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Effects of the nuclear structure of fission fragments on the high-energy prompt fission $\gamma$-ray spectrum in $^{235}\mathrm{U}({n}_{\mathrm{th}},f)$

Authors :
Makii, H.
Nishio, K.
Hirose, K.
Orlandi, R.
Léguillon, R.
Ogawa, T.
Soldner, T.
Köster, U.
Pollitt, A.
Hambsch, F.J.
Tsekhanovich, I.
Aïche, M.
Czajkowski, S.
Mathieu, L.
Petrache, C.M.
Astier, A.
Guo, S.
Ohtsuki, T.
Sekimoto, S.
Takamiya, K.
Frost, R.J.W.
Kawano, T.
Institut Laue-Langevin (ILL)
ILL
Centre d'Etudes Nucléaires de Bordeaux Gradignan (CENBG)
Université Sciences et Technologies - Bordeaux 1-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Centre de Sciences Nucléaires et de Sciences de la Matière (CSNSM)
Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11)
Source :
Phys.Rev.C, Phys.Rev.C, 2019, 100 (4), pp.044610. ⟨10.1103/PhysRevC.100.044610⟩, Physical Review C, Physical Review C, American Physical Society, 2019, 100 (4), pp.044610. ⟨10.1103/PhysRevC.100.044610⟩
Publication Year :
2019
Publisher :
HAL CCSD, 2019.

Abstract

International audience; The prompt fission γ-ray energy spectrum for cold-neutron-induced fission of U235 was measured in the energy range Eγ=0.8–20MeV, by gaining a factor of about 105 in statistics compared to the measurements performed so far. The spectrum exhibits local bump structures at Eγ≈4MeV and ≈6MeV, and also a broad one at ≈15MeV. In order to understand the origins of these bumps, the γ-ray spectra were calculated using a statistical Hauser-Feshbach model, taking into account the deexcitation of all the possible primary fission fragments. It is shown that the bump at ≈4MeV is created by the transitions between the discrete levels in the fragments around Sn132, and the bump at ≈6MeV mostly comes from the complementary light fragments. It is also indicated that a limited number of nuclides, which have high-spin states at low excitation energies, can contribute to the bump structure around Eγ≈15MeV, induced by the transition feeding into the low-lying high-spin states.

Details

Language :
English
ISSN :
24699985 and 24699993
Database :
OpenAIRE
Journal :
Phys.Rev.C, Phys.Rev.C, 2019, 100 (4), pp.044610. ⟨10.1103/PhysRevC.100.044610⟩, Physical Review C, Physical Review C, American Physical Society, 2019, 100 (4), pp.044610. ⟨10.1103/PhysRevC.100.044610⟩
Accession number :
edsair.dedup.wf.001..dc1e418c4d48af6eaeb9a395093a4c4e