Numerical simulations of compact object binaries
Harald P. Pfeiffer
TL;DR
This paper reviews recent progress in numerical simulations of coalescing compact object binaries, which are key sources for gravitational wave detection.
Contribution
It provides an overview of the current state and advancements in simulating black hole and neutron star binaries.
Findings
Recent simulation techniques have improved accuracy
Simulations have enhanced understanding of gravitational wave signals
Progress has been made in modeling binary mergers
Abstract
Coalescing compact object binaries consisting of black holes and/or Neutron stars are a prime target for ground-based gravitational wave detectors. This article reviews the status of numerical simulations of these systems, with an emphasis on recent progress.
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