Evaporating black-to-white hole

Pierre Martin-Dussaud (1) , Carlo Rovelli (1)

1 CPT - Centre de Physique Théorique - UMR 7332

We construct and discuss the form of the (effective) spacetime geometry inside a black hole undergoing a quantum transition to a white hole, taking into account the back-reaction of the component of the Hawking radiation falling into the hole.

Mots clés: space-time: geometry; radiation: Hawking; back reaction; black hole: evaporation; effect: quantum

Domaines: Relativité Générale et Cosmologie Quantique [gr-qc]

Pierre Martin-Dussaud, Carlo Rovelli. Evaporating black-to-white hole. 2024. ⟨hal-02148273⟩