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Newtonian force as a covariant or contravariant quantity |
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| Jan30-13, 07:23 PM | #103 |
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Newtonian force as a covariant or contravariant quantity
While searching for information relative to this thread, I stumbled across this on Google Books (Richard A Mould, Basic Relativity, p.258). It claims that, under some circumstances, "covariant energy" (time component of covariant 4-momentum) is globally conserved, but "contravariant energy" (time component of contravariant 4-momentum) is conserved only locally but not globally. Unfortunately the next page is missing from the preview, so it's not clear what the "some circumstances" actually are, or how you prove the claim.
Does anyone know what is the correct statement and its proof? Well, in the case of Rindler coordinates [tex] ds^2 = g^2 z^2 \, dt^2 - dx^2 - dy^2 -dz^2 [/tex](c=1) the contravariant 4-momentum of a particle at rest is [tex] P^\alpha = \begin{bmatrix} \frac{m}{gz} \\ 0 \\ 0 \\ 0 \end{bmatrix} [/tex]whereas the covariant 4-momentum is [tex] P_\alpha = \begin{bmatrix} mgz && 0 && 0 && 0 \end{bmatrix} [/tex]Of course [itex]mgz[/itex] is the correct formula for "gravitational" potential energy in Rindler coordinates, whereas [itex]m/(gz)[/itex] has no significance that I know of. Another non-relativistic example I can think of is cylindrical polar coordinates in Euclidean 3-space [tex] ds^2 = dr^2 + r^2 \, d\theta^2 + dz^2 [/tex]For an arbitrary particle [tex] x^i = \left( r(t), \theta(t), z(t) \right) [/tex]we have a contravariant 3-momentum [tex] p^i = \begin{bmatrix} m \dot{r} \\ m \dot{\theta} \\ m \dot{z} \end{bmatrix} [/tex]whereas the covariant 3-momentum is [tex] p_i = \begin{bmatrix} m \dot{r} && m r^2 \dot{\theta} && m \dot{z} \end{bmatrix} [/tex]Here again we see that the covariant component [itex]m r^2 \dot{\theta}[/itex] is the conserved angular momentum, whereas the contravariant component [itex]m \dot{\theta}[/itex] is not conserved. So all of the above seems to be more evidence to suggest that momentum and its time-derivative, force, are naturally covariant rather than contravariant. |
| Jan30-13, 07:37 PM | #104 |
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Is the statement that the 0 component of contravariant 4 - momentum is NEVER globally conserved and can only ever be locally conserved whereas the 0 component of covariant 4 - momentum CAN be globally conserved under the appropriate conditions?
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| Jan30-13, 09:44 PM | #105 |
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Here's another thing I have to try to wrap my head around: I think Killing vectors are naturally lower-index vectors, and even though you do have a metric, it doesn't make sense to try to raise their indices. The reason is that the Killing vector is a field, not just a vector defined at a point, and the metric is varying...Does that make sense!? |
| Jan30-13, 11:54 PM | #106 |
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Recognitions:
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| Jan31-13, 12:02 AM | #107 |
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| Jan31-13, 06:38 AM | #108 |
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[itex]g(\nabla_Y (X),Z) + g(Y , \nabla_Z (X)) = 0[/itex] which is an equation on vector fields [itex]X^\mu[/itex]. However, it also says that in "local coordinates", this is equivalent to [itex]\nabla_\mu X_\nu + \nabla_\nu X_\mu = 0[/itex] which is an equation on covector fields [itex]X_\mu[/itex]. I don't quite understand this, because it seems that the latter equation doesn't even involve the metric (except indirectly, through the covariant derivative). It would seem to me that the latter could be defined even for a manifold without a metric, with just a connection, as a definition of a Killing co-vector field [itex]X_\mu[/itex]. |
| Jan31-13, 06:55 AM | #109 |
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| Jan31-13, 07:21 AM | #110 |
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| Jan31-13, 07:27 AM | #111 |
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Why the insistence on what is natural for a certain field when examples keep popping up that contradict any abstract "naturalness" in the presence of a metric of the covariance or contravariance of (co)vector fields? |
| Jan31-13, 07:50 AM | #112 |
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| Jan31-13, 10:11 AM | #113 |
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Trying to clear up my foggy thinking re Killing vectors...
The Killing equation [itex]\nabla_a \xi_b+\nabla_b \xi_a=0[/itex] does use the metric, because the covariant derivative is defined in terms of the metric. Likewise if you define Killing vectors in terms of preserving distances, you're still appealing to a metric. On a bare manifold without a connection, there is no way to define a Killing vector. For instance, if I take the spacetime in and around the planet earth, it has Killing vectors such as rotation and time translation. If I take away the metrical information, then all I have is a topological space that's topologically isomorphic to R^3, and there's no way to say what its Killing vectors are. You can raise the indices like this [itex]\nabla^a \xi^b+\nabla^b \xi^a=0[/itex]. Note how the structure of the equation forces you to raise the indices on the derivatives as well as the Killing vector. If we're thinking of derivatives as being "naturally" lower-index quantities, then this does provide some motivation for saying that Killing vectos are naturally lower-index. But the fact that this is a *covariant* derivative means that you must have a metric defined, and therefore there's nothing to stop you from raising its index. This is different from the case of a plain old partial derivative. People normally express Killing vectors using partial derivatives as a basis, e.g., [itex]\partial_t[/itex] for a metric that doesn't change over time. So if there is a "natural" way to write them, it would definitely have to be lower-index. On the other hand, it would also seem extremely natural to me to express the same symmetry as a translation of the time coordinate, [itex]x^t \rightarrow x^t+dt[/itex]. When you have a Killing vector [itex]\xi_a[/itex], test particles follow trajectories that conserve [itex]\xi_a v^a[/itex]. This seems odd to me because we normally think of momentum as being what's conserved, not velocity. We can multiply by m to get a momentum, but then it would be an upper-index momentum, which is not the natural way to express momentum. I would like to connect this to DrGreg's #103, which wasn't explicitly written in terms of a discussion of Killing vectors. |
| Jan31-13, 10:15 AM | #114 |
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| Jan31-13, 11:21 AM | #115 |
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| Jan31-13, 11:42 AM | #116 |
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| Jan31-13, 12:10 PM | #117 |
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| Jan31-13, 12:11 PM | #118 |
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| Jan31-13, 12:12 PM | #119 |
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