Duality-invariant non-extreme black holes in toroidally compactified string theory

@article{Cveti1997DualityinvariantNB,
  title={Duality-invariant non-extreme black holes in toroidally compactified string theory},
  author={Mirjam Cveti{\vc} and Ingo Gaida},
  journal={Nuclear Physics},
  year={1997},
  volume={505},
  pages={291-306}
}

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References

SHOWING 1-10 OF 47 REFERENCES

Entropy of nonextreme charged rotating black holes in string theory.

  • CvetićYoum
  • Physics
    Physical review. D, Particles and fields
  • 1996
The explicit expression for four-dimensional rotating charged black hole solutions of N=4 (or N=8) superstring vacua, parameterized by the ADM mass, four charges, and the angular momentum and the asymptotic values of four toroidal moduli of two-torus and the dilaton-axion field are given.

Dyonic BPS saturated black holes of heterotic string on a six-torus.

  • CvetićYoum
  • Physics
    Physical review. D, Particles and fields
  • 1996
Within effective heterotic superstring theory compactified on a six-torus we derive minimum energy (supersymmetric), static, spherically symmetric solutions, which are manifestly invariant under the

Solitonic strings and BPS saturated dyonic black holes.

The expression for the level of the WZW theory describing the throat region implies a renormalisation of the string tension by a product of magnetic charges, thus relating the entropy and the number of oscillations of the solitonic string in compact directions.