Heavy Exotic Nuclei for Nuclear Astrophysics (HENNA)

Description of the granted funding

The origin of chemical elements heavier than iron is not yet fully understood. Around half of the heavy-element abundances beyond iron have been created by the rapid neutron capture process, the r process, taking place at least in binary neutron star mergers. In order to model the r process, precise data on nuclear masses are needed. In this project, we will produce heavy exotic nuclei in the JYFL-ACCLAB Accelerator Laboratory at the University of Jyväskylä and study their masses using novel techniques and instrumentation. Experiments at international radioactive beam facilities, such as ISOLDE at CERN and GSI/FAIR, will yield complementary data on masses of neutron-rich nuclei. Masses of several previously unknown, or poorly known nuclei and their long-lived excited states, isomers, will be measured. The results will be compared to state-of-the-art nuclear models and their impact on the r process will be studied in detail.
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Starting year

2023

End year

2027

Granted funding

Anu Kankainen Orcid -palvelun logo
584 970 €

Funder

Research Council of Finland

Funding instrument

Academy projects

Decision maker

Scientific Council for Natural Sciences and Engineering
06.06.2023

Other information

Funding decision number

354968

Fields of science

Physical sciences

Research fields

Hiukkas- ja ydinfysiikka

Identified topics

nuclear safety, nuclear reactors