The dust needed to explain GRB 230307A's infrared continuum is not produced in any tested kilonova nucleosynthesis model, so the continuum is either not dust or the burst is not a binary neutron-star merger.
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GRB 230307A Formed No Dust or Was Not a Binary Neutron Star Merger
The dust needed to explain GRB 230307A's infrared continuum is not produced in any tested kilonova nucleosynthesis model, so the continuum is either not dust or the burst is not a binary neutron-star merger.