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• W3133986019 abstract "Gravitational waves emitted from the coalescence of neutron star binaries open a new window to probe matter and fundamental physics in unexplored, extreme regimes. To extract information about the supranuclear matter inside neutron stars and the properties of the compact binary systems, robust theoretical prescriptions are required. We give an overview about general features of the dynamics and the gravitational wave signal during the binary neutron star coalescence. We briefly describe existing analytical and numerical approaches to investigate the highly dynamical, strong-field region during the merger. We review existing waveform approximants and discuss properties and possible advantages and shortcomings of individual waveform models, and their application for real gravitational-wave data analysis." @default.
• W3133986019 created "2021-03-15" @default.
• W3133986019 creator A5001801624 @default.
• W3133986019 creator A5011726392 @default.
• W3133986019 creator A5063256945 @default.
• W3133986019 date "2021-03-01" @default.
• W3133986019 modified "2023-10-18" @default.
• W3133986019 title "Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections" @default.
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