In neutron star merger ejecta simulations, coupling in-situ nuclear networks with composition-dependent thermalization and frequency-dependent opacities changes nucleosynthesis yields, delays and reddens early emission, and produces brighter, bluer kilonovae than simplified analytic prescriptions.
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Impact of in situ nuclear networks and atomic opacities on neutron star merger ejecta dynamics, nucleosynthesis, and kilonovae
In neutron star merger ejecta simulations, coupling in-situ nuclear networks with composition-dependent thermalization and frequency-dependent opacities changes nucleosynthesis yields, delays and reddens early emission, and produces brighter, bluer kilonovae than simplified analytic prescriptions.