Equation for acceleration in MTW

In summary, the equation MTW is trying to make between the two equations is that the geodesic deviation in an electromagnetic field is a quadrupole shear due to the electric and magnetic components of the Riemann tensor.
  • #1
jfy4
649
3
Hi,

In MTW, there is a box (3.1) where certain equations for acceleration are used as a model for determining the components of the curvature tensor. the equations are

[tex]\frac{d^2x^a}{d\tau^2}=\frac{e}{m}F^{a}_{b}u^b[/tex]

and

[tex] \frac{d^2\xi^a}{d\tau^2}=-R^{a}_{bcd}u^b\xi^cu^d[/tex]

However, I was under the impression that the latter equation was the equation for geodesic deviation, and that the first equation was the equation of motion for E&M.

What's the relationship MTW is trying to make between these two?
 
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  • #2
Hi Judah! :smile:

I don't have a copy of MTW, but the equation I've seen elsewhere for geodesic deviation in an electromagnetic field is

[tex]\frac{D^2\,\delta x^{\alpha}}{D\tau^2}\ =\ \frac{q}{m}\,F^{\alpha}_{\ \mu\,;\,\beta}\,V^{\mu}\,\delta x^{\beta}[/tex]

(where δxα is the gap between two world-lines).
 
  • #3
MTW is trying to draw a parallel (a rather vague parallel!) between the effect of a gravitational field vs an electromagnetic field, and at the same time give an operational significance to the Riemann tensor. While the electromagnetic field produces an acceleration on a charged particle, the gravitational field produces instead a differential acceleration on a cloud of neighboring particles. In more detail, the structure of the second equation shows that in the rest frame of the particles it is the 'electric' components of the Riemann tensor, Ra0c0, that do this, and that the effect is a quadrupole shear.
 
  • #4
Bill_K said:
MTW is trying to draw a parallel (a rather vague parallel!) between the effect of a gravitational field vs an electromagnetic field, and at the same time give an operational significance to the Riemann tensor. While the electromagnetic field produces an acceleration on a charged particle, the gravitational field produces instead a differential acceleration on a cloud of neighboring particles. In more detail, the structure of the second equation shows that in the rest frame of the particles it is the 'electric' components of the Riemann tensor, Ra0c0, that do this, and that the effect is a quadrupole shear.

Thanks,

To try and get a handle on what it means to call those components the "electric" parts, let me try something here. I have here from one of my reference books Exact Solutions to Einstein's Field Equations by Stephani et al... a relationship between the Weyl Conformal tensor (which is a component of the Riemann curvature tensor) and it's "electric" and "magnetic" parts.

[tex]C^{\ast}_{abcd}u^bu^d=E_{ac}+iB_{ac}[/tex]

where

[tex]u_bu^b=-1[/tex]

and

[tex]C^{\ast}_{abcd}=C_{abcd}+iC^{\sim}_{abcd}[/tex]

where

[tex]C^{\sim}_{abcd}=\frac{1}{2}\varepsilon_{cdef}C_{ab}{}^{ef}[/tex]

Is it ok to draw a parallel between these two (the Riemann and Weyl) tensors and their "electric" and "magnetic" parts?

EDIT:
That is, can I identify these corresponding parts (analogously from the Weyl tensor)?

[tex]R_{abcd}u^bu^d=E_{ac}[/tex]

and

[tex]\frac{1}{2}R_{ab}{}^{ef}\varepsilon_{cdef}u^bu^d=B_{ac}[/tex]
 
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  • #5
Try writing Cabcd in terms of Rabcd and plugging that into the expressions for the Weyl E and B.

Somewhere you'll find a formula like

Rabcd = Cabcd - Xabcd/2 - R/6 Yabcd

where X is a function of the Ricci tensor and Y of the metric.

The answer should be easiest to get in the case where Rab=0.
 
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  • #6
Mentz114 said:
Try writing Cabcd in terms of Rabcd and plugging that into the expressions for the Weyl E and B.

Somewhere you'll find a formula like

Rabcd = Cabcd - Xabcd/2 - R/6 Yabcd

where X is a function of the Ricci tensor and Y of the metric.

The answer should be easiest to get in the case where Rab=0.

I have

[tex]C_{abcd}=R_{abcd}-N_{abcd}-G_{abcd}[/tex]

where [itex]R_{abcd}[/itex] is the Riemann curvature tensor,

[tex]N_{abcd}=\frac{1}{2}(g_{ac}S_{bd}+g_{bd}S_{ac}-g_{ad}S_{bc}-g_{bc}S_{ad})[/tex]

and

[tex]G_{abcd}=\frac{1}{12}\mathcal{R}(g_{ac}g_{bd}-g_{ad}g_{bc})=\frac{1}{12}\mathcal{R}\,g_{abcd}[/tex]

where

[tex]S_{ab}=R_{ab}-\frac{1}{4}\mathcal{R}\, g_{ab}[/tex]

where [itex]\mathcal{R}[/itex] is the Curvature scalar and [itex]R_{ab}[/itex] is the Ricci tensor.

Then when I insert this into the electric and magnetic relation I have three tensors responsible for the electric and magnetic parts, not just the Riemann tensor, which is what I want to know. Currently I have

[tex](R_{abcd}-N_{abcd}-G_{abcd})u^bu^d=E_{ac}[/tex]

and

[tex]\frac{1}{2}\epsilon_{cdef}(R_{ab}^{\;\;\;ef}-N_{ab}^{\;\;\;ef}-G_{ab}^{\;\;\;ef})u^bu^d=B_{ac}[/tex]

If there is a way to get the electric and magnetic components solely in terms of the Riemann tensor, I need a little push forward.
 
  • #7
I might not be understanding the question, but what you've now got is the E and B parts of the Weyl tensor in terms of the Riemann tensor and its contractions.

I thought that was what you wanted.:smile:
 
  • #8
Mentz114 said:
I might not be understanding the question, but what you've now got is the E and B parts of the Weyl tensor in terms of the Riemann tensor and its contractions.

I thought that was what you wanted.:smile:

Almost! as you said, I have the E and B parts of the Weyl tensor, I want the E and B parts of the Riemann tensor. I was asking earlier if in fact it was what I had posted

[tex]R_{\alpha\beta\gamma\delta}u^\beta u^\delta=E_{\alpha\gamma}[/tex]

and

[tex]
\frac{1}{2}R_{\alpha\beta}{}^{\epsilon\zeta}\varepsilon_{\gamma\delta\epsilon\zeta}u^\beta u^\delta=B _{\alpha\gamma}
[/tex]

where [itex]u^{\alpha}[/itex] is a time-like vector.
 

FAQ: Equation for acceleration in MTW

What is the formula for acceleration in MTW?

The equation for acceleration in MTW (Minkowski, Taylor, and Wheeler) is a = (vf - vi)/t, where a represents acceleration, vf represents final velocity, vi represents initial velocity, and t represents time.

How is the MTW equation for acceleration different from the traditional equation?

The MTW equation for acceleration is different from the traditional equation (a = (vf - vi)/t) because it takes into account the concept of spacetime, as described in Einstein's theory of relativity. This equation is used in special relativity to calculate acceleration in a four-dimensional spacetime.

Can the MTW equation for acceleration be used in all situations?

No, the MTW equation for acceleration is only applicable in situations where relativistic effects must be taken into account. In everyday situations on Earth, the traditional equation for acceleration (a = (vf - vi)/t) is sufficient.

How does the MTW equation for acceleration relate to the concept of spacetime curvature?

The MTW equation for acceleration is closely related to the concept of spacetime curvature, which is a fundamental aspect of Einstein's theory of general relativity. In this equation, acceleration is affected by the curvature of spacetime caused by massive objects, such as planets and stars.

Can the MTW equation for acceleration be derived from other fundamental equations?

Yes, the MTW equation for acceleration can be derived from other fundamental equations, such as the principle of equivalence and the Lorentz transformation. These equations are the basis for understanding spacetime and relativistic effects, which are essential in deriving the equation for acceleration in MTW.

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