Second fundamental form and Mean Curvature

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SUMMARY

The discussion focuses on calculating the second fundamental form and mean curvature from a specified metric tensor in a spacetime context. The metric is given by the equation ds² = e^{\tilde{A}(\tilde{\tau})} d\tilde{t} - d\tilde{r} - e^{\tilde{C}(\tilde{\tau})} dΩ, with components defined for g_{00}, g_{11}, g_{22}, and g_{33}. The second fundamental form is derived using the formula h_{ij} = g_{kl} Γ^{k}_{ij} n^{l}, resulting in a diagonal matrix. The mean curvature is expressed as h = g^{ij}h_{ij} = \frac{1}{2}\tilde{A'} - \frac{1}{2}\tilde{C'} - e^{-\tilde{C}}cot{θ}, with a critical note on the absence of r-dependence in the metric leading to zero extrinsic curvature.

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  • Understanding of differential geometry concepts, specifically metric tensors.
  • Familiarity with the calculation of Christoffel symbols in general relativity.
  • Knowledge of the second fundamental form and its significance in geometry.
  • Basic understanding of mean curvature and its applications in physics.
NEXT STEPS
  • Study the derivation of Christoffel symbols for various metrics in general relativity.
  • Explore the implications of extrinsic curvature in higher-dimensional spaces.
  • Investigate the role of mean curvature in the context of minimal surfaces.
  • Learn about the applications of second fundamental forms in modern theoretical physics.
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Students and researchers in theoretical physics, particularly those focusing on general relativity and differential geometry, as well as mathematicians interested in curvature properties of manifolds.

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Homework Statement



Metric ansatz:
[itex] ds^{2} = e^{\tilde{A}(\tilde{\tau})} d\tilde{t} - d\tilde{r} - e^{\tilde{C}(\tilde{\tau})} dΩ[/itex]

where: [itex]d\tilde{r} = e^{\frac{B}{2}} dr[/itex]

Homework Equations



How to calculate second fundamental form and mean curvature from this metric?

The Attempt at a Solution



Metric tensor:

[itex]g_{00}= e^{\tilde{A}(\tilde{\tau})}[/itex]
[itex]g_{11}= -1[/itex]
[itex]g_{22}= - e^{\tilde{C}(\tilde{\tau})}[/itex]
[itex]g_{33}- e^{\tilde{C}(\tilde{\tau})} sin^2 θ[/itex]

Second fundamental form:

[itex]h_{ij}= g_{kl} \Gamma^{k}_{ij} n^{l}[/itex]

where:

[itex]i, j, k, l = 0, 1, 2, 3[/itex]

[itex]n^{l} =[/itex]normal vector [itex]= (0, 1, 0, 0)[/itex]

so:

[itex]n^{0} = 0[/itex]
[itex]n^{1} = 1[/itex]
[itex]n^{2} = 0[/itex]
[itex]n^{3} = 0[/itex]

Second fundamental form:

[itex]h_{ij}= diag (\frac{1}{2}e^{\tilde{A}}\tilde{A'}, 0, \frac{1}{2}e^{\tilde{C}}\tilde{C'}, sin {θ} cos {θ})[/itex]

Mean curvature:

[itex]h = g^{ij}h_{ij}= \frac{1}{2}\tilde{A'}-\frac{1}{2}\tilde{C'}-e^{-\tilde{C}}cot {θ}[/itex]
 
Last edited:
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Your idea seems correct, but I don't understand what you're doing. Is there any r-dependence in the metric? If not, then all the relevant Christoffel symbols vanish and the extrinsic curvature should be zero (all r=const hyperslices are flat)
 

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