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