## Abstract A general method to quantize strings in curved spaceβtimes is exposed. It treats the spaceβtime metric exactly and the string excitations small as compared with the energy scale of the geometry. The method is applied to cosmological (de Sitter) and blackβhole (Schwarzschild) geometries
β¦ LIBER β¦
Electromagnetic variations in curved space-times
β Scribed by E. A. Evangelidis
- Publisher
- Springer Netherlands
- Year
- 1980
- Tongue
- English
- Weight
- 425 KB
- Volume
- 68
- Category
- Article
- ISSN
- 0004-640X
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Abstrae. The covariant Weyl (spin s = 1/2) and Maxwell (s = 1) equations in certain local charts (U, 9 ) of a space-time ( M , g ) are considered. It is shown that the condition goo(z) > 0 for all z E U is necessary and sufficient to rewrite them in a unified manner as evolution equations at4 = L(,)