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kuibit: Analyzing Einstein Toolkit simulations with Python

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arxiv 2104.06376 v1 pith:PYOIWLZB submitted 2021-04-13 gr-qc astro-ph.HE

classification gr-qcastro-ph.HE
keywords kuibiteinsteincodedataseriestoolkitanalyzingequations
verification ladder T0 review T1 audit T2 compute T3 formal
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In the era of gravitational-wave astronomy, general-relativistic simulations of compact objects play a role of paramount importance. These calculations can be performed with the Einstein Toolkit, an open-source and community-supported software for numerical-relativity and relativistic astrophysics. The code comes with multiple solvers for Einstein's equations and for the equations of general-relativistic magneto-hydrodynamics, along with a series of useful diagnostics. However, analyzing the output of the Einstein Toolkit can be a challenging task. Usually, the process involves a series of technical obstacles, like combining data from different restarts or working with HDF5 files. Here, we present kuibit, a Python library that takes care of all these low-level details (and many other more) and that provides high-level, intuitive, representations of the data. Kuibit ships with a wide range of features that include full support for 1-3D ASCII and HDF5 grid data, time and frequency series, gravitational waves, and apparent horizons. With kuibit, users can inspect most of the content of a simulation with just a few lines of code. Importantly, kuibit is designed to be a code for the community: it is user-friendly and does not require any proprietary software to run, it has documentation and examples, and it is openly developed with emphasis on extensibility and maintainability.

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Cited by 2 Pith papers

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  1. Gravitational Wave Modeling of White-Dwarf--Compact-Object Binaries and Observational Outlook

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    WD–CO binaries produce unique GW waveforms with a sharp f_max cutoff; LGWA/DECIGO will detect many end stages, while terrestrial detectors will not mistake them for sub-solar compact objects.

  2. High-Density Sound Speed and Post-Merger Dynamics

    astro-ph.HE 2026-07 conditional novelty 5.0 of 10

    The slope of the high-density sound-speed curve shifts the post-merger gravitational-wave peak frequency and ejecta mass, and that peak frequency partially correlates with an integrated 'intrinsic tidal response' — bu...

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