We consider the modifications to general relativity by the non-local (classical and quantum) string effects for the case of a \(D\)-dimensional Schwarzschild black hole. The classical non-local effects do not alter the spacetime topology (the horizon remains unshifted, at least perturbatively). We s
✦ LIBER ✦
Remarks on thermal strings outside black hole
✍ Scribed by J.L.F. Barbón
- Publisher
- Elsevier Science
- Year
- 1994
- Tongue
- English
- Weight
- 597 KB
- Volume
- 339
- Category
- Article
- ISSN
- 0370-2693
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We criticize and generalize some properties of No ther charges presented in a paper by V. Iyer and R. M. Wald and their application to entropy of black holes. The first law of black holes thermodynamics is proven for any gauge natural field theory. As an application charged Kerr Newman solutions are