Abstract
Basic features of dynamical black holes in full, non-linear general relativity are summarized in a pedagogical fashion. Qualitative properties of the evolution of various horizons follow directly from the celebrated Raychaudhuri equation.
| Original language | English (US) |
|---|---|
| Pages (from-to) | 77-92 |
| Number of pages | 16 |
| Journal | Pramana - Journal of Physics |
| Volume | 69 |
| Issue number | 1 |
| DOIs | |
| State | Published - Jul 2007 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy
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