9–11 avr. 2025
Observatoire de Paris - Site de Meudon
Fuseau horaire Europe/Paris

Black Holes in modified gravity theories

11 avr. 2025, 13:45
15m
Amphithéâtre Evry Schatzman (Observatoire de Paris - Site de Meudon)

Amphithéâtre Evry Schatzman

Observatoire de Paris - Site de Meudon

Observatoire de Paris - Site de Meudon 5, place Jules Janssen 92195 MEUDON
Oral presentation Astrophysics Session 10

Orateur

Hugo Candan (LUTH, Observatoire de Paris PSL & IJCLab, Université Paris-Saclay)

Description

The search for alternative theories of gravity is motivated by several considerations, such as Dark Energy, or the existence of singularities in General Relativity. A general subclass of modified gravity theories are scalar-tensor theories, which have been developed in the last decades. It is rather interesting to search for observables that could constrain those theories. Black Holes are objects with extreme gravitational field, making them very suitable for testing gravity theories, and so are in the scope of this work. The goal of the work presented is to find new Black Hole solutions in scalar-tensor theories, which might differ from the unique Kerr Black Hole of General Relativity. With the upcoming of high precision detectors such as LISA, or Einstein Telescope, we will have the observational tools required to assess whether or not real Black Holes are compatible with General Relativity, or with the ones of alternative theories.

Astrophysics Field Compact Objects / theory

Author

Hugo Candan (LUTH, Observatoire de Paris PSL & IJCLab, Université Paris-Saclay)

Documents de présentation

Aucun document.