Abstract
We perform numerical simulations of the approach to spacetime singularities. The simulations are done with sufficient resolution to resolve the small scale features (known as spikes) that form in this process. We find an analytical formula for the shape of the spikes and show that the spikes in the simulations are well described by this formula.
Original language | English (US) |
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Article number | 124067 |
Journal | Physical Review D |
Volume | 102 |
Issue number | 12 |
DOIs | |
State | Published - Dec 29 2020 |
All Science Journal Classification (ASJC) codes
- Physics and Astronomy (miscellaneous)