Abundance of live 244Pu in deep-sea reservoirs on Earth points to rarity of actinide nucleosynthesis View Full Text


Ontology type: schema:ScholarlyArticle      Open Access: True


Article Info

DATE

2015-01-20

AUTHORS

A. Wallner, T. Faestermann, J. Feige, C. Feldstein, K. Knie, G. Korschinek, W. Kutschera, A. Ofan, M. Paul, F. Quinto, G. Rugel, P. Steier

ABSTRACT

Half of the heavy elements including all actinides are produced in r-process nucleosynthesis, whose sites and history remain a mystery. If continuously produced, the Interstellar Medium is expected to build-up a quasi-steady state of abundances of short-lived nuclides (with half-lives ≤100 My), including actinides produced in r-process nucleosynthesis. Their existence in today's interstellar medium would serve as a radioactive clock and would establish that their production was recent. In particular (244)Pu, a radioactive actinide nuclide (half-life=81 My), can place strong constraints on recent r-process frequency and production yield. Here we report the detection of live interstellar (244)Pu, archived in Earth's deep-sea floor during the last 25 My, at abundances lower than expected from continuous production in the Galaxy by about 2 orders of magnitude. This large discrepancy may signal a rarity of actinide r-process nucleosynthesis sites, compatible with neutron-star mergers or with a small subset of actinide-producing supernovae. More... »

PAGES

5956

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/ncomms6956

DOI

http://dx.doi.org/10.1038/ncomms6956

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1033800809

PUBMED

https://www.ncbi.nlm.nih.gov/pubmed/25601158


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