Deriving the Schwarzschild metric just by using the equivalence principle

In summary, according to this paper, Lorentz transformations can be used in frames that are in constant linear acceleration, but they should be done in the same form as they are locally in SR.
  • #1
Huashan
7
0
I've read a few papers about derivation of the Schwarzschild metric by using the equivalence principle ( http://cdsweb.cern.ch/record/1000100/files/0611104.pdf" )... but I couldn't understand them completely

they assume , According to Einstein’s equivalence principle, that the influence of gravitation on phenomena in a local reference frame that is at rest in the field is equivalent to the influence of the accelerated motion of a local reference frame in which phenomena are described in the absence of gravitation . ( till now there is no problem ).

and then for such an accelerated frame they write the metric in the form :
03.JPG


(no problem yet ).

then... they relate the local coordinates x’, t’ in the accelerated frame to the corresponding coordinates in the stationary frame by the usual differential form of the Lorentz transformation for the value of the velocity that has been reached , by the formulae :

04.JPG


here is the problem ... can these frames be related to each other by the above expressions ?? According to the fact that one of them is non-inertial frame? ... the derivation of the above expressions are based on the fact that the frames are inertial and moving with respect to each other with a constant velocity v .

Can anybody help me?? ...
 
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  • #2
I don't think it can be done, since many metrics (and many theories, not just general relativity) are consistent with some sort of equivalence principle.
 
  • #3
atyy said:
I don't think it can be done, since many metrics (and many theories, not just general relativity) are consistent with some sort of equivalence principle.

yes I know ... my question is whether we can use Lorentz transformations (in the same form as they are locally in SR ) in constant-linear-acceleration frames or nor ?, if yes how ?...
 
  • #4
Along atyy's comments, I've heard that Nordstrom's theory of gravity satisfies the strong equivalence princple. I searched and found a paper that made this claim in passing, but couldn't find any that had a good discussion on this. Can anyone comment if this is true about Nordstrom's theory?

This sounds a bit over-stating the case, but wikipedia claims:
"All metric theories satisfy the Einstein equivalence principle"
http://en.wikipedia.org/wiki/Brans-Dicke_theory
Is that really true? Then is the only issue whether a metric theory satisfies the strong equivalence princple?
 
  • #5
Huashan said:
yes I know ... my question is whether we can use Lorentz transformations (in the same form as they are locally in SR ) in constant-linear-acceleration frames or nor ?, if yes how ?...
You can always locally make the metric match that of flat spacetime. And then yes, the lorentz transformations apply locally at least. I think it is valid only in that sense.
 
  • #6
my question is whether we can use Lorentz transformations (in the same form as they are locally in SR ) in constant-linear-acceleration frames or nor ?
Maybe one should mention that the author does not use Lorentz transformations, but timae dilation and length contraction applied to basic vectors, which is wrong.
Lorentz transformations leave all intervals (the metric) unchanged. That's more or less how they are defined.
This paper is cranky, not surprising as the author is a philosopher.
 
  • #7
Huashan, a reliable source you may want to look at for additional perspective on this is Taylor & Wheeler's excellent textbook "Black Holes." In Query 3 on p B-7 and on p B-13 they combine a Lorentz transformation with the Schwarzschild metric to create a metric for an object in radial freefall from infinity toward a black hole, which they refer to as the "rain frame."

This metric demonstrates that in the frame of the falling object, the local space is flat regardless of the spacetime curvature. They credit this metric to Charles Misner, who in turn derived it from Painleve & Gullstrand.

The Painleve-Gullstrand metric for the "river model" described in the Czerniawski paper you cite certainly is a widely accepted and quite interesting variation on the Schwarzschild metric.

Taylor & Wheeler reference a paper providing formal derivations and references:http://arxiv.org/abs/gr-qc/0001069" by Martel and Poisson, AJP 69-4, 2001, p. 476-480.

Peacock also combines a relativistic Doppler shift and a gravitational shift to derive a formula for the cosmological redshift in Schwarzschild coordinates, in his http://arxiv.org/abs/0809.4573" , eq. 16. This equation produces demonstrably correct calculations.

There probably are many other reliable examples to be found where equations using Lorentz transformations are applied in the context of the Schwarzschild metric. Conceptually I see nothing wrong with doing so, as long as one is careful.
 
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Related to Deriving the Schwarzschild metric just by using the equivalence principle

1. What is the Schwarzschild metric?

The Schwarzschild metric is a mathematical description of the curvature of space-time around a non-rotating, spherically symmetric massive object, such as a black hole. It is a key component of Einstein's theory of general relativity.

2. What is the equivalence principle?

The equivalence principle is a fundamental concept in physics that states that the effects of gravity are indistinguishable from the effects of acceleration. This means that an observer in a uniform gravitational field would not be able to tell the difference between being at rest in that field or accelerating in the absence of gravity.

3. How does the equivalence principle relate to the Schwarzschild metric?

The equivalence principle is the basis for deriving the Schwarzschild metric. By assuming that the effects of gravity are equivalent to those of acceleration, Einstein was able to develop the mathematical framework for general relativity and derive the equations that describe the curvature of space-time around massive objects.

4. Can the Schwarzschild metric be derived using other methods?

Yes, the Schwarzschild metric can also be derived using other approaches, such as the Einstein field equations or the geodesic equation. However, the derivation using the equivalence principle is considered to be the most intuitive and fundamental method.

5. What are some implications of the Schwarzschild metric?

The Schwarzschild metric has many important implications in physics, including the prediction of the existence of black holes and the behavior of light near massive objects. It also plays a crucial role in our understanding of the structure and evolution of the universe, as well as in the study of gravitational waves and other phenomena related to general relativity.

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