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Gravitational collapse to regular black holes

Ottobre 10, 2022 @ 11:30 am - 12:30 pm

DATE: Monday, October 10, 11:30 a.m.


LOCATION: AULA OVEST (INAF-OACT) – Audience in-person max 20

Link for the remote audience:

SPEAKER: Dott. Daniele Malafarina (Nazarbayev University)

The Oppenheimer-Snyder-Datt model for homogeneous dust collapse describes how a black hole forms. Considering semi-classical corrections at large curvature obtained from general relativity coupled to non-linear electrodynamics may lead to the resolution of the central singularity and the formation of a regular black hole.


A few rules:
— access the virtual room with the microphone and camera switched off.
— for questions leave a message in the chat and the answers at the end of the webinar.


Ottobre 10, 2022
11:30 am - 12:30 pm
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