Ricci flow and black holes

@inproceedings{Headrick2006RicciFA,
  title={Ricci flow and black holes},
  author={Matthew Headrick},
  year={2006}
}
Gradient flow in a potential energy (or Euclidean action) landscape provides a natural set of paths connecting different saddle points. We apply this method to General Relativity, where gradient flow is Ricci flow, and focus on the example of 4-dimensional Euclidean gravity with boundary S1 × S2, representing the canonical ensemble for gravity in a box. At high temperature the action has three saddle points: hot flat space and a large and small black hole. Adding a time direction, these also… CONTINUE READING
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