must follow a geodesic or there will be a torque around the COM, which would violate conservation of angular momentum.

Maybe it's possible to prove this, but I haven't come across it.

I don't think this is true. The body radiates gravitational waves at a rate that is proportional to the square of its mass. Therefore its trajectory depends on its mass, and can't be a geodesic.
 

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