The Einstein-Euler-Heisenberg-AdS black hole has a minimum Hawking temperature; above it large black holes are stable and small ones evaporate, and the nonlinear correction leaves this phase structure intact.
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The thermodynamic stability and phase structure of the Einstein-Euler-Heisenberg-AdS black holes
The Einstein-Euler-Heisenberg-AdS black hole has a minimum Hawking temperature; above it large black holes are stable and small ones evaporate, and the nonlinear correction leaves this phase structure intact.