Kerr
General Relativity · Part 4
184 KB10 sections4 key equationsLaTeX typeset
Table of Contents
- 1.The Boyer-Lindquist Metric
- 2.The Newman-Janis Algorithm
- 3.Event Horizons
- 4.The Ergosphere
- 5.Important Limiting Cases
- 6.Metric Determinant and Inverse
- 7.The Kerr Metric
- 8.Newman-Janis procedure:
- 9.Kerr Horizons
- 10.Outer horizon r₊
Key Equations
$$ds^2 = -\left(1 - \frac{2Mr}{\Sigma}\right)dt^2 - \frac{4Mar\sin^2\theta}{\Sigma}\,dt\,d\phi + \frac{\Sigma}{\Delta}\,dr^2 + \Sigma\,d\theta^2 + \frac{\mathcal{A}\sin^2\theta}{\Sigma}\,d\phi^2$$
$$\mathcal{A} = (r^2 + a^2)^2 - a^2\Delta\sin^2\theta$$
$$g_{tt} = -\left(1 - \frac{2Mr}{\Sigma}\right) > 0 \quad \Longrightarrow \quad r < r_{\text{ergo}}(\theta)$$
$$ds^2 = -dt^2 + \frac{r^2 + a^2\cos^2\theta}{r^2 + a^2}\,dr^2 + (r^2 + a^2\cos^2\theta)\,d\theta^2 + (r^2+a^2)\sin^2\theta\,d\phi^2$$
Equations are rendered with MathJax in the PDF with professional LaTeX typesetting.
Course Context
This PDF is part of the General Relativity course on CoursesHub.World. Explore Einstein's theory of gravity as curved spacetime. Covers differential geometry, curvature tensors, Einstein field equations, classic solutions including Schwarzschild and Kerr black holes, gra...