Speaker
Sebastian Murk
(Macquarie University and Sydney Quantum Academy)
Description
In spherical symmetry, only two classes of dynamic solutions to the semiclassical Einstein equations describe physical black holes, and their formation follows a unique scenario. To be compatible with their existence, modified gravity theories must satisfy several constraints.
Primary author
Sebastian Murk
(Macquarie University and Sydney Quantum Academy)
Co-author
Prof.
Daniel R. Terno
(Macquarie University)
