Anomalies in the Charge Yields of Fission Fragments from the U ( n , f ) 238 Reaction
Fast-neutron-induced fission of 238U at an energy just above the fission threshold is studied with a novel technique which involves the coupling of a high-efficiency γ-ray spectrometer (MINIBALL) to an inverse-kinematics neutron source (LICORNE) to extract charge yields of fission fragments via γ-γ...
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| Published in: | Physical review letters Vol. 118; no. 22 |
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
United States
American Physical Society (APS)
01.06.2017
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| Subjects: | |
| ISSN: | 0031-9007, 1079-7114 |
| Online Access: | Get full text |
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| Summary: | Fast-neutron-induced fission of 238U at an energy just above the fission threshold is studied with a novel technique which involves the coupling of a high-efficiency γ-ray spectrometer (MINIBALL) to an inverse-kinematics neutron source (LICORNE) to extract charge yields of fission fragments via γ-γ coincidence spectroscopy. Experimental data and fission models are compared and found to be in reasonable agreement for many nuclei; however, significant discrepancies of up to 600% are observed, particularly for isotopes of Sn and Mo. This indicates that these models significantly overestimate the standard 1 fission mode and suggests that spherical shell effects in the nascent fission fragments are less important for low-energy fast-neutron-induced fission than for thermal neutron-induced fission. Finally, this has consequences for understanding and modeling the fission process, for experimental nuclear structure studies of the most neutron-rich nuclei, for future energy applications (e.g., Generation IV reactors which use fast-neutron spectra), and for the reactor antineutrino anomaly. |
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| Bibliography: | USDOE Science and Technology Facilities Council (STFC), UK AC52-07NA27344; 05P15PKCIA; 222287 LLNL-JRNL-737167 Research Council of Norway |
| ISSN: | 0031-9007 1079-7114 |
| DOI: | 10.1103/PhysRevLett.118.222501 |