Show Spherical Symmetry of Schwarzschild Metric

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SUMMARY

The Schwarzschild metric is confirmed to be spherically symmetric through the analysis of its Lie derivative with respect to the vector field X = sin φ ∂/∂θ + cot θ cos φ ∂/∂φ. The metric components are defined as g_{00} = 1 - 2gm/r, g_{11} = -(1 - 2gm/r)^{-1}, g_{22} = -r^2, and g_{33} = -r^2 sin²θ, with all nondiagonal components being zero. The Lie derivative calculation reveals that all components vanish except for the (33) component, which simplifies to -4r² sin θ cos θ sin φ. The discussion emphasizes the importance of recognizing the inherent rotational symmetry in the angular part of the metric.

PREREQUISITES
  • Understanding of General Relativity (GR) concepts
  • Familiarity with the Schwarzschild metric
  • Knowledge of Lie derivatives in differential geometry
  • Proficiency in tensor calculus
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  • Study the properties of the Schwarzschild metric in detail
  • Learn about Lie derivatives and their applications in General Relativity
  • Explore the implications of spherical symmetry in gravitational fields
  • Investigate the role of angular momentum in the Schwarzschild solution
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Students and researchers in theoretical physics, particularly those focusing on General Relativity, differential geometry, and gravitational theories. This discussion is beneficial for anyone looking to deepen their understanding of the Schwarzschild metric and its symmetries.

mjordan2nd
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In one of the lectures I was watching it was stated without proof that the Schwarzschild metric is spherically symmetric. I thought it would be a good exercise in getting acquainted with the machinery of GR to show this for at least one of the vector fields in the algebra. The Schwarzschild metric is given as follows

g_{00} = 1-\frac{2gm}{r}
g_{11} = - \left( 1 - \frac{2gm}{r} \right)^{-1}
g_{22} = -r^2
g_{33} = -r^2 sin \theta

and all nondiagonal components are zero. Right now I'm just trying to show that the Lie derivative vanishes with respect to the following vector field:

X=sin \phi \frac{\partial}{\partial \theta} + \cot \theta \cos \phi \frac{\partial}{\partial \phi}.

By the way, if my chart map is Q then the convention I'm using is t = Q^0, r=Q^1, \theta = Q^2 and \phi = Q^3.

In components the Lie derivative is given by

(\ell_X g)_{ij} = X^m \frac{\partial}{\partial x^m}(g_{ij}) - \frac{\partial X^s}{\partial x^i} g_{sj} - \frac{\partial X^s}{\partial x^j}g_{is}.

I've been able to show that all components of the Lie derivative are zero except for the (33) component. For the (33) component of the Lie derivative the only term that shows up from the first term is when m=2, and it is -2r^2 \sin \theta \cos \theta \sin \phi. For the next two terms, the only contribution will be when s=3, and the two terms will be equal so that term can be written as

-2 \frac{\partial X^3}{\partial \phi} g_{33}
2 \cot \theta \sin \phi g_{33}
-2 r^2 \cot \theta \sin \phi sin^2 \theta
-2r^2 \cos \theta \sin \theta \sin \phi

So overall I'm getting

(\ell_X g)_{ij} = -4r^2 \sin \theta \cos \theta \sin \phi. I feel like maybe I'm just dropping a negative somewhere, but I'm not seeing it. Any help figuring this out would be appreciated. Thanks.
 
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Never mind. I now see that my formula for the Lie derivative is wrong. The minuses should be pluses.
 
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Likes   Reactions: Dale
Even if you solved it already, I would just point out that it should be quite clear from the beginning, as it is an assumption Schwarzschild used to derive it. The angular part of the metric is just the regular metric on a sphere - which displays rotational symmetry. It is the only part of the metric that is affected by rotations.
 
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Likes   Reactions: vanhees71
Thank you for pointing this out. I have a tendency to miss these kind of connections and get lost in the heap of algebra, especially when learning something new.
 

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