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# Ricci flow and black holes

@inproceedings{Headrick2006RicciFA, title={Ricci flow and black holes}, author={Matthew Headrick}, year={2006} }

- Published 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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