Anisotropic bipolar and equatorial ejecta distributions produce two-peak features in late-time radio light curves that align with main thermal emissions, with non-detections in AT 2017gfo consistent under typical parameters.
D., Piro, A
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Review summarizing the role of dense-matter equation of state, weak interactions, and r-process nucleosynthesis in binary neutron star mergers and their multimessenger observables.
citing papers explorer
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Anisotropic Ejecta from Binary Neutron Star Mergers: Self-Consistent Main Thermal and Late-Time Radio Emission of NS-Powered Kilonovae
Anisotropic bipolar and equatorial ejecta distributions produce two-peak features in late-time radio light curves that align with main thermal emissions, with non-detections in AT 2017gfo consistent under typical parameters.
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Nuclear Physics of Binary Neutron Star Mergers
Review summarizing the role of dense-matter equation of state, weak interactions, and r-process nucleosynthesis in binary neutron star mergers and their multimessenger observables.