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The i-process and CEMP-r/s stars

We showed that the observed abundances of heavy elements in CEMP-r/s stars could be reproduced surprisingly well in simple one-zone simulations of i-process nucleosynthesis.

Project summary

Distributions of heavy-element abundances obtained in one-zone simulations of i-process nucleosynthesis for different neutron exposures are fitted to the observed chemical composition of CEMP-r/s stars.

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Refereed NIC XIII paper

Proceedings of XIII Nuclei in the Cosmos (NIC XIII). 7-11 July, 2014. Debrecen, Hungary.

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