Bulletin of the American Physical Society
6th Joint Meeting of the APS Division of Nuclear Physics and the Physical Society of Japan
Sunday–Friday, November 26–December 1 2023; Hawaii, the Big Island
Session 3WDB: Recent Developments in Fission IIInvited Workshop
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Chair: Nathan Giha, University of Michigan Room: Hilton Waikoloa Village Kings 2 |
Monday, November 27, 2023 11:00AM - 11:30AM |
3WDB.00001: Measurement of spontaneous fission of Fm isotopes Invited Speaker: Masato Asai Spontaneous fission (SF) of neutron-rich Fm and transfermium nuclei exhibits various fascinating properties of fission. One of the highlights is the sudden change of fission-fragment mass distribution (FFMD) between 256Fm and 258Fm; the SF of 256Fm shows typical asymmetric mass distribution, while that of 258Fm shows very sharp symmetric one with total-kinetic energy (TKE) much higher than those of the asymmetric fission [1]. This high-TKE symmetric fission is observed only in neutron-rich Fm and Md isotopes, and is interpreted as the fission with compact configuration forming two spherical Sn fragments. Moreover, the SF of neutron-rich No, Lr, and Rf isotopes show another type of fission with low-TKE symmetric mass distribution [1]. This low-TKE symmetric fission competes or coexists with the high-TKE symmetric fission in neutron-rich Fm region. Recent progress in theoretical calculations has enabled to calculate the competition between the asymmetric and the high-TKE symmetric fission as well as their mass and TKE distributions. However, the experimental data to be compared are very limited. In particular, more precise and detailed mass and TKE distribution data are indispensable to understand the fission mechanism in this neutron-rich Fm region. |
Monday, November 27, 2023 11:30AM - 12:00PM |
3WDB.00002: Advances in Fission Product Yield Evaluation and Modeling Invited Speaker: Amy E Lovell Throughout the past several years, there have been significant advances in modeling and experimental measurements for fission product yields. Facilities have been able to measure fission products with increasingly shorter half lives that can be used to constrain calculations that can consistently model both prompt and delayed fission observables. Here, we describe our modeling framework for calculating independent and cumulative fission products along with prompt and delayed neutron and gamma-ray multiplicities and energies. We discuss this work in the context of the larger multi-institute fission product yield evaluation project that combines the consistent modeling with calculations for the underlying fission fragment initial conditions, new measurements, and corrections to historic data. |
Monday, November 27, 2023 12:00PM - 12:30PM |
3WDB.00003: Measurement of prompt γ-ray spectrum for 235U(nth,f) Invited Speaker: Hiroyuki Makii Prompt fission γ-ray spectra (PFGS) are important as they allow us to study the structure and de-excitation process of neutron-rich fission fragments (FFs). They are also required as nuclear data to design new types of reactors, such as the Generation-IV reators. For spontaneous fission of 252Cf, the PFGS show broad structures at around γ-ray energy of 15 MeV, which was explained by incorporating the giant dipole resonance γ-ray emission. For neutron-induced fissions (nth,f), however, no data are available in the energy range higher than 7 MeV. With a goal to measure the PFGS for 235U(nth,f) up to energies of 20 MeV, we have developed a new measurement system. The system consists of two position-sensitive multi-wired proportional counters (MWPCs) to detect both FFs in coincidence, and two large volume LaBr3(Ce) scintillators to measure the γ-rays in fission. The measurement has been carried out at the PF1B cold-neutron facility of the Institut Laue Langevin (ILL), Grenoble, France. Throughout the 437-hour run the total number of recorded γ rays in coincidence with FFs was reached to 1.7x109. The obtained PFGS reached about 20 MeV, high enough to reveal the structure associated with the GDR of the FFs, for the first time in (nth,f). The resulting PFGS do not follow the linearly decreasing trend as a function of γ-ray energy in logarithmic scale, but reveal the bump structures at about 4 MeV, 6 MeV, and 15 MeV. In this contribution, we will discuss the origins of the bump structures in comparison with the statistical Hauser-Freshbach model calculation. |
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