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arxiv: gr-qc/0606135 · v1 · submitted 2006-06-30 · 🌀 gr-qc

Boosted Kerr black hole

classification 🌀 gr-qc
keywords blackboostedholekerrnumericallyadoptedalgorithmsapparent
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Initial data for boosted Kerr black hole are constructed in an axially symmetric case. Momentum and hamiltonian constraints are solved numerically using finite element method (FEM) algorithms. Both Bowen-York and puncture boundary conditions are adopted and appropriate results are compared. Past and future apparent horizons are also found numerically and the Penrose inequality is tested in detail.

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  1. General Boosted Black Holes: A First Approximation

    gr-qc 2025-08 unverdicted novelty 5.0

    An approximate solution for a general boosted Kerr-Newman black hole is derived from a BMS twisting metric, shown to satisfy Einstein equations up to 1/r^4, with analysis of horizons, ergosphere, and electromagnetic f...