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

Other information

Funding decision number

354968

Fields of science

Physical sciences

Research fields

Hiukkas- ja ydinfysiikka

Identified topics

nuclear safety, nuclear reactors