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Interpreting Binary Neutron Star Mergers: Describing the Binary Neutron Star Dynamics, Modelling Gravitational Waveforms, and Analyzing Detections

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arxiv 2004.02527 v1 pith:L57VYKKN submitted 2020-04-06 gr-qc astro-ph.COastro-ph.HE

Tim Dietrich , Tanja Hinderer , Anuradha Samajdar This is my paper
classification gr-qcastro-ph.COastro-ph.HE
keywords neutronbinarystargravitationalcoalescenceduringdynamicsexisting
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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.

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Cited by 4 Pith papers

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    Future high-frequency-sensitive GW detectors can distinguish binary neutron star from low-mass black hole mergers in late phases, enabling separation of merger rates and constraints on heavy non-annihilating dark matt...

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