Find Geodesics in Dynamic Ellis Orbits Metric

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Discussion Overview

The discussion revolves around finding geodesics in the dynamic Ellis orbits metric, specifically the metric given by ##ds^2=-dt^2+dp^2+(5p^2+4t^2)d\phi^2##. Participants explore various methods for solving the geodesic equations, including the geodesic Lagrangian method, and consider the implications of the metric's properties on these methods.

Discussion Character

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

Main Points Raised

  • One participant inquires about the possibility of finding geodesics analytically in the given metric.
  • Another participant questions the applicability of techniques discussed in a previous thread on geodesics.
  • Several participants reference the Wikipedia article on Ellis Wormholes to clarify the metric in question.
  • It is noted that ##\partial_\phi## is a Killing field, which may provide a conserved quantity useful for simplifying the geodesic equations.
  • Participants discuss the geodesic Lagrangian method and its potential advantages over brute force methods, particularly due to the metric's structure.
  • There is uncertainty about the existence of Killing fields for ##t## and ##p##, which complicates the analysis.
  • One participant expresses a desire to find a way to integrate geodesics exactly rather than using numerical methods like Euler or Runge-Kutta.
  • Concerns are raised about the feasibility of integrating certain differential equations exactly, emphasizing the need to analyze the equations themselves.
  • Discussion includes whether the Lagrangian method is applicable to both timelike and null geodesics, with some technical complications noted for the latter.
  • Participants debate the merits of different approaches to solving the geodesic equations, with suggestions to experiment with various methods.

Areas of Agreement / Disagreement

Participants express differing views on the applicability of previous techniques and the effectiveness of various methods for finding geodesics. No consensus is reached on the best approach or the solvability of the equations involved.

Contextual Notes

Participants highlight the complexity of the geodesic equations due to the specific form of the metric and the presence of only one function of the coordinates. There is also mention of the potential for certain Christoffel symbols to vanish, affecting the analysis.

Who May Find This Useful

This discussion may be of interest to those studying general relativity, particularly in the context of wormhole metrics and geodesic calculations.

  • #31
Their derivatives with respect to the affine parameter.

This is what I meant by one-forms
 
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  • #32
Onyx said:
This is what I meant by one-forms
Then you should be aware that that is not correct terminology.
 
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  • #33
So, @Onyx, what is the relevant Lagrangian for GR, and for Schwarzschild spacetime specifically?
 
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  • #34
Ibix said:
So, @Onyx, what is the relevant Lagrangian for GR, and for Schwarzschild spacetime specifically?
Ibix said:
So, @Onyx, what is the relevant Lagrangian for GR, and for Schwarzschild spacetime specifically?
##L=\sqrt{{g_{uv}}u'v'}##
 
  • #35
Onyx said:
##L=\sqrt{{g_{uv}}u'v'}##
Well, I wouldn't bother with the square root, but that's up to you. Set ##\theta=\pi/2## for simplicity's sake, which makes ##\partial\mathcal{L}/\partial\theta=\partial\mathcal{L}/\partial\dot\theta=0##. What do the three remaining Euler-Lagrange equations give you?
 
  • #36
Ibix said:
Well, I wouldn't bother with the square root, but that's up to you. Set ##\theta=\pi/2## for simplicity's sake, which makes ##\partial\mathcal{L}/\partial\theta=\partial\mathcal{L}/\partial\dot\theta=0##. What do the three remaining Euler-Lagrange equations give you?
##\partial\mathcal{L}/\partial\dot\phi=r^2d\phi##
##\partial\mathcal{L}/\partial\dot t=\frac{r_s-r}{r}dt##
##\partial\mathcal{L}/\partial\dot r=\frac{r}{r-r_s}dr##
 
  • #37
No. ##\mathcal{L}=\left(1-\frac{r_S}{r}\right)\dot{t}^2-\left(1-\frac{r_S}{r}\right)^{-1}\dot{r}^2-r^2\dot{\phi}^2##. Where are the differentials coming from on your right hand side?
 
  • #38
Ibix said:
No. ##\mathcal{L}=\left(1-\frac{r_S}{r}\right)\dot{t}^2-\left(1-\frac{r_S}{r}\right)^{-1}\dot{r}^2-r^2\dot{\phi}^2##. Where are the differentials coming from on your right hand side?
##\partial\mathcal{L}/\partial\dot\phi=2r^2d\phi##
##\partial\mathcal{L}/\partial\dot t=2\frac{r_s-r}{r}dt##
##\partial\mathcal{L}/\partial\dot r=2\frac{r}{r-r_s}dr##
 
  • #39
Why are there differentials on your right hand sides?
 
  • #40
Ibix said:
Why are there differentials on your right hand sides?
##\frac{dx^u}{d\tau}##
 
  • #41
Onyx said:
##\frac{dx^u}{d\tau}##
Just the chain rule applied to the right side when differentiating wrt the dotted variables.
 
  • #42
Onyx said:
Just the chain rule applied to the right side when differentiating wrt the dotted variables.
##d\phi = \dot\phi##
 
  • #43
Onyx said:
##d\phi = \dot\phi##
No it doesn't. ##\dot{\phi}=d\phi/d\tau##. What is the correct expression for ##\partial\mathcal{L}/\partial \dot x^i##? Don't randomly replace symbols with unrelated ones.
 
  • #44
Ibix said:
No it doesn't. ##\dot{\phi}=d\phi/d\tau##. What is the correct expression for ##\partial\mathcal{L}/\partial \dot x^i##? Don't randomly replace symbols with unrelated ones.
Just replace the differentials in post #38 with dotted variables.
 
  • #45
Onyx said:
Just replace the differentials in post #38 with dotted variables.
If not that, then I don't know.
 
  • #46
Onyx said:
Just replace the differentials in post #38 with dotted variables.
No, you replace the differentials with dotted variables. If you want help, you need to do that part of the work yourself. We're not going to auto-correct what you post for you.
 
  • #47
Onyx said:
Just replace the differentials in post #38 with dotted variables.
I suspect that's correct, but you seem to have some odd ideas about differentials so it would be a good idea for you to write it out.

You will also need the three ##\partial\mathcal{L}/\partial x^i##, which I don't think you've posted.
 
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  • #48
Ibix said:
I suspect that's correct, but you seem to have some odd ideas about differentials so it would be a good idea for you to write it out.

You will also need the three ##\partial\mathcal{L}/\partial x^i##, which I don't think you've posted.
Oh, I see what you mean. In that case, ##\partial\mathcal{L}/\partial \phi=\partial\mathcal{L}/\partial t=0##. Meanwhile, ##\partial\mathcal{L}/\partial r## is a function of ##r##.
 
  • #49
So what do you now know about ##dt/d\tau## and ##d\phi/d\tau##?
 
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  • #50
Okay, so for the Ellis metric, I get from the EL equation that ##\frac{\partial \dot t}{\partial \tau}=-4t\dot \phi^2## and ##\frac{\partial \dot p}{\partial \tau}=5p\dot \phi^2##. But I'm unsure how to proceed. Could I divide the equations to get an equation of ##\frac{dp}{dt}##? My thinking is that would take care of the ##\dot \phi^2.##
 
  • #51
Onyx said:
Okay, so for the Ellis metric, I get from the EL equation that ##\frac{\partial \dot t}{\partial \tau}=-4t\dot \phi^2## and ##\frac{\partial \dot p}{\partial \tau}=5p\dot \phi^2##.
No, that's not quite what you get from the EL equations. Since you haven't shown your work I can't tell where you went wrong, but you went wrong somewhere. Note that you should get three equations, not two; even though the metric does not depend on ##\phi##, the EL equation for ##\dot{\phi}## still has non-negligible content.
 
  • #52
##\mathcal{L}=-\dot t^2+\dot p^2+\frac{1}{5p^2+4t^2}##
##\frac{\partial\mathcal{L}}{\partial t}=\frac{d}{d\tau}\frac{\partial\mathcal{L}}{\partial\dot t}##
##\frac{\partial\mathcal{L}}{\partial t}=-2\frac{d}{d\tau}\dot t##
##-\frac{8t}{(5p^2+4t^2)^2}=-2\frac{d}{d\tau}\dot t##
##\frac{4t}{(5p^2+4t^2)^2}=\frac{d}{d\tau}\dot t##
 
  • #53
Onyx said:
##\mathcal{L}=-\dot t^2+\dot p^2+\frac{1}{5p^2+4t^2}##
##\frac{\partial\mathcal{L}}{\partial t}=\frac{d}{d\tau}\frac{\partial\mathcal{L}}{\partial\dot t}##
##\frac{\partial\mathcal{L}}{\partial t}=-2\frac{d}{d\tau}\dot t##
##-\frac{8t}{(5p^2+4t^2)^2}=-2\frac{d}{d\tau}\dot t##
##\frac{4t}{(5p^2+4t^2)^2}=\frac{d}{d\tau}\dot t##
And so it follows that...
##-\frac{5p}{(5p^2+4t^2)^2}=\frac{d}{d\tau}\dot p##
 
  • #54
You are missing a ##\dot\phi^2## in the last term in your expression for ##\mathcal{L}##, so your expressions for ##d\dot p/d\tau## and ##d\dot t/d\tau## are both incorrect by that factor.

As Peter says, you also need the ##\phi## Euler-Lagrange equation which will enable you to eliminate ##\dot\phi## from the other two equations if you use it.
 
Last edited:
  • #55
Onyx said:
##\mathcal{L}=-\dot t^2+\dot p^2+\frac{1}{5p^2+4t^2}##
##\frac{\partial\mathcal{L}}{\partial t}=\frac{d}{d\tau}\frac{\partial\mathcal{L}}{\partial\dot t}##
##\frac{\partial\mathcal{L}}{\partial t}=-2\frac{d}{d\tau}\dot t##
##-\frac{8t}{(5p^2+4t^2)^2}=-2\frac{d}{d\tau}\dot t##
##\frac{4t}{(5p^2+4t^2)^2}=\frac{d}{d\tau}\dot t##
As @Ibix pointed out, the last term in your ##\mathcal{L}## needs a ##\dot{\phi}^2##. Also I don't understand why ##5p^2 + 4t^2## is in the denominator.

Your second line does correctly state the Euler-Lagrange equation for one coordinate, namely ##t##. There are two others, for ##p## and ##\phi##.

Your third line does correctly evaluate ##d / d\tau ( \partial \mathcal{L} / \partial \dot{t} )##.

Your fourth and fifth lines, however, do not correctly evaluate ##\partial \mathcal{L} / \partial t##.
 
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  • #56
Onyx said:
And so it follows that...
##-\frac{5p}{(5p^2+4t^2)^2}=\frac{d}{d\tau}\dot p##
But if I treated the lagrangian
PeterDonis said:
As @Ibix pointed out, the last term in your ##\mathcal{L}## needs a ##\dot{\phi}^2##. Also I don't understand why ##5p^2 + 4t^2## is in the denominator.

Your second line does correctly state the Euler-Lagrange equation for one coordinate, namely ##t##. There are two others, for ##p## and ##\phi##.

Your third line does correctly evaluate ##d / d\tau ( \partial \mathcal{L} / \partial \dot{t} )##.

Your fourth and fifth lines, however, do not correctly evaluate ##\partial \mathcal{L} / \partial t##.
I forgot to mention that I made the angular momentum ##1##, which is why ##5p^2+4t^2## is in the denominator.
 
  • #57
Onyx said:
I forgot to mention that I made the angular momentum ##1##
Which is wrong. The Lagrangian does not specify particular values for any conserved quantities.

Do you understand how to convert an expression for the metric into a Lagrangian?
 
  • #58
Onyx said:
I forgot to mention that I made the angular momentum ##1##, which is why ##5p^2+4t^2## is in the denominator.
So you are using the remaining Euler-Lagrange equation, ##\frac d{d\tau}\frac{d\mathcal{L}}{d\dot\phi}=0##, to imply ##2\dot\phi(5p^2+4t^2)=\mathrm{const}##, then setting the constant to 1 and substituting into your expression for ##\mathcal{L}##? In that case, I think you actually set your angular momentum to 2. And you should definitely make this calculation explicit rather than leaving usto guess that you are treating a special case.

It would make more sense to use the ##\phi## Euler-Lagrange equation to get the conservation law (as I did in my last paragraph) and then substitute it in to your other expressions.
 
  • #59
Ibix said:
So you are using the remaining Euler-Lagrange equation, ##\frac d{d\tau}\frac{d\mathcal{L}}{d\dot\phi}=0##, to imply ##2\dot\phi(5p^2+4t^2)=\mathrm{const}##, then setting the constant to 1 and substituting into your expression for ##\mathcal{L}##?
A more pertinent question would be, is doing that correct? And the answer to that is no.
 
  • #60
PeterDonis said:
A more pertinent question would be, is doing that correct? And the answer to that is no.
Doesn't it just constrain the Lagrangian to apply to the case where the angular momentum is as specified? My maths suggests it works out correctly (at least in this case), but I did it with Maxima on my phone so the possibility of arithmetic slips is non-zero.
 

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