Carlo Rovelli

Physics with non-perturbative quantum gravity: the end of the Hawking evaporation

Physics & Hype

Measuring Quantum Discreteness of Time in the Lab with Gravity Entanglement Interference

What happens at the end of Hawking's evaporation?

Covariant Loop Quantum Gravity, the State of the Art

A possible quantum gravity observation. Cosmic rays from Planck stars: black holes decay via tunneling.

Emergent Time Discussion

• Carlo Rovelli Centre de Physique Théorique

• Jenann Ismael Columbia University

• Andreas Albrecht University of California System

Black hole decay and Fast Radio Bursts

Promising Paths: What Have We Learned So Far About Quantum Gravity?

• Abhay Ashtekar Pennsylvania State University

• Carlo Rovelli Centre de Physique Théorique

Explorations in Quantum Gravity - Lecture 14