humanino said:
Why do you introduce the dinstiction between Energy and Proper energy whereas it is irrelevant to the the Photon ?
It was you who commented on the applicability of the relation E = mc
2. I pointed out that relation is E
0 = mc
2 and, assuming m = proper mass, holds only for proper energy. I.e. you omitted the subscript denoting proper energy.
What kind of gravitational field could have a vanishing Riemann tensor and a non-vanishing affine connection ?
Any gravitational field with no tidal forces, E.g. a uniform gravitational field. The metric of a uniform gravitational field is
ds^2 = c^2(1+gz/c^2)^2dt^2 - dx^2 - dy^2 - dz^2
The Christoffel symbols are calculated at -
http://www.geocities.com/physics_world/uniform_chris.htm. The only non-vanishing Christoffel symbols are
\Gamma ^0_{03} = \frac {g}{c^2}\frac{1}{1 + gz/c^2}
\Gamma ^3_{00} = -\frac {g}{c^2}\frac{1}{1 + gz/c^2}
where g = gravitational acceleration at z = 0. According to the equivalence principle a uniform gravitational field is equivalent to a uniformly accelerating frame of reference in flat spacetime. One can obtain the metric for the uniform g-field by transforming from an inertial frame in flat spacetime to a uniformly accelerating frame of reference. The Christoffel symbols will change from zero to the above values but the Riemann tensor will remain zero as it must (i.e. if a tensor vanishes in one coordinate system then it vanishes in all coordinate systems). The uniform gravitational field was the very first gravitational field that Einstein considered in his theory of general relativity. In fact one form of the equivalence principle is stated as follows
Einstein's Equivalence Principle: A uniform gravitational field is equivalent to a uniformly accelerating frame of reference.
A few examples of a gravitational field with zero spacetime curvature from the general relativity/cosmology literature are the gravitational field of a vacuum domain wall and a straight cosmic string. E.g. see
Gravitational Field of Vacuum Domain Walls, Alexander Vilenkin, Phys. Lett. 133B, page 177-179
Gravitational field of vacuum domain walls and strings, Alexander Vilenkin, Phys. Rev. D, Vol 23(4), (1981), page 852-857
Cosmic strings: Gravitation without local curvature, T. M. Helliwell, D. A. Konkowski, Am. J. Phys. 55(5), May 1987, page 401-407
(Note: The author of the Ma. J. Phys. article uses the term "local curvature" in the title of this paper but he is referring to
Riemann = 0)
The action for the gravitational is determined by the integral of the curvature : if the curvature is zero, there is non action, no Gravitational field ! Where am I wrong ?!
What does the action have to do with gravitational acceleration?
The view proposed in this paper are supposed to be Einstein's one, with opposition to other physisicists such as : Hawking and Thorne.
It is a fact that Hawking and Thorne are in opposition to Einstein on this point. But then again they're in opposition to other GRist such as Tolman too.
In any case this is not about what Hawking and Thorne think. Its about what Einstein thought. You haven't supported your claim that Einstein associtated the non-vanishing of the gravitational field with the non-vanishing of the Riemann tensor. Would you care to support your claim?
Its funny that you should mention Thorne since it was Thorne who pointed out to me that the Riemman tensor for a uniform gravitational field is zero. In fact he was the one who sent me the references to the paper by Vilinken for the domain wall which also has zero spacetime curvature (in the region of the gravitational field outside the wall itself). When I asked him about this and his position on gravity = curavture he simply told me that it all depends on how you define gravity.
And is also not in opposition to the GR historian/GR expert Dr. John Stachel, Boston University, former head of the Einstein Papers project. His paper is referenced in that article. Did you even read the paper you're now complaining about? It was intented to explain all the details of why I said this since its too long to get into in detail in a forum.
Try reading
The Foundation of the General Theory of Relativity, A. Einstein, Annalen der Physik, 1916 and/or
The Meaning of Relativity, A. Einstein, Princeton University Press.
It's pretty clear what Einstein meant when he wrote in a letter to Max von Laue (Einstein to Max von Laue, September 1950)
... what characterizes the existence of a gravitational field from the empirical standpoint is the non-vanishing of the components of the [affine connection], not the vanishing of the [components of the Riemann tensor]. If one does not think in such intuitive (anschaulich) ways, one cannot grasp why something like curvature should have anything at all to do with gravitation. In any case, no rational person would have hit upon anything otherwise. The key to the understanding of the equality of gravitational mass and inertial mass would have been missing.
That comment cannot be taken in any other way.
But if you want more on this then all you need to do is go to the library and read
How Einstein Discovered General Relativity: A Historical Tale With Some Contemporary Morals, J.J. Stachel, General Relativity and Gravitation, Proceedings of the 11th International Conference on General Relativity and Gravitation, (Stockholm,Cambridge University Press, Jul 6-12, 1986). As Stachel writes on page 202
Within a few year years, Lavi-Civita, Weyl and Cartan generalized the Christoffel symbols to the concept of affine connection. This concept served to make the relationship between the mathematical representations of various concepts much clearer. Just because it is not a tensor field, the connection field provides adequate representation of the gravitational-cum-inertial field required by Einstein's equivalence principle. There is no (unique) decomposition of the connection field into an inertial plus gravitational tesor.
Since Stachel is probably the world's leading authority on the history of general relativity, as well as being a noted GRist as well, I'm very comforatable with everything I've explained.
In any case this is all written in Einstein's work. All one has to do is pick it up and read it. Why would you think otherwise? On what basis do you hold that the Riemann tensor must vanish when there is no gravitational field?
A uniform gravitational field is defined as a gravitational field with no spacetime curvature. For this definition and a derivation of the metric based on this definition please also see
Principle of Equivalence, F. Rohrlich, Ann. Phys. 22, 169-191, (1963), page 173.
Pete