Singularities associated with an incomplete space time (S) are not well-defined until a boundary is attached to it. Moreover, each boundary (B) gives rise to a different singularity structure for SwB, the resulting "total" space-time (TST). Since S is compatible with a variety of boundaries, it ther
โฆ LIBER โฆ
The total space-time of a point charge and its consequences for black holes
โ Scribed by Leonard S. Abrams
- Publisher
- Springer
- Year
- 1996
- Tongue
- English
- Weight
- 727 KB
- Volume
- 35
- Category
- Article
- ISSN
- 0020-7748
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