General relativity, geodesic question

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Homework Help Overview

The discussion revolves around a question related to geodesics in the context of general relativity, specifically within Minkowski spacetime. Participants are examining the conditions under which a curve can be classified as a geodesic based on the behavior of a tangent vector and its derivatives.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants are analyzing the expression ##V^{\alpha}\nabla_{\alpha}V^u=0## and its implications in Minkowski space. There are discussions about whether the components of the tangent vector can be independent of the parameter ##\Lambda## and how this affects the geodesic condition. Questions arise regarding the interpretation of multiple equations derived from the tangent vector's components and their consistency.

Discussion Status

The conversation is ongoing, with participants providing hints and clarifications regarding the conditions for a geodesic. There is a recognition that the original poster's approach may need reevaluation, particularly in connecting different parts of the question. While some guidance has been offered, there is no explicit consensus on the interpretation of the equations or the overall approach.

Contextual Notes

Participants note that the original poster has not provided specific textbook references, which may limit the context of the discussion. There is also mention of the need for relevant equations to be clearly stated in future posts to facilitate better understanding.

binbagsss
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Homework Statement



question attached

geodesicgrii.png


Homework Equations

The Attempt at a Solution



Attempt :

Check if ##V^{\alpha}\nabla_{\alpha}V^u=0##

Since Minkowski space, connection tensors/christoffel symbols are zero so this reduces to:

##V^{\alpha}\partial_{\alpha}V^u=0##

where ##\partial_{\alpha}=\frac{\partial}{\partial x^{\alpha}}##

Where ##V^{\alpha}=\frac{\partial x^{\alpha}}{\Lambda}## is the tangent vector

##\frac{\partial x^{\alpha}}{\Lambda} \partial_{\alpha}V^u = \frac{\partial x^{0}}{\Lambda} \partial_{0}V^u + \frac{\partial x^{1}}{\Lambda} \partial_{1}V^u +\frac{\partial x^{2}}{\Lambda} \partial_{2}V^u +\frac{\partial x^{3}}{\Lambda} \partial_{3}V^u
= 4 \frac{\partial V^u}{\Lambda} ## (using the chain rule)

which is 4 separate equations for ## u=0,1,2,3,4 ##, obviously these are not zero.

Have I done something wrong and should I have expected a summation ?

Or would I argue that these can not simultaneously all be zero for the same ##\Lambda## since cosh and sinh are independent?

Many thanks.
 
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Apologies typo edit:

Where ##V^{\alpha}=\frac{\partial x^{\alpha}}{ \partial \Lambda}## is the tangent vector

##\frac{\partial x^{\alpha}}{\partial \Lambda} \partial_{\alpha}V^u = \frac{\partial x^{0}}{\partial\Lambda} \partial_{0}V^u + \frac{\partial x^{1}}{\partial\Lambda} \partial_{1}V^u +\frac{\partial x^{2}}{\partial\Lambda} \partial_{2}V^u +\frac{\partial x^{3}}{\partial\Lambda} \partial_{3}V^u
= 4 \frac{\partial V^u}{\partial\Lambda} ## (using the chain rule)
 
Which part of the question are you trying to answer in your attempt in post #1? (If you're trying to answer part (c), that depends on the answer to part (a) which you haven't shown.)

Also, which textbook are you working from?

[And btw, I notice in several of your HW posts you make no attempt to write down any "relevant equations". That's not helping.]
 
strangerep said:
Which part of the question are you trying to answer in your attempt in post #1? (If you're trying to answer part (c), that depends on the answer to part (a) which you haven't shown.)

Also, which textbook are you working from?

[And btw, I notice in several of your HW posts you make no attempt to write down any "relevant equations". That's not helping.]

I have not listed relevant equations since they are either included in the question or attempt.

I am attempting part c)

For part a) you simply differentiate w.r.t ##\Lambda## and then compute ##g_{uv}V^vV^u## and check it's sign. ## < 0 ## here being time-like from the chosen metric convention.

Therefore I would identify a failure to make a connection between these two parts of the question as a mistake in the attempt, rather than purposely not showing to attempt question a, because I thought this wasn't as issue to me. Pretty much then, my approach to the question is wrong, which is all needed to be said.
 
binbagsss said:
I am attempting part c)

For part a) you simply differentiate w.r.t ##\Lambda## and then compute ##g_{uv}V^vV^u## and check it's sign. ## < 0 ## here being time-like from the chosen metric convention.
Are you sure? What are your components ##V^\mu## explicitly?

For part (c), can't you simply evaluate ##dV^\mu/d\lambda## (since the connection is 0 in Minkowski spacetime) ?

And you didn't tell me which textbook the question is from. Or is it from private lecture notes?
 
strangerep said:
Are you sure? What are your components ##V^\mu## explicitly?

For part (c), can't you simply evaluate ##dV^\mu/d\lambda## (since the connection is 0 in Minkowski spacetime) ?

And you didn't tell me which textbook the question is from. Or is it from private lecture notes?

My second post was exactly this? To evaluate ##dV^\mu/d\lambda=0##. My question was this is 4 separate equations? So to check whether it's a geodesic or not you check whether all four equations are consistent in the ##\lambda## which solves them?

For part a)
##V^u=( sinh \Lambda, \frac{1}{\sqrt 3} coshh \Lambda, \frac{1}{\sqrt{2}}cosh \Lambda, \frac{1}{\sqrt{6}}cosh \Lambda) ##

So the check for part c) returns the components of the original vector as four separate equations. My question was concerning solving them anyway. THIS: So to check whether it's a geodesic or not you check whether all four equations are consistent in the ##\lambda## which solves them?
 
binbagsss said:
My second post was exactly this? To evaluate ##dV^\mu/d\lambda=0##. My question was this is 4 separate equations? So to check whether it's a geodesic or not you check whether all four equations are consistent in the ##\lambda## which solves them?

For part a)
##V^u=( sinh \Lambda, \frac{1}{\sqrt 3} coshh \Lambda, \frac{1}{\sqrt{2}}cosh \Lambda, \frac{1}{\sqrt{6}}cosh \Lambda)##.
[...]
So to check whether it's a geodesic or not you check whether all four equations are consistent in the ##\lambda## which solves them?
I think you're overcomplicating this. To be a geodesic you'd need ##dV^\mu/d\lambda=0## for all ##\lambda##.
 
strangerep said:
I think you're overcomplicating this. To be a geodesic you'd need ##dV^\mu/d\lambda=0## for all ##\lambda##.

but ##\mu## runs over ##\mu=0,1,2,3## so need to solve, there are four equations to check, what am i over-complicated, don't we need to solve the following system of equations? To which the answer will be inconsistency due to the non-linear dependence of sinh and cosh?

## \frac{dV^{0}}{d\Lambda}=0##
## \frac{dV^{1}}{d\Lambda}=0##
## \frac{dV^{2}}{d\Lambda}=0##
## \frac{dV^{3}}{d\Lambda}=0##
 
I get the feeling you're not reading my reply hints carefully enough. I'll try one more time:
me said:
To be a geodesic you'd need ##dV^\mu/d\lambda=0## for all ##\lambda##.
Note the "for all ##\lambda##" part.
 
  • #10
strangerep said:
I get the feeling you're not reading my reply hints carefully enough. I'll try one more time:
Note the "for all ##\lambda##" part.

oh okay.
but there are four equations?
so this would have only happened if ## V^{u} ## components were constants indepedent of ##\Lambda##?
 
  • #11
binbagsss said:
oh okay.
but there are four equations?
So? It's a single vector (which has 4 components).

so this would have only happened if ## V^{u} ## components were constants independent of ##\lambda##?
If by "this", you mean "the curve would be a geodesic only if..." then yes -- because you're working with Minkowski spacetime in this question.
 
  • #12
strangerep said:
So? It's a single vector (which has 4 components).

because you're working with Minkowski spacetime in this question.

As in this is the expected result since we are in flat space-time?
I don't think I'm picking up what you are saying properly, could you explain a tad more?
greatly appreciated, thanks
 
  • #13
In Minkowski spacetime, with metric ##(-1,+1,+1,+1)##, the Christoffel connection coefficients are all 0. So the equation for a geodesic curve (in terms of an arbitrary parameter ##\lambda##) is just $$0 ~=~ \frac{d^2 x^\mu(\lambda)}{d\lambda^2} ~\equiv~ \frac{dV^\mu(\lambda)}{d\lambda} ~.$$ So if this equation is not satisfied (for any component), then the curve is not a geodesic.
 

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