How to Study Fermi-Walker Transport in Minkowski Spacetime

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Discussion Overview

The discussion revolves around the study of Fermi-Walker transport in Minkowski spacetime, focusing on its implications, definitions, and comparisons with parallel transport along geodesics and non-geodesics. Participants explore theoretical aspects, mathematical formulations, and conceptual clarifications related to the topic.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested
  • Mathematical reasoning

Main Points Raised

  • Some participants discuss the limitations of parallel transport along non-geodesics, suggesting that the timelike tangent of a worldline is not parallel transported along such paths.
  • There is a proposal that Fermi-Walker transport requires at least three dimensions to clarify the concept of "non-rotating," while others argue that it can be demonstrated in two dimensions using the Rindler case.
  • Participants explore the relationship between acceleration, velocity, and the orthogonality of vectors in the context of Fermi-Walker transport.
  • One participant presents a detailed mathematical derivation of Fermi-Walker transport, discussing the implications of rotation-free transformations and the concept of Wigner rotation.
  • Clarifications are made regarding the applicability of covariant derivatives and whether Fermi-Walker transport is limited to vector fields or can also apply to individual vectors along a curve.
  • There is a discussion about the relationship between parallel transport and Lie transport along curves defined by Killing vector fields.

Areas of Agreement / Disagreement

Participants express differing views on the dimensional requirements for demonstrating Fermi-Walker transport and the nature of parallel transport along non-geodesics. The discussion remains unresolved regarding the best approach to illustrate these concepts and the implications of various mathematical formulations.

Contextual Notes

Some limitations are noted, such as the dependence on definitions of rotation and the mathematical complexity involved in transitioning from Riemannian to Lorentzian metrics. The discussion also highlights unresolved questions about the nature of vector fields and their transport along curves.

  • #31
Sorry, I have some problem to grasp how you get the two non-trivial equations:

$$
\dot X^x = X^x \partial_x V^x + X^y \partial_y V^x = - \omega X^y, \qquad
\dot X^y = \omega X^x
$$
The LHS for each of the above equations should be ##(\mathcal L_V X)^a = [V,X]^a = \dot X^a - X^b \partial_b V^a = 0## evaluated for index ##a=x## and ##a=y## respectively. What about the respective RHS terms, namely ##- \omega X^y## and ##\omega X^x## ?

Thank you.

Orodruin said:
While this is true, it is not very satisfying as it makes it appear as if the Lie derivative depends on the connection. It does not.
Yes, you are definitely right.
 
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  • #32
cianfa72 said:
The LHS for each of the above equations should be (LVX)a=[V,X]a=X˙a−Xb∂bVa=0 evaluated
No. I moved the term ##X^b \partial_b V^a## to the RHS. Hence resulting in
$$
\dot X^a = X^b \partial_b V^a = X^x \partial_x V^a + X^y \partial_y V^a.
$$
 
  • #33
Orodruin said:
No. I moved the term ##X^b \partial_b V^a## to the RHS. Hence resulting in
$$
\dot X^a = X^b \partial_b V^a = X^x \partial_x V^a + X^y \partial_y V^a.
$$
Yes, sure. The point is where the two terms ##- \omega X^y## and ##\omega X^x## come from ?
 
  • #34
cianfa72 said:
Yes, sure. The point is where the two terms ##- \omega X^y## and ##\omega X^x## come from ?
Evaluating the derivatives of ##V##.
 
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  • #35
facenian said:
In my opinion the origen of FWT is better understood in flat spacetime. Its generalization to curved space time is then rutinary as explained in this paper https://doi.org/10.1007/s10699-020-09679-9
I think that's a bit overcomplicating the issue. Indeed FWT provides a transport of a tetrad along a time-like worldline which is locally rotation free. That's must simpler derived directly by simply using an infinitesimal Lorentz transformation when moving an "infinitesimal increment" along the worldline:

https://itp.uni-frankfurt.de/~hees/pf-faq/srt.pdf p. 21ff
 
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  • #36
facenian said:
My point was that to understand the FWT concept, it is simpler to carry out the analysis in flat spacetime
Which, as has already been pointed out, is exactly what the article under discussion does. If other references try to start the analysis in curved spacetime, that is irrelevant for this discussion.

You have now been banned from further posting in this thread.
 
  • #37
Orodruin said:
However, the Lie derivative of ##X## if you want to Lie transport it is given by ##(\mathcal L_V X)^a = [V,X]^a = \dot X^a - X^b \partial_b V^a = 0##, leading to the two non-trivial equations
$$
\dot X^x = X^x \partial_x V^x + X^y \partial_y V^x = - \omega X^y, \qquad
\dot X^y = \omega X^x
$$ with the solution ##X^x = \cos(\omega s)## and ##X^y = \sin(\omega s)## and therefore ##X^x = \cos(\omega)## and ##X^y = \sin(\omega)## for ##s = 1##, which is generally different from (0,1,0).
Just to be complete: there is a third equation namely
$$ \dot X^t = X^t \partial_t V^t = X^t$$ for which ##X^t=0## identically is a solution.

Therefore the solution vector field ##X## 'evaluated' at the point ##(0,0,0)## matches the vector ##X^x=1,X^t,X^y=0## we started with. Hence the vector field ##X## (i.e. its components ##X^t,X^x,X^y##) is function of ##s## coordinate only.

Is the above correct ? Thanks.
 
Last edited:
  • #38
cianfa72 said:
Just to be complete: there is a third equation namely
$$ \dot X^t = X^t \partial_t V^t = X^t$$ for which ##X^t=0## identically is a solution.
The component ##V^t## is equal to one. Therefore its derivative is zero.
 
  • #39
Orodruin said:
The component ##V^t## is equal to one. Therefore its derivative is zero.
Yes sure, we get ##\dot X^t = 0## therefore ##X=const=0## identically. As said in #37 the solution vector field ##X## is a function of coordinate ##t## only (i.e. ##s## along the curve), right ?
 
  • #40
cianfa72 said:
Yes sure, we get ##\dot X^t = 0## therefore ##X=const=0## identically. As said in #37 the solution vector field ##X## is a function of coordinate ##t## only (i.e. ##s## along the curve), right ?
Technically ##X## is not a full field, but only defined along the integral curve, which makes it a function of the curve parameter such that ##s\mapsto X(s) \in T_{\gamma(s)}M##, where ##\gamma(s)## is the point the parameter maps to along the curve.
 
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  • #41
Orodruin said:
Technically ##X## is not a full field, but only defined along the integral curve, which makes it a function of the curve parameter such that ##s\mapsto X(s) \in T_{\gamma(s)}M##, where ##\gamma(s)## is the point the parameter maps to along the curve.
So basically the solution ##X## is not defined in a open neighborhood of each point along the integral curve. What has been done is to solve the three differential equations along the integral curve ##t=0##.
 
  • #42
cianfa72 said:
So basically the solution ##X## is not defined in a open neighborhood of each point along the integral curve. What has been done is to solve the three differential equations along the integral curve ##t=0##.
The integral curve is ##x = y = 0##, ##t## is the only varying coordinate.
 
  • #43
Orodruin said:
The integral curve is ##x = y = 0##, ##t## is the only varying coordinate.
Oops, yes (i.e. let me say ##t## becomes the curve parameter ##s##). Thank you.
 

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