28 July 2024 to 3 August 2024
Europe/London timezone

Observing black hole features in the collapsed phase of EDT

30 Jul 2024, 18:15
1h
Poster Theoretical Developments Poster session and reception

Speaker

Jan Smit (University of Amsterdam)

Description

Propagators of massless scalar fields have been computed on configurations of Euclidean dynamical triangulations (EDT) in the collapsed phase. They are used to calculate -- up to an integration constant -- the scale factor of a rotational invariant metric. This scale factor is non-zero at the origin, which we assume to be caused by the presence of the well-known singular structure in the collapsed phase. A transformation to a metric in (1+3)-dimensions reveals Euclidean black hole features at an instant in time, with a horizon separating interior and exterior parts. Assuming effective Einstein equations, the energy and pressure of a `geometric condensate' are computed with the software OGRe. arXiv [gr-qc] 2301.07081 and 2305.16011

Primary author

Jan Smit (University of Amsterdam)

Presentation materials

There are no materials yet.