Numerical simulations of black-hole binaries and gravitational wave emission
Ulrich Sperhake, Emanuele Berti, Vitor Cardoso
TL;DR
This paper reviews recent advances in numerical relativity simulations of black-hole spacetimes, focusing on gravitational wave sources, astrophysical systems, and high-energy physics applications.
Contribution
It provides a comprehensive summary of recent progress and identifies urgent future tasks in numerical relativity related to black holes.
Findings
Black-hole mergers as gravitational wave sources
Insights into astrophysical black-hole systems
Applications of black holes in high-energy physics
Abstract
We review recent progress in numerical relativity simulations of black-hole (BH) spacetimes. Following a brief summary of the methods employed in the modeling, we summarize the key results in three major areas of BH physics: (i) BHs as sources of gravitational waves (GWs), (ii) astrophysical systems involving BHs, and (iii) BHs in high-energy physics. We conclude with a list of the most urgent tasks for numerical relativity in these three areas.
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