Three questions related to the principle of general covariance in GR

In summary: But then we realize that the derivative of the metric with respect to itself is zero, so we can solve for the Lagrangian in terms of the metric and its derivative with respect to the other fields. 3. ... and the toughest one: Above, when formulating the equivalence principle, I used the wording "at each point of the general-relativity manifold". Is this wording at all legitimate? I mean: is it right to assume that each point of the manifold is a physical event? I am asking, because
  • #1
Michael_1812
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1. A (presumably) simple question:

We are used to think that the affine connections emerge whenever one wants to
differentiate a vector (tensor, spinor) on a curved manifold in general relativity. Now suppose that we are still on a flat background of special relativity, though in a curvilinear grid. Will the connections show up there?

2. Now comes a tougher one:

According to the (weak) equivalence principle, at each point of the general-relativity manifold there exists a reference frame (the freely falling one) wherein the motions are the same as in an inertial frame of the special relativity.

According to the principle of general covariance, all the fundamental laws of physics stay form-invariant under a transition between any two coordinate charts (provided the derivatives in these laws are covariant and are taken with respect to a true scalar - the interval). Stated alternatively, the fundamental laws can be expressed in a coordinate-independent way.

How do these two fundamental principles square?

I think it was Weinberg's book where I saw a sentence saying that the principle of general
covariance is a mathematical implementation of the equivalence principle. Why is that??

3. ... and the toughest one:

Above, when formulating the equivalence principle, I used the wording "at each point of the general-relativity manifold". Is this wording at all legitimate? I mean: is it right to assume that each point of the manifold is a physical event? I am asking, because we have gauge invariance, so it may happen that a whole orbit corresponds to one and the same event.
Please correct me if I am wrong.

Many thanks for your time and help,
Michael
 
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  • #2
Michael_1812 said:
1. A (presumably) simple question:

We are used to think that the affine connections emerge whenever one wants to
differentiate a vector (tensor, spinor) on a curved manifold in general relativity. Now suppose that we are still on a flat background of special relativity, though in a curvilinear grid. Will the connections show up there?

Yes. And they even show up in Galilean/Newtonian mechanics in curvilinear coordinates.

Sorry for not getting back to you. I kept putting this off in the hope of writing a more detailed answer than I give above.
 
  • #3
Michael_1812 said:
2. Now comes a tougher one:

According to the (weak) equivalence principle, at each point of the general-relativity manifold there exists a reference frame (the freely falling one) wherein the motions are the same as in an inertial frame of the special relativity.

According to the principle of general covariance, all the fundamental laws of physics stay form-invariant under a transition between any two coordinate charts (provided the derivatives in these laws are covariant and are taken with respect to a true scalar - the interval). Stated alternatively, the fundamental laws can be expressed in a coordinate-independent way.

How do these two fundamental principles square?

I think it was Weinberg's book where I saw a sentence says that the principle of general
covariance is a mathematical implementation of the equivalence principle. Why is that??

I believe Weinberg does say GC=EP BUT he does not define GC as you do, and says that GC as normally defined is physically empty. (But check his book to be sure.)

I think it's something like:
GC (as normally defined, not Weinberg's def) is physically empty.
EP implies gravity can be geometrically formulated, but does not lead uniquely to GR - see eg. Newton-Cartan theory or Nordstrom's second theory.
GR requires one more principle: "no prior geometry" (MTW).
And GR in full form does not have particles traveling on geodesics - it's a field with "metric" symmetry, whose equations of motion are derived from a Lagrangian, and matter is just other fields, which are also derived from a Lagrangian.

Edit: In addition to "no prior geometry", GR also requires an assumption about the highest order derivative that enters the field equations.
 
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  • #4
Michael_1812 said:
Above, when formulating the equivalence principle, I used the wording "at each point of the general-relativity manifold". Is this wording at all legitimate? I mean: is it right to assume that each point of the manifold is a physical event? I am asking, because we have gauge invariance, so it may happen that a whole orbit corresponds to one and the same event.
Please correct me if I am wrong.

It's legitimate. Strictly speaking, you should say isometry equivalence class of manifolds and metrics or something like that, but it's taken for granted you can just make true statements about one member of the equivalence class. See eg. Ellis & Hawking p56.
 
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  • #5
atyy said:
Edit: In addition to "no prior geometry", GR also requires an assumption about the highest order derivative that enters the field equations.

Sean Carroll's http://nedwww.ipac.caltech.edu/level5/March01/Carroll3/Carroll4.html gives more detail. A quick summary of the essential points. Suppose we already decided from the EP that the "metric" should become a field that models gravity. Then we should presumably seek a Lagrangian whose terms contain the metric. Because the Lagrangian is a scalar, a further restriction on these terms is that they should be scalars. This allows Lagrangians such as Eq 4.76. To obtain the Hilbert action 4.55, a further restriction is made to include only terms containing up to 2 derivatives of the metric.

Also useful:
Luca Bombelli, http://www.phy.olemiss.edu/~luca/Topics/grav/higher_order.html .
Donoghue, http://arxiv.org/abs/gr-qc/9512024, especially Eq 21.
 
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  • #6
Hmmm, I didn't realize that there are many subtleties about the relationship between metric theories of gravity and the equivalence principle:

http://arxiv.org/abs/0707.2748
Theory of gravitation theories: a no-progress report
Thomas P Sotiriou, Valerio Faraoni, Stefano Liberati
 
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  • #7
particles (not??) following geodesics

Dear atyy,
Thank you for answering my questions.
You say: "And GR in full form does not have particles traveling on geodesics..."
What do you mean by this? How can a free particle deviate from its geodesic?
(Or did you imply that particles were interacting with fields other than gravity?)
Many thanks,
Michael
 
  • #8
The Bianchi identity as a reincarnation of the momentum-conservation law

Guys,

Can anyone explain to me in simple words (i.e., without referring to forms on the frame bundle, etc) why the Bianchi identity is the relativistic generalisation of the momentum-conservation law?

Here comes my hypothesis, but I am not 100% convinced that it is correct. In Newtonian mechanics, we used to get momentum (and energy) conservation from the action's invariance under infinitesimal spatial and time displacements. In the GR, the Hilbert action stays stationary under gauge-like changes of the metric, i.e., under infinitesimal displacements of the coordinates. Variation of the Hilbert action with respect to these entails:

G^{\mu\nu}_{ ; \nu} = 0 .

To get this, repeat verbatim eqns (94.5 - 94.7) in Landau & Lifgarbagez, with the Lagrangian changed to R,
and with T_{\mu\nu} changed to G_{\mu\nu}.

[Had we varied the Hilbert action with respect to NONgauge variations of the metric, we would have arrived to the equations of motion G^{\mu\nu} = 0. The difference stems from the fact that the NONgauge variations of the metric are all independent, up to symmetry. The gauge variations are dependent and, thus, must be expressed via the coordinate shifts, like in section 94 of Landau & Lifgarbagez.]

Now, G^{\mu\nu}_{ ; \nu} = 0 is equivalent to:

R^{\mu\nu}_{ ; \nu} = 0 ,

which, in its turn, is identical to Bianchi. (Well, it follows from Bianchi, but I guess they are just identical.)

This line of reasoning seems to show that Bianchi (or, to be more exact, its corollary R^{\mu\nu}_{ ; \nu} = 0) is the relativistic analogue to momentum conservation.

Is that true? Can this conclusion be achieved by less cumbersome means?

Learning the math sometimes is easier than grasping the physics beneath it...

Great many thanks,
Michael
 
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  • #9
This thread is three months old and on a different topic. Your new question is one I'd be interested in hearing people's thoughts on, but I think you should really start a new thread for it rather than posting it in this old thread.
 
  • #10
which of my two questions do you have in mind - geodesics or Bianchi?
 
  • #11
Michael_1812 said:
which of my two questions do you have in mind - geodesics or Bianchi?

Bianchi was the one I was interested in.
 
  • #12
I have re-posted the latter two questions as new threads
 

FAQ: Three questions related to the principle of general covariance in GR

1. What is the principle of general covariance in General Relativity (GR)?

The principle of general covariance is a fundamental principle in GR, which states that the laws of physics should be the same for all observers, regardless of their reference frame or motion. This means that the laws of physics should be expressed in a way that is independent of the specific coordinate system used to describe them.

2. Why is the principle of general covariance important in GR?

The principle of general covariance is important because it allows for the formulation of a theory of gravity that is consistent with the principles of special relativity, which states that the laws of physics should be the same for all observers in inertial frames of reference. This allows GR to explain the effects of gravity in a way that is consistent with our current understanding of the laws of physics.

3. How does the principle of general covariance affect the equations of GR?

The principle of general covariance requires that the equations of GR be expressed in a way that is independent of the specific coordinate system used. This is achieved through the use of tensor calculus, which allows for the formulation of equations that are invariant under coordinate transformations. This ensures that the equations remain valid for all observers, regardless of their reference frame or motion.

4. Is the principle of general covariance unique to GR?

No, the principle of general covariance is not unique to GR. It is a fundamental principle in the theory of relativity and is also applied in other areas of physics, such as quantum field theory. However, it plays a crucial role in GR, as it allows for the consistent incorporation of gravity into the framework of special relativity.

5. Are there any experimental tests of the principle of general covariance?

Yes, there have been several experimental tests of the principle of general covariance. One notable example is the observation of gravitational lensing, which is a direct consequence of the principle of general covariance in GR. Additionally, the predictions of GR have been extensively tested and verified through various experiments, providing further evidence for the validity of the principle of general covariance.

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