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 languageEnglish (US)
Pages (from-to)77-92
Number of pages16
JournalPramana - Journal of Physics
Volume69
Issue number1
DOIs
StatePublished - Jul 1 2007

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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