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arXiv · 2509.03003

Kilonovae and Long-duration Gamma-ray Bursts

Marko Ristić·Brandon L. Barker·Samuel Cupp·Axel Gross·Nicole Lloyd-Ronning·Oleg Korobkin·Jonah M. Miller·Matthew R. Mumpower
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Abstract

Recent detections of kilonova-like emission following long-duration gamma-ray bursts GRB211211A and GRB230307A have been interpreted as originating from the merger of two neutron stars. In this work, we demonstrate that these observations are also consistent with nucleosynthesis originating from a collapsar scenario. Our model accurately predicts the observed optical and infrared light curves using a single weak $r$-process component. The absence of lanthanide-rich material in our model, consistent with the data, challenges the prevailing interpretation that a red evolution in such transients necessarily indicates the presence of heavy $r$-process elements.

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Marko Ristić, Brandon L. Barker, Samuel Cupp, Axel Gross, Nicole Lloyd-Ronning, Oleg Korobkin, Jonah M. Miller, Matthew R. Mumpower. 2025-09-03. Kilonovae and Long-duration Gamma-ray Bursts. https://arxiv.org/abs/2509.03003

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