Two physical characteristics of numerical apparent horizons
classification
🌀 gr-qc
keywords
apparenthorizonsnumericalarticlecharacteristicscharacterizeclosedescribed
read the original abstract
This article translates some recent results on quasilocal horizons into the language of $(3+1)$ general relativity so as to make them more useful to numerical relativists. In particular quantities are described which characterize how quickly an apparent horizon is evolving and how close it is to either equilibrium or extremality.
This paper has not been read by Pith yet.
discussion (0)
Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.