CORDIS Project
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This research focuses on understanding the dynamics of spinning black holes in the presence of matter. It aims to explore the interactions between matter and the rotation of spacetime, contributing to our knowledge of black hole stability and implications for various fields of physics.
Black holes (BHs), where gravity is strongest in the universe, are the objects where we must confront the most extreme phenomena predicted by general relativity (GR) and extensions thereof.
As for the majority of astrophysical bodies, BHs are typically spinning.
However, addressing rotation in GR is notoriously difficult.
Moreover, BHs are ‘dirty’: they are accompanied by clouds of gas or accretion disks, which introduce deviations from the known vacuum solutions.
The complexity of the Einstein…
UNIVERSITAT DE BARCELONA
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