Abstract
Recent theorems regarding topological censorship are in apparent conflict with simulations of the collapse of rotating matter to form toroidal black holes. The geometry of a temporarily toroidal event horizon is analyzed and shown to be completely consistent with the theorems. A simple flat space model provides insight into the geometry of a toroidal black hole.
Original language | English (US) |
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Pages (from-to) | 6982-6987 |
Number of pages | 6 |
Journal | Physical Review D |
Volume | 52 |
Issue number | 12 |
DOIs | |
State | Published - 1995 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)