The Schwartzschild solution - why no Stress Tensor?

In summary: Schwarzschild geometry.In summary, the Schwartzschild solution tells us that there is a mass at the middle of a vacuum region that does not generate a stress energy tensor. This mass is a strange anomaly, and Experts seem to be unaware of it.
  • #36
atyy said:
I'm curious what your preferred terminology is for the maximally extended vacuum Schwarzschild solution. Would you say there is a mass in its centre (along the lines of the OP)?

Well, why not use that terminology you gave? It is said that the mass center of Schwartzschild spacetime is at the origin! Is there any problem with that terminology, atyy?

AB
 
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  • #37
Thanks to Birkhoff we know that we can 'remove' the mass from the solution. So even if there is not a black hole but an existing spherical mass, the spacetime curvature outside this mass is identical to the case of a black hole. Note that this is distinctly different from a Kerr solution, which is only valid in case there is a black hole. If there is no black hole and a rotating spherical mass we cannot use the Kerr solution for the spacetime outside this mass.
 
  • #38
Altabeh said:
Well, why not use that terminology you gave? It is said that the mass center of Schwartzschild spacetime is at the origin! Is there any problem with that terminology, atyy?

AB

Well, I go back and forth on this.

Option A: If we accept the mass at the centre, then we accept that the curvature singularity is physical, but there is no problem with matching to observations since there is an event horizon for this solution, cosmic censorship holds and there is no naked singularity.

Option B: OTOH, there is the more accepted point of view that the singularities of GR are unphysical, and imply a breakdown of the theory. In this view, it is usually said that we expect quantum gravity to replace GR at high curvatures, and the singularities will be "resolved" in such a theory.

Of course, if option A is acceptable, that doesn't mean that GR will not be replaced by some theory of quantum gravity, only that GR does not indicate its own failure at high curvatures.
 
  • #39
atyy said:
Well, I go back and forth on this.

Option A: If we accept the mass at the centre, then we accept that the curvature singularity is physical, but there is no problem with matching to observations since there is an event horizon for this solution, cosmic censorship holds and there is no naked singularity.

Option B: OTOH, there is the more accepted point of view that the singularities of GR are unphysical, and imply a breakdown of the theory. In this view, it is usually said that we expect quantum gravity to replace GR at high curvatures, and the singularities will be "resolved" in such a theory.

Of course, if option A is acceptable, that doesn't mean that GR will not be replaced by some theory of quantum gravity, only that GR does not indicate its own failure at high curvatures.

Well I think the option one is widely accepted but there is a question then arising from the existence of a physical singularity at the center: Do you think the appearence of such singularity is a failure for GR?

I recently hit this http://www.holoscience.com/news/img/DPS%20talk.pdf" on the Internet which claims based on the falsifying Hilbert's version of Schwarzschild solution, our knowledge of Schwarzschild metric has grown up in the wrong way and the definition of "r" in this spacetime "has never been rightly identified by the physicists"! I did not take my time to read the whole paper but you might do so in order to find out if the option A lacks the defect you mentioned!

AB
 
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  • #40
Altabeh said:
Well I think the option one is widely accepted but there is a question then arising from the existence of a physical singularity at the center: Do you think the appearence of such singularity is a failure for GR?

I recently hit this http://www.holoscience.com/news/img/DPS%20talk.pdf" on the Internet which claims based on the falsifying Hilbert's version of Schwarzschild solution, our knowledge of Schwarzschild metric has grown up in the wrong way and the definition of "r" in this spacetime "has never been rightly identified by the physicists"! I did not take my time to read the whole paper but you might do so in order to find out if the option A lacks the defect you mentioned!

AB

I am quite happy (intellectually) to live with a singularity in the universe. I don't see how the singularities are mathematical inconsistencies, nor do I see any conflict with observation (in principle).

The paper you mentioned is famous on PF - it's complete nonsense.
 
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  • #41
Altabeh said:
That is not so much of pain for me to quote a paragraph of book that I deal with every day! That is you who have brought up the idea of "what is better" and "when who is right" so do not digress the discussion through playing with words! I exactly said that

You posted something that was factually incorrect. Now , it sems I'm on the defensive (or supposed to be on the defensive) for daring to mention it. Meh.

And you cut a quarter of it, I guess!

Oh - the utter horror, of trimming a reference to a book that you "deal with every day." But you certainly are good at dragging up irrelevancies that serve to derail any serious discussion of the original issue at hand, i.e. the difference between the mass M in the Schwarzschild line element and integrating rho * volume, which yield two different numbers.

To recap the discussion to date.

1) I mentioned, briefly, that the two numbers were different, and provided a textbook reference that showed the difference.

2) This gets ignored, and you suggest that "I'm confused" (which is rather rude), and you provide a reference of your own. Having access to said reference, I read it, and it doesn't support your position, and agrees with my reference.

3) I point this out, and go to the trouble of actually quoting a large section of the reference, bolding the important points. You respond by saying "you deal with the book everyday", and seem to suggest that quoting references is an unseemly way to settle an argument. I suppose it's much better to settle arguments by saying "I deal with the book everyday", an appeal to (non-existent, but presumably desired) personal authority.

Sorry - it's pretty clear to me that you aren't listening, and that you like to flame and debate rather than to discusss the actual physics involved.
 
  • #42
@pervect: Isn't Altabeh's equations exactly the same as 10.41 on p259 of Schutz? ie. it isn't over elements of "proper volume".
 
  • #43
atyy said:
@pervect: Isn't Altabeh's equations exactly the same as 10.41 on p259 of Schutz? ie. it isn't over elements of "proper volume".

While one does integrate 4 pi r^2 dr to get the mass (10.41 of Schutz), the resemblence of 10.41 to a volume element is only formal. 10.41 is *not* equivalent to integrating the volume times the density. It's an easy mistake to make if one is unwary - Schutz warns specifically against it , and I was essentially doing the same.

The proper volume element is (4 pi r^2) (dr / sqrt(1-2M/r)) for the constant density star case and

[tex]
4 \pi r^2 e^{\Lambda} dr
[/tex]

in the more general case where the interior metric is

[tex]
(e^{\Phi} dt)^2 + (e^{\Lambda} dr)^2 + (r d \theta)^2 + (r \sin \theta d\phi)^2
[/tex]
 
  • #44
stevenb said:
I understand TerryW's concerns. Sometimes the whole thing seems like magic. But that's the price we sometimes pay for elegant solutions. They are so amazing and powerful that they seem impossibly simple and even somewhat magical.

Well my post does seem to have generated a lot of interest and debate. For the moment, I'm going to carry on working with the 'accepted' paradigm but to me, this elegant solution has a big wart at the end of its nose!

Regards to all
 
  • #45
pervect said:
You posted something that was factually incorrect. Now , it sems I'm on the defensive (or supposed to be on the defensive) for daring to mention it. Meh.

Ugh, what factually is wrong is that your eyes must be rolled over all the sentences people write here! I don't have time to help you out with that problem! Sorry!

Oh - the utter horror, of trimming a reference to a book that you "deal with every day." But you certainly are good at dragging up irrelevancies that serve to derail any serious discussion of the original issue at hand, i.e. the difference between the mass M in the Schwarzschild line element and integrating rho * volume, which yield two different numbers.

Another nonsense you're making here is that you clearly ignore the fact that still Schutz has not changed his mind on his equation 10.41. I'm still insisting that you're hugely confused because you said Newtonian mass is not as important as it is in classical mechanics! All I said is that you better look at Schutz' notes to understand we do not really need any relativistic contribution to the mass term because certainly m/r<<1 for almost all known stars\planets and stuff! It seems to me that you're like the guy who doesn't neglect the second order terms and so on in linearizing field equations because he "thinks" such terms would contribute to the results enormously. With all such nonsense claims that you've made about the importance of Newtonian mass in GR, nothing has changed the minds to stop thinking about it to date! You better understand that in almost every critical situation in GR, as in the case where we want to introduce "conservation laws", the use of Newtonian definition of mass is unbelievably excessive! If you still disbelieve it , I can quote from the "books" I've read until now! I'm not of non-scientific type!

To recap the discussion to date.

1) I mentioned, briefly, that the two numbers were different, and provided a textbook reference that showed the difference.

And if there is any confusion about this is from your side!

2) This gets ignored, and you suggest that "I'm confused" (which is rather rude), and you provide a reference of your own. Having access to said reference, I read it, and it doesn't support your position, and agrees with my reference.

Yet you're confused which this quote from atyy's post makes me strongly confortable with this credo:

atyy said:
@pervect: Isn't Altabeh's equations exactly the same as 10.41 on p259 of Schutz? ie. it isn't over elements of "proper volume".


3) I point this out, and go to the trouble of actually quoting a large section of the reference, bolding the important points. You respond by saying "you deal with the book everyday", and seem to suggest that quoting references is an unseemly way to settle an argument. I suppose it's much better to settle arguments by saying "I deal with the book everyday", an appeal to (non-existent, but presumably desired) personal authority.

Irrelevant! This is not psychology class and you're not the one who has authority over the others to see things from that angle!

Sorry - it's pretty clear to me that you aren't listening, and that you like to flame and debate rather than to discusss the actual physics involved.

Looking at my posts, everybody can see if I'm talking about actual physics! So let people judge!

AB
 
  • #46
pervect said:
While one does integrate 4 pi r^2 dr to get the mass (10.41 of Schutz), the resemblence of 10.41 to a volume element is only formal. 10.41 is *not* equivalent to integrating the volume times the density.

What? Either I can't understand this or the problem is you can't understand that in the case of a spherically symmetric material distribution,

[tex]\rho=\rho(r)[/tex]

with r being the distance from the center of symmetry, we clearly have

[tex]M=\int \rho d^3x[/tex].

If you're against this argument, then you're not even wrong! I can assert this by quoting another book I've read! But since you believe it is not right, then I don't!

It's an easy mistake to make if one is unwary - Schutz warns specifically against it , and I was essentially doing the same.

In general relativity, it is like a very easy essay: In case you're in a nearly flat spacetime, all contributions from gravitational energies are neglected and thus the definition gets narrowed down to

[tex]M=E/c^2=c^{-2}\int_V T_{00}dV. [/tex]

And this may sound deceptive, but it is always written in that way!

The proper volume element is (4 pi r^2) (dr / sqrt(1-2M/r)) for the constant density star case and

[tex]
4 \pi r^2 e^{\Lambda} dr
[/tex]

in the more general case where the interior metric is

[tex]
(e^{\Phi} dt)^2 + (e^{\Lambda} dr)^2 + (r d \theta)^2 + (r \sin \theta d\phi)^2
[/tex]

Nice try! We are all aware of that!

AB
 
  • #47
atyy said:
@pervect: Isn't Altabeh's equations exactly the same as 10.41 on p259 of Schutz? ie. it isn't over elements of "proper volume".

Oh, the other thing I should have added is that while the initial error in confusing the volume elements may seem small and unimportant, the subsequent error in ignoring the contribution of gravitational binding energy to mass results in really, really bad self-consistency problems.

I'd be tempted to get more into how bad this is, but it's hard to find textbooks that discuss it (they focus on doing things right in the first place, not disucssing the consequences of incorrect assumptions), and the discussion isn't proceeding well for a less formal approach.
 
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  • #48
pervect said:
Oh, the other thing I should have added is that while the initial error in confusing the volume elements may seem small and unimportant, the subsequent error in ignoring the contribution of gravitational binding energy to mass results in really, really bad self-consistency problems.

I'd be tempted to get more into how bad this is, but it's hard to find textbooks that discuss it (they focus on doing things right in the first place, not disucssing the consequences of incorrect assumptions), and the discussion isn't proceeding well for a less formal approach.

I do understand the difference between the two integrals. But isn't Altabeh's equation the exactly correct one, since he is not integrating over proper volume elements (well, technically it's hard to tell, since the Schwarzschild solution is usually given in coordinates that don't have x,y,z, whereas his equation has dxdydz, so one would need to know how x,y,z in his equation relate to the usual coordinates).
 
  • #49
atyy said:
I do understand the difference between the two integrals. But isn't Altabeh's equation the exactly correct one, since he is not integrating over proper volume elements (well, technically it's hard to tell, since the Schwarzschild solution is usually given in coordinates that don't have x,y,z, whereas his equation has dxdydz, so one would need to know how x,y,z in his equation relate to the usual coordinates).

How does "ambiguous and invites confusion" sound (rather than exactly corrrect)? Schutz's 10.41

[tex]\int 4 \, \pi r^2 \, \rho \, dr[/tex]

would be "exactly correct", and would be an adequate definition of mass for a static, spherically symmetric space-time, though unfortunately it does not generalize, and it's also written in a coordinate dependent form.

One of the OTHER issues with writing d^3x, aside from the fact that it's at best unclear, is that it invites the reader to believe that the formula would apply in cases other than a static, spherically symmetric space-time, which is not the case.

The formula is coordinate dependent. The notation d^3x does not match the coordinates used, which must be the Schwarzschild coordinates for the formula to work.
 
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  • #50
pervect said:
How does "ambiguous and invites confusion" sound (rather than exactly corrrect)? Schutz's 10.41

[tex]\int 4 \, \pi r^2 \, \rho \, dr[/tex]

would be "exactly correct", and would be an adequate definition of mass for a static, spherically symmetric space-time, though unfortunately it does not generalize, and it's also written in a coordinate dependent form.

One of the OTHER issues with writing d^3x, aside from the fact that it's at best unclear, is that it invites the reader to believe that the formula would apply in cases other than a static, spherically symmetric space-time, which is not the case.

The formula is coordinate dependent. The notation d^3x does not match the coordinates used, which must be the Schwarzschild coordinates for the formula to work.

Sure - it's just that Altabeh was commenting on one of my posts, and (not initially) after rereading his post I gave Altabeh the benefit of the doubt from my experience with his usually reliable posts, and his readiness to correct any of his technical errors (almost all disagreements are usually purely about terminology).
 
  • #51
pervect said:
I'd be tempted to get more into how bad this is, but it's hard to find textbooks that discuss it (they focus on doing things right in the first place, not disucssing the consequences of incorrect assumptions), and the discussion isn't proceeding well for a less formal approach.

Textbooks do not go into such unipmortant things because it is of no concern in the models we have discussed to date about the structure of spacetime in a nearly flat spacetime! If you claim you got something interesting and instructive, then I'm ready to discuss it! But on a personal point, there you won't come up with anything appealing if you want to take the binding energy into account because the correction terms appearing in the equation are very tiny compared to terms up to the linear order! In the same book, on page 158, when Schutz proves a theorem on local flatness, you can see that the non-vanishing of terms like [tex]g_{ab,cd}[/tex], [tex]g_{ab,cde}[/tex] in the geodesic coordinates are definitely not guaranteed so they appear in the Taylor expansion of [tex]g'_{ab}[/tex] meaning that in the neighbourhood of a particular point, say, P at which a coordinate basis is chosen so that the metric is flat, metric may not really be "nearly" flat according to the fact that there is an infinite sum over all terms of higher order in the metric derivatives! But this is simply negligible because infinitesimally small as an "assumption" means [tex]x^a-x^a_p[/tex] are supposed to be really small that all that sum is inconsiderable!

Such assumptions as the one mentioned above are generally true even if your spacetime is stupidly curved and the the contribution of metric-derivative factors go over the top compared to the factors involving multiples of coordinate differences! But no one has ever claimed the theorem of local flatness wouldn't work somewhere around the intrinsic singularity of Schwartzschild metric!

I'm always ready to hear new ideas and if you think this is something never been worked out, it is time to shine and let us know if it deservers to be published!

AB
 
  • #52
Having now got as far as Chapter 18 and the Reisner Nordstrom solution, it is interesting to see that you put in the Maxwell Tensor, work through to a solution and lo, the solution contains a term which we can identify as the charge sitting at the origin. It also contains the mass sitting at the origin, but this appears without having started out with a Mass/Energy Tensor!

I'm kind of resigned to a train of thought that goes along the line that the general solution worked out from the canonical form of the metric produces a general solution which says that a space will be flat if there is no mass at the origin and curved if there is, but I can't say I'm all that happy!
 
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