Curvature Invariants for Charged and Rotating Black Holes
Riemann curvature invariants are important in general relativity because they encode the geometrical properties of spacetime in a manifestly coordinate-invariant way. Fourteen such invariants are required to characterize four-dimensional spacetime in general, and Zakhary and McIntosh showed that as...
| 主要な著者: | , , , |
|---|---|
| フォーマット: | 論文 |
| 言語: | English |
| 出版事項: |
MDPI AG
2020-01-01
|
| シリーズ: | Universe |
| 主題: | |
| オンライン･アクセス: | https://www.mdpi.com/2218-1997/6/2/22 |