Possibility and properties of Electromagnetically-bright sources of gravitational-wave events

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  • License: MIT License (MIT)
  • Author: Deep Chatterjee
  • Requires: Python >=3.8, <4.0
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ligo.em_bright

This library provides the tools to compute the possibilty of merging gravitational-wave binaries to have an electromagnetic counterpart. The data products are source properties

  • HasNS: The mass of at least one of the compact binary coalescence is consistent with a neutron star.
  • HasRemnant: A non-zero amount of remnant matter remained outside the final compact object (a necessary but not sufficient condition to produce certain kinds of electromagnetic emission such as a short GRB or a kilonova).

Both quantities depends on, and are marginalized over several neutron star equations of state (EOS). The marginalization is done using data from GW170817.

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Avatar for andrew.toivonen from gravatar.com andrew.toivonen Avatar for deep.chatterjee from gravatar.com deep.chatterjee Avatar for frenbox from gravatar.com frenbox

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  • License: MIT License (MIT)
  • Author: Deep Chatterjee
  • Requires: Python >=3.8, <4.0
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1.2.2

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