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DOE OSTI · 1778739

Light Curves and Spectra from Kilonova Models

Wollaeger, Ryan Thomas
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Abstract

Kilonovae are the radioactively powered optical/IR transients following a binary neutron star or neutron star black hole merger. A broad grid (varying ejecta mass, velocity, composition) of 900 2D kilonova models were simulated with Monte Carlo on Grizzly, using MPI+OpenMP. The set of models are being compared to observation AT2017gfo (the electromagnetic counterpart of gravitational wave GW170817), and hint at potential fidelity improvements.

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BibTeXRIS

Wollaeger, Ryan Thomas. 2021-04-15. Light Curves and Spectra from Kilonova Models. https://doi.org/10.2172/1778739

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