Chapter 11: Symmetries and Killing Vectors
Killing vectors generate symmetries of spacetimeβisometries that leave the metric unchanged. Each Killing vector corresponds to a conserved quantity along geodesics, providing powerful tools for solving the geodesic equation.
Killing's Equation
A vector field ΞΎΞΌ is a Killing vector if the Lie derivative of the metric vanishes:
\( \mathcal{L}_\xi g_{\mu\nu} = 0 \)
Equivalently: \( \nabla_\mu \xi_\nu + \nabla_\nu \xi_\mu = 0 \)
This means the metric is unchanged when we "flow" along the direction of ΞΎΞΌ. The spacetime looks the same from any point along this flow.
Common Killing Vectors
Time Translation (Schwarzschild)
\( \xi^\mu = (1, 0, 0, 0) = \partial_t \)
Metric doesn't depend on t β Energy conservation
Axial Rotation (Schwarzschild)
\( \psi^\mu = (0, 0, 0, 1) = \partial_\phi \)
Metric doesn't depend on Ο β Angular momentum conservation
Minkowski Space (10 Killing vectors)
4 translations + 3 rotations + 3 boosts = 10 generators of PoincarΓ© group
Conserved Quantities
For a geodesic with tangent uΞΌ, each Killing vector gives a conserved quantity:
\( Q = \xi_\mu u^\mu = \text{constant along geodesic} \)
Energy
\( E = -\xi_\mu u^\mu = -g_{tt} \frac{dt}{d\tau} \)
From time translation symmetry
Angular Momentum
\( L = \psi_\mu u^\mu = g_{\phi\phi} \frac{d\phi}{d\tau} \)
From axial rotation symmetry
Killing Tensors
Some spacetimes have higher-rank Killing tensors KΞΌΞ½ satisfying:
\( \nabla_{(\rho} K_{\mu\nu)} = 0 \)
Carter Constant (Kerr Spacetime)
The Kerr metric has a non-trivial Killing tensor giving the Carter constant Q:
\( Q = K_{\mu\nu} u^\mu u^\nu = \text{constant} \)
This "hidden symmetry" makes geodesics in Kerr spacetime integrable.
Python: Killing Vector Analysis
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Fortran: Conserved Quantities
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