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 possibility of merging gravitational-wave binaries to have an electromagnetic counterpart or having a component in the lower mass-gap region. 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).
  • HasMassGap: The mass of at least one of the compact binary coalescence is consistent with lower mass-gap region i.e. between 3-5 solar mass.

The HasNS and HasRemnant quantities depend 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

1.2.1

1.2.0

1.1.7

1.1.6

1.1.5

1.1.4.post2

1.1.4

1.1.3

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1.1.1

1.1.0

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1.0.2

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0.1.6

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