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Numerical Inside View of Hypermassive Remnant Models for GW170817 supplemental data

Research datakeyboard_double_arrow_right Dataset 01 Mar 2021Publisher:Zenodo
Authors: Kastaun, Wolfgang; Ohme, Frank;

doi: 10.5281/zenodo.4968764 , 10.5281/zenodo.4570825 , 10.5281/zenodo.4570824

Numerical Inside View of Hypermassive Remnant Models for GW170817 supplemental data

Abstract

This archive contains gravitational waveform data discussed in the article Wolfgang Kastaun, Frank Ohme, "Numerical Inside View of Hypermassive Remnant Models for GW170817" (2021) It was extracted from numerical simulations using the SFHO EOS and the chirp mass inferred for GW170817, using two mass ratios 1 and 0.9. Both the raw numerical waveform and a hybridized waveform are provided. The data format is described in the README file.

Changes in 1.1: improved README file

Related Organizations
Keywords

Numerical relativity, Gravitational waves, Neutron stars

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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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