Difficult general relativity problem - Weyl's axisymmetric solution

In summary, the conversation is about a course on general relativity and a difficult exercise involving Weyl's solution to the field equations in a vacuum. The exercise reduces to Laplace's equation in cylindrical coordinates and suggests a way to generate solutions to the Einstein Fields equations. The conversation also discusses the static nature of the Weyl metric, the irrelevance of adding a constant to U and V, and the relationship between U and V in terms of generating flat space. The conversation also mentions a simple solution to Laplace's equation and its corresponding V, and the asymptotically flat nature of the metric. Lastly, the conversation mentions the Curzon-Chazy solution and its relationship to Schwarzschild and spherical symmetry in the context of Newton
  • #1
patrick_gold
1
0
I'm currently doing a course on general relativity, and I'm struggling with the following exercise - I would greatly appreciate the help anyone might offer. Whilst not technically homework (not assessed or in a tutorial set) it is from a collection of difficult questions from a recommended resource. It is as follows:

Homework Statement



Weyl's solution to the field equations in a vacuum has that

$$ ds^{2} = e^{2U}dt^{2} -e^{-2U}(r^{2}d\phi ^{2} + e^{2V}(dr^{2} +dz^2)) $$ $$ where \; \; U=U(r,z),\; V=V(r,z); $$

and the field equations reduce to Laplace's equation in cylindrical coordinates, that being

$$ \nabla^{2}U = U_{,rr} + r^{-1}U_{,r} + U_{,zz}=0, $$

as given U we can find V by integration:

$$ V_{,r}=r((U_{,r})^{2}-(U_{,z})^2)\;, \; \; \; V_{,z}=2rU_{,r}U_{,z} \;. $$

This suggests a way of generating solutions to the Einstein Fields equations: Laplace's
equation is linear, so just add arbitrary (axially symmetric) solutions of it to get U
and then find V .


(a) Why is the Weyl metric static?


(b) Explain why adding a constant to either (or both) U and V is geometrically
(and hence physically) irrelevant.


(c) If $$U\equiv 0 $$ we clearly have flat space. Show that if $$U = V$$ we also have flat space. [Hint: perhaps we might change coordinates (something about hyperbolic trig functions and rapidity?)] This suggests generating GR solutions from Newtonian ones will not be as easy as it seems.


(d)The simplest non-trivial solution to Laplace's equation is the (spherically symmetric) potential of a point particle: $$U=-\frac{m}{\sqrt{r^{2}+z^{2}}}$$. Show this is a solution to $$\nabla^{2}U=0$$, find the corresponding V and explain why the metric is asymptotically flat.


(e) The solution is part (d) is known as the Curzon-Chazy solution. Prove it is not Schwarzschild and so not spherically symmetric. (Thus once again demonstrating that the Newtonian solution and the Einsteinian solutions are not simply related.)


*Nota bene c=1 here.




Homework Equations


See question statement


The Attempt at a Solution


I've struggled a bit, there's some obvious substitution work in here verifying things are solutions but I'm not very confident with the rest of the material.
 
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  • #2
(a) The Weyl metric is static as the metric does not depend on time.(b) Adding a constant to either U or V does not change the metric in terms of its geometry, and thus any physical effects of the metric are unchanged.(c) I'm a bit lost here. (d) $$\nabla^{2}U = U_{,rr} + r^{-1}U_{,r} + U_{,zz}= -\frac{m}{(r^{2}+z^{2})^{\frac{3}{2}}}(-2r^{2}+2z^{2}) + \frac{m}{r(r^{2}+z^{2})^{\frac{1}{2}}} + \frac{m}{(r^{2}+z^{2})^{\frac{3}{2}}}(-2z^{2}+2r^{2}) =0.$$V can be calculated from the given expression for V_{,r} and V_{,z}. The metric is asymptotically flat as it approaches a flat metric as values for r and z become large.(e) I'm also a bit lost here.
 

Related to Difficult general relativity problem - Weyl's axisymmetric solution

1. What is the Weyl's axisymmetric solution in general relativity?

The Weyl's axisymmetric solution is a mathematical solution to Einstein's field equations in general relativity. It describes the gravitational field of a rotating, axially symmetric mass distribution.

2. Why is the Weyl's axisymmetric solution considered a difficult problem in general relativity?

The Weyl's axisymmetric solution is considered difficult because it involves complex mathematical calculations and concepts, such as the Weyl tensor and the Kerr metric, making it challenging to solve and understand.

3. What is the significance of the Weyl's axisymmetric solution?

The Weyl's axisymmetric solution is significant because it provides a theoretical framework for understanding the gravitational field of rotating objects, such as black holes, which have been observed in our universe.

4. How is the Weyl's axisymmetric solution related to other solutions in general relativity?

The Weyl's axisymmetric solution is one of the most important solutions in general relativity and has connections to other solutions, such as the Schwarzschild solution for non-rotating objects and the Kerr solution for rotating objects.

5. What are some applications of the Weyl's axisymmetric solution?

The Weyl's axisymmetric solution has various applications in astrophysics and cosmology, such as in the study of black holes, gravitational waves, and the evolution of the universe. It also has practical applications in the gravitational lensing effect, which is used in astronomical observations to study distant objects in the universe.

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