Interacting black holes

@inproceedings{Costa2000InteractingBH,
  title={Interacting black holes},
  author={M. S. Costa and Malcolm J. Perry},
  year={2000}
}
We revisit the geometry representing l collinear Schwarzschild black holes. It is seen that the black holes’ horizons are deformed by their mutual gravitational attraction. The geometry has a string like conical singularity that connects the holes but has nevertheless a well defined action. Using standard gravitational thermodynamics techniques we determine the Free energy for two black holes at fixed temperature and distance, their entropy and mutual force. When the black holes are far apart… CONTINUE READING

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