We report on the development of a lattice formalism for studying the real time behavior of radially symmetric configurations of massless scalar fields in radially symmetric, curved space times in 3+1 dimensions.
It is intended to numerically study back reaction effects due to semiclassical gravity in the time evolution of scalar field configurations, especially for those that will eventually evolve into black holes.
Volume 430 -
The 39th International Symposium on Lattice Field Theory (LATTICE2022) -
Theoretical Developments
Real time evolution of scalar fields in semiclassical gravity
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Pre-published on:
February 26, 2023
Published on:
April 06, 2023
Abstract
DOI: https://doi.org/10.22323/1.430.0391
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Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.