A1 Journal article (refereed)
Discovery of an Exceptionally Strong β-Decay Transition of 20F and Implications for the Fate of Intermediate-Mass Stars (2019)
Kirsebom, O. S., Jones, S., Strömberg, D. F., Martínez-Pinedo, G., Langanke, K., Röpke, F. K., Brown, B. A., Eronen, T., Fynbo, H. O. U., Hukkanen, M., Idini, A., Jokinen, A., Kankainen, A., Kostensalo, J., Moore, I., Möller, H., Ohlmann, S. T., Penttilä, H., Riisager, K., . . . Äystö, J. (2019). Discovery of an Exceptionally Strong β-Decay Transition of 20F and Implications for the Fate of Intermediate-Mass Stars. Physical Review Letters, 123(26), Article 262701. https://doi.org/10.1103/PhysRevLett.123.262701
JYU authors or editors
Publication details
All authors or editors: Kirsebom, O. S.; Jones, S.; Strömberg, D. F.; Martínez-Pinedo, G.; Langanke, K.; Röpke, F. K.; Brown, B. A.; Eronen, T.; Fynbo, H. O. U.; Hukkanen, M.; et al.
Journal or series: Physical Review Letters
ISSN: 0031-9007
eISSN: 1079-7114
Publication year: 2019
Volume: 123
Issue number: 26
Article number: 262701
Publisher: American Physical Society
Publication country: United States
Publication language: English
DOI: https://doi.org/10.1103/PhysRevLett.123.262701
Publication open access: Not open
Publication channel open access:
Publication is parallel published (JYX): https://jyx.jyu.fi/handle/123456789/67383
Abstract
A significant fraction of stars between 7 and 11 solar masses are thought to become supernovae, but the explosion mechanism is unclear. The answer depends critically on the rate of electron capture on 20Ne in the degenerate oxygen-neon stellar core. However, because of the unknown strength of the transition between the ground states of 20Ne and 20F, it has not previously been possible to fully constrain the rate. By measuring the transition, we establish that its strength is exceptionally large and that it enhances the capture rate by several orders of magnitude. This has a decisive impact on the evolution of the core, increasing the likelihood that the star is (partially) disrupted by a thermonuclear explosion rather than collapsing to form a neutron star. Importantly, our measurement resolves the last remaining nuclear physics uncertainty in the final evolution of degenerate oxygen-neon stellar cores, allowing future studies to address the critical role of convection, which at present is poorly understood.
Keywords: nuclear physics; astrophysics; stars
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Ministry reporting: Yes
Reporting Year: 2019
JUFO rating: 3