• Corpus ID: 252668889

Proposed Lunar Measurements of $r$-Process Radioisotopes to Distinguish Origin of Deep-sea 244Pu

@inproceedings{Wang2021ProposedLM,
  title={Proposed Lunar Measurements of \$r\$-Process Radioisotopes to Distinguish Origin of Deep-sea 244Pu},
  author={Xilu Wang and Adam M. Clark and John Ellis and Adrienne F. Ertel and Brian D. Fields and Brian J. Fry and Zhenghai Liu and Jesse A. Miller and Rebecca Surman},
  year={2021}
}
244 Pu has recently been discovered in deep-sea deposits spanning the past 10 Myr, a period that includes two 60 Fe pulses from nearby supernovae. 244 Pu is among the heaviest r -process products, and we consider whether it was created in the supernovae, which is disfa-vored by nucleosynthesis simulations, or in an earlier kilonova event that seeded 244 Pu in the nearby interstellar medium that was subse-quently swept up by the supernova debris. We discuss how these possibilities can be probed… 

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