Tests of EFE: Assessing General Relativity's Validity Beyond Cosmology

  • Thread starter CycoFin
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In summary: No, I did not write this for Wikipedia. I am just providing a summary of the conversation for the given task. The conversation was about the tests of general relativity and the validity of the Einstein field equations (EFE). The person expressing their concerns about the EFE being based on vacuum solutions and not being a good proof of validity. However, another person argued that the vacuum solutions still possess non-zero Weyl curvature and are valid solutions to the EFE. They also mentioned that changing the action being extremized can change the EFE and that the Schwarzschild metric satisfies all experimental tests. The conversation then delved into the logic of solving equations and how the EFE is a second order partial differential equation.
  • #1
CycoFin
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There are several tests of general relativity:

- gravitational redshift
- deflaction of light
- perihelion precession of Mercury
- Shapiro delay
- Lense-Thirring precession
- binary pulsars


Now comes the part that problems me. These all are based on vacuum solution of Einstein field equations.
With vacuum solution EFE is 0 = 0, IMO not that good proof of validity of equations.


So is there any real tests of EFE, other than Cosmology? (which have it's problems as we all know)

Also looking for good explanations why left side of EFE must equal right side.
 
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  • #2
CycoFin said:
There are several tests of general relativity:

- gravitational redshift
- deflaction of light
- perihelion precession of Mercury
- Shapiro delay
- Lense-Thirring precession
- binary pulsars


Now comes the part that problems me. These all are based on vacuum solution of Einstein field equations.
With vacuum solution EFE is 0 = 0, IMO not that good proof of validity of equations.


So is there any real tests of EFE, other than Cosmology? (which have it's problems as we all know)

Also looking for good explanations why left side of EFE must equal right side.

The field equations follow from extrememizing an action as in any field theory.

Your concerns about vacuum solutions are groundless. The vacuum solutions have zero Ricci tensor but still possesses non-zero Weyl curvature which
describes the field. It is very technical and if you study hard for a few years you will understand.
 
  • #3
CycoFin said:
With vacuum solution EFE is 0 = 0, IMO not that good proof of validity of equations.
You can always simplify any equation to that form if you choose. This is a complete non issue.

All of the tests you mention are non-trivial solutions to the EFE.
 
  • #4
Mentz114 said:
The field equations follow from extrememizing an action as in any field theory.

Your concerns about vacuum solutions are groundless. The vacuum solutions have zero Ricci tensor but still possesses non-zero Weyl curvature which
describes the field. It is very technical and if you study hard for a few years you will understand.

Can you then write EFE using only Weyl tensors? Is it so that basically Riemann tensor = Ricci tensor (trace part) + Weyl tensor(everything else)?

DaleSpam said:
You can always simplify any equation to that form if you choose. This is a complete non issue.

All of the tests you mention are non-trivial solutions to the EFE.

I disagree, the vacuum solution is the Schwarzschild metric which have 0 = 0
 
  • #5
CycoFin said:
Can you then write EFE using only Weyl tensors? Is it so that basically Riemann tensor = Ricci tensor (trace part) + Weyl tensor(everything else)?
The only way to change the EFE is to change the action being extremized.

A vacuum solution is created by solving the differential equations
##G(g)^{\mu\nu} =0##
where ##g## is a function of the coordinates. We thus find a valid metric, which gives us ##0=0##, which is what we wanted.

See here http://en.wikipedia.org/wiki/Deriving_the_Schwarzschild_solution
 
  • #6
Yes, deriving the schwarzschild solution we assume that rigth side must be zero because vacuum and then find metric that gives also left side zero (R = 0).

But this 0 = 0 does not prove that EFE is correct hypothesis. One can put anything one wants to the right side, just make sure it is zero (e.g. number of magnetic monopoles).

I ask again, is there any experimental tests that have rigth side of EFE not zero?
 
  • #7
CycoFin said:
Yes, deriving the schwarzschild solution we assume that rigth side must be zero because vacuum and then find metric that gives also left side zero (R = 0).

But this 0 = 0 does not prove that EFE is correct hypothesis. One can put anything one wants to the right side, just make sure it is zero (e.g. number of magnetic monopoles).

I ask again, is there any experimental tests that have rigth side of EFE not zero?

That is rubbish. You have to put the correct metric in. The metric is the solution. Your understanding of logic and mathematics is flawed.

The Schwarzschild metric satisfies all the experimental tests that have been tried - so your assumption is flawed in any case.

The equation ##x^2-2ax+a^2=0## has a solution ##x=a## which gives ##0=0##. What is wrong with that logic ?
 
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  • #8
Nothing is wrong with that logic.

You have proved that x2-2ax+a2 = 0 is true (have solution) but you have not proved that x2-2ax+a2 = b when b is not 0.

I agree that the Schwarzschild metric satisfies all the experimental tests that have been tried and those I listed on first post.

I just don't understand how Schwardschild metric can "prove" EFE if equation reads 0 = 0.
 
  • #9
CycoFin said:
Nothing is wrong with that logic.

You have proved that x2-2ax+a2 = 0 is true (have solution) but you have not proved that x2-2ax+a2 = b when b is not 0.

I agree that the Schwarzschild metric satisfies all the experimental tests that have been tried and those I listed on first post.

I just don't understand how Schwarzschild metric can "prove" EFE if equation reads 0 = 0.

Well, you need to understand what solving an equation means. It is like a set of scales. The scales still work when they have nothing to weight. They are saying ##0=0##.

Take the quadratic equation I wrote. I could have written ##x^2-2ax = -a^2##. Now put in the solution ##x=a##. Now the equation reads ##-a^2=-a^2##.

We know the solution is correct when both sides are the same.

I don't think I can help any further with this.
 
  • #10
CycoFin said:
With vacuum solution EFE is 0 = 0

No, it isn't. The EFE is a second order partial differential equation (more precisely, it's a system of 10 of them in the general case). So the RHS being zero just means it's a homogeneous second order partial differential equation, which certainly has solutions other than the trivial one. See here for an overview:

http://en.wikipedia.org/wiki/Vacuum_solution_(general_relativity)
 
  • #11
PeterDonis said:
No, it isn't. The EFE is a second order partial differential equation (more precisely, it's a system of 10 of them in the general case). So the RHS being zero just means it's a homogeneous second order partial differential equation, which certainly has solutions other than the trivial one. See here for an overview:

http://en.wikipedia.org/wiki/Vacuum_solution_(general_relativity)
So, you wrote this for wiki? Cool.
 
  • #12
John F. Gogo said:
you wrote this for wiki?

If you mean, did I write the Wikipedia page I linked to, no, I didn't. I just linked to it as a reference.
 
  • #13
CycoFin said:
I disagree, the vacuum solution is the Schwarzschild metric which have 0 = 0
So what? This is true of any solution of any equation. You can always simplify it to 0=0:

Given A=B
A-B=0 by subtraction
0=0 by substitution

It is a completely useless complaint because it is always true for any equation. If you over-simplify you can always get 0=0. Your query about experiments or observations with a non-vacuum metric is a valid question, but this bit about 0=0 is not.
 
  • #14
CycoFin said:
There are several tests of general relativity:

- gravitational redshift
- deflaction of light
- perihelion precession of Mercury
- Shapiro delay
- Lense-Thirring precession
- binary pulsars


Now comes the part that problems me. These all are based on vacuum solution of Einstein field equations.
With vacuum solution EFE is 0 = 0, IMO not that good proof of validity of equations.


Conceptually, these are not tests of the pure vacuum solutions, because in addition to the vacuum solution, geodesic motion is assumed. The geodesic motion is derived by assuming the presence of matter: http://arxiv.org/abs/0806.3293.

CycoFin said:
So is there any real tests of EFE, other than Cosmology? (which have it's problems as we all know)

What problems does cosmology have? Are you thinking about dark matter?

For general relativity with matter, there seems to still be research going in these areas;
http://www.einstein-online.info/spotlights/hydrodynamics_realm
http://arxiv.org/abs/1210.4921
http://arxiv.org/abs/1206.2503
 
  • #15
atyy said:
geodesic motion is derived by assuming the presence of matter

Just to clarify, this is referring to geodesic motion of bodies that are not "test bodies", because they have significant self-gravity, correct? For example, geodesic motion of the Earth in the gravitational field of the Sun.

This "presence of matter" is still very different from the "matter" that is present in cosmological solutions. In the latter, the matter significantly affects the spacetime geometry everywhere. In the former, the matter only significantly affects the spacetime geometry (in the sense of requiring a nonzero stress-energy tensor in the local solution of the EFE) in isolated regions corresponding to the central gravitating body producing the overall geometry (e.g., the Sun), and the self-gravitating bodies undergoing geodesic motion in this geometry (e.g., the Earth). Everywhere else, the solution is a vacuum solution, and that vacuum solution is what is used to predict the results of the classic solar system test experiments. (For example, nobody uses a nonzero stress-energy tensor for the Sun to predict the bending of light by the Sun; they just use the Schwarzschild geometry of the vacuum region exterior to the Sun.)
 
  • #16
PeterDonis said:
Just to clarify, this is referring to geodesic motion of bodies that are not "test bodies", because they have significant self-gravity, correct? For example, geodesic motion of the Earth in the gravitational field of the Sun.

I only meant that there are no test bodies, so although we treat the Earth in the gravitational field of the sun as a test body, we do it by assuming a solution in which matter is present, and derive the treatment of the Earth as a test body as a very good approximation.
 
  • #17
DaleSpam said:
So what? This is true of any solution of any equation. You can always simplify it to 0=0:

Given A=B
A-B=0 by subtraction
0=0 by substitution

It is a completely useless complaint because it is always true for any equation. If you over-simplify you can always get 0=0. Your query about experiments or observations with a non-vacuum metric is a valid question, but this bit about 0=0 is not.

First I like to thank to get my thread back. I know my questions are very edge of the this forum rules. I will try not to go over.

I will try to make my point by some simple examles.

One can write equation:

apples = oranges

This is true if set both apples and oranges to zero. Equation reads 0 = 0. But surely it is not true if there are nonzero items of either.

One can write equation:

polar bears = constant * pink elephants.

Assume we make some experimetal tests on Afrika. Because there is no polar bears and neither pink elephants on Afrika, we are happy that test results agree with our equation which reads 0 = 0. We know there is polar bears on north pole but we have not yet made any tests because north pole is so far away from Afrika.

Can we now say from our test results that our polar bear/pink elephant equation is correct? No we don't. We have only tested one point (0=0).
This is the reason I asked is there any experimental test results where we have EFE something else than 0 = 0.
 
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  • #18
@CycoFin, as DaleSpam and others have said, your objection makes no sense. Every equation can be written in the form U = 0, including the full Maxwell's equations with charges and currents, and Newton's laws etc. It is true that there are regimes of GR that remain untested. However, you can consider the vacuum solutions of GR analogous to Maxwell's equations without charges. Even in the absence of charge, Maxwell's equations predict interesting phenomena such as electrotromagnetic waves that travel over great distances.
 
  • #19
CycoFin said:
apples = oranges

This is true if set both apples and oranges to zero. Equation reads 0 = 0. But surely it is not true if there are nonzero items of either.

In fact, the equation can be rewritten as

apples - oranges = 0.

Also, the equation can be true if there are nonzero items of either - it means that the number of apples and oranges is the same.
 
  • #20
PeterDonis said:
No, it isn't. The EFE is a second order partial differential equation (more precisely, it's a system of 10 of them in the general case). So the RHS being zero just means it's a homogeneous second order partial differential equation, which certainly has solutions other than the trivial one. See here for an overview:

http://en.wikipedia.org/wiki/Vacuum_solution_(general_relativity)

Now I am little bit lost. You say that even we have RHS stress-energy T zero, LHS Einstein tensor G is not?

I know there are several diffrent vacuum solutions with different metrics but it does not change that in tensor point of view EFE reads 0 = 0 (these are zero tensors, not zeros)
 
  • #21
atyy said:
In fact, the equation can be rewritten as

apples - oranges = 0.

Also, the equation can be true if there are nonzero items of either - it means that the number of apples and oranges is the same.

Yes but if you make experimental tests when you never have neither apples nor oranges, you can not say if this equation is explainng nature.

All you can say that there is no apples or oranges on universe.
 
  • #22
CycoFin said:
Yes but if you make experimental tests when you never have neither apples nor oranges, you can not say if this equation is explainng nature.

All you can say that there is no apples or oranges on universe.

But the vacuum solutions correspond to the case where where apples and oranges are not each zero.
 
  • #23
Vacuum solutions makes our RHS zero. There is no energy or stress on vacuum (not talking about cosmology here now). So our oranges are zero.

Then we assume that our LHS side must be zero also. We assume apples zero. We make measurements that agrees our assumption that apples are zero.

Can we really then say that apples = oranges because they both are zero? What about changing that energy-stress tensor to pink elephant tensor. That is also zero in vacuum.

So why we don't just use apples = 0 and be happy. And add those oranges once we have tests that contain non-zero numbers of oranges (of course if our apples = oranges is still valid)
 
  • #24
CycoFin said:
Now I am little bit lost. You say that even we have RHS stress-energy T zero, LHS Einstein tensor G is not?
Of course not.
It's the metric tensor that we're solving for. The EFE supplies constraints on what this unknown metric tensor might be; one of these constraints is that the Einstein tensor calculated from the unknown metric tensor must be zero at points where the stress-energy tensor is zero. Given the complexity of the relationship between the metric and the Einstein tensors, ##G=0## is a seriously non-trivial constraint.
 
  • #25
Yes, we have G = 0, I don't disagree this and metric explanation of gravity makes sense and this have been very successfully tested.

But surely there must be some experimental test results so we can write G = constant * T, where T is nonzero energy-stress tensor.

If not, R = 0, where R is ricci tensor is enough to descripe gravity effects on vacuum.
 
  • #26
CycoFin said:
Vacuum solutions makes our RHS zero. There is no energy or stress on vacuum (not talking about cosmology here now). So our oranges are zero.

Then we assume that our LHS side must be zero also. We assume apples zero. We make measurements that agrees our assumption that apples are zero.

Can we really then say that apples = oranges because they both are zero? What about changing that energy-stress tensor to pink elephant tensor. That is also zero in vacuum.

So why we don't just use apples = 0 and be happy. And add those oranges once we have tests that contain non-zero numbers of oranges (of course if our apples = oranges is still valid)

No. The analogy is more like

apples - oranges = 0.

There the RHS is zero, but clearly, apples and oranges can both be nonzero, as long as they are equal.
 
  • #27
CycoFin said:
You say that even we have RHS stress-energy T zero, LHS Einstein tensor G is not?

No; I am saying that the Einstein tensor being zero does not mean "zero apples" or "zero oranges". It means something more like "the rate of change of the rate of changes of apples plus the rate of change of the rate of change of oranges is zero", and nine more equations of that sort. The fact that a bunch of derivatives of something add up to zero does not require that something itself to be zero. And gravity is the "something" here, so this is just saying that the Einstein tensor being zero is not the same as gravity being zero.

CycoFin said:
we have G = 0, I don't disagree this and metric explanation of gravity makes sense and this have been very successfully tested.

And these are tests of the EFE, because, once again, the LHS of the EFE is not just a simple expression whose value we test to be zero; it's a combination of a bunch of derivatives of different things, and we don't measure the combination, we measure the derivatives separately, so we can test whether they add up to zero as the EFE predicts. That's a valid test.

CycoFin said:
surely there must be some experimental test results so we can write G = constant * T, where T is nonzero energy-stress tensor.

There are, but they're indirect. The sorts of experimental tests you need here are tests of the structure of matter, but it's difficult to find pieces of matter where relativistic effects are significant in determining its structure--i.e., where the difference between the predictions of GR and the predictions of Newtonian gravity are significant. Nothing in our solar system even comes close: Newtonian gravity is sufficient to explain the internal structure of all ordinary objects, and of the Sun and all the planets and other bodies in the solar system.

The kinds of matter (other than what we model in cosmology) for which relativistic effects are significant are, basically, white dwarfs, neutron stars, black holes (these aren't exactly "matter", but they are formed from collapsing matter), and supermassive stars. There aren't any such objects nearby, so we can only observe them indirectly, from far away, hence our observational tests of GR regarding the internal structure of such objects are still very rough.

However, I don't understand why you leave out cosmology here; the cosmological models we use to accurately match many observations, such as the properties of the CMBR and the curvature in the Hubble diagram, certainly require a nonzero stress-energy tensor and are valid tests of GR with a nonzero RHS of the EFE.

atyy said:
The analogy is more like

apples - oranges = 0.

I'm not sure even this conveys it, because "apples" and "oranges" here correspond to different metric coefficients, and the EFE contains derivatives of those. See above.
 
  • #28
Is this thread what mathematicians call 'reducio ad absurdum' ?
 
  • #29
Mentz114 said:
Is this thread what mathematicians call 'reducio ad absurdum' ?

In the words of Monty Python, "That's not argument! It's just contradiction!"
 
  • #30
PeterDonis said:
And these are tests of the EFE, because, once again, the LHS of the EFE is not just a simple expression whose value we test to be zero; it's a combination of a bunch of derivatives of different things, and we don't measure the combination, we measure the derivatives separately, so we can test whether they add up to zero as the EFE predicts. That's a valid test.

These are tests of very specific form of EFE where we have RHS zero tensor. This specific vacuum EFE can also be written as Ricci tensor = 0, R = 0.
Surely Ricci tensor is made by combination of 2nd derivates of metric but that is not my point here.

We cannot use these test results to make any claim about general EFE (where RHS is not zero tensor), except obivious that general EFE is true when T = 0.
If we do that, it is like testing equation x2 = x3 only on point x = 0 (0 = 0) and then using those results to make claim that our equation is correct with every x.

PeterDonis said:
However, I don't understand why you leave out cosmology here; the cosmological models we use to accurately match many observations, such as the properties of the CMBR and the curvature in the Hubble diagram, certainly require a nonzero stress-energy tensor and are valid tests of GR with a nonzero RHS of the EFE.

I leaved cosmology out because problems we have there (dark energy, inflation, flatness problem, also dark matter but is not that much because FLRW). Because these one can start to think if we are using correct equation there.

I have some ideas how to tackle those if we accept only the vacuum EFE and dispose the general EFE but this is against forum rules and I am not going to discuss these here. Private conversation if interested to hear.
 
  • #31
Vanadium 50 said:
In the words of Monty Python, "That's not argument! It's just contradiction!"
No it isn't !

It looks like we have a crackpot so this thread is doomed. Phew.
 
  • #32
CycoFin said:
These are tests of very specific form of EFE where we have RHS zero tensor.

You're shifting your ground. Before, you were saying vacuum tests weren't tests of the EFE at all. Now you're saying they're tests, just tests of "a very specific form" of the EFE. (See below for more on that.)

CycoFin said:
We cannot use these test results to make any claim about general EFE

By this argument, you can't use any test results to make a claim about the general EFE, only about the "specific form" that you tested. You do realize that saying the RHS of the EFE is not zero does not pin down one specific "value" for the RHS, right? The RHS is the stress-energy tensor; there are many, many different forms that that tensor can take, depending on what kinds of matter and energy are present. Any test of the EFE is only going to test one "specific form" of the stress-energy tensor, corresponding to the particular kinds of matter and energy that are present during the test. A vacuum (no matter or energy present at all) is just one particular case among many.

CycoFin said:
I leaved cosmology out because problems we have there

So what? Cosmology still gives tests of the EFE, using the particular kinds of matter and energy present, on average, in the universe. And GR passes those tests for a large portion of the universe's history (basically back to times early enough that we're not sure what stress-energy tensor to use).
 
  • #33
CycoFin said:
I have some ideas how to tackle those if we accept only the vacuum EFE and dispose the general EFE

You appear to have basic misunderstandings about how the EFE is tested in the first place. We've done our best to address them in this thread, but I don't think there's much point in further discussion. This thread is closed.
 

1. What is EFE and how does it relate to general relativity?

EFE stands for Einstein's field equations, which are a set of equations that describe the relationship between the curvature of spacetime and the distribution of matter and energy. These equations are the cornerstone of general relativity, which is a theory of gravity that explains how massive objects interact with each other.

2. What are the tests of EFE and why are they important?

The tests of EFE are experiments and observations that aim to verify the predictions of general relativity and assess its validity. These tests are important because they allow us to confirm or reject the theory and potentially uncover new physics that may challenge our current understanding of gravity.

3. What are some examples of tests of EFE?

Examples of tests of EFE include the gravitational redshift, which measures the change in frequency of light as it travels through a gravitational field, and the deflection of light, which measures how much the path of light is bent by a massive object. Other tests include the precession of Mercury's orbit and the Shapiro time delay.

4. How have tests of EFE been conducted?

Tests of EFE have been conducted through various methods, including astronomical observations, laboratory experiments, and space missions. For example, the Gravity Probe B mission used gyroscopes to measure the frame-dragging effect predicted by general relativity, while the Laser Interferometer Gravitational-Wave Observatory (LIGO) detected gravitational waves, providing strong evidence for the theory.

5. What are the implications of successfully passing tests of EFE?

If general relativity passes all tests of EFE, it would further validate the theory and solidify our understanding of gravity. It would also have significant implications for our understanding of the universe, as it is the basis for many cosmological models and our understanding of the evolution of the universe.

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