2017
DOI: 10.1051/epjconf/201714604036
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Measurement of high-energy prompt gamma-rays from neutron induced fission of U-235

Abstract: Abstract.We have developed a new setup to measure prompt γ -rays from the 235 U(n th , f ) reaction. The setup consists of two multi-wire proportional counters (MWPCs) to detect the fission fragments, two LaBr 3 (Ce) scintillators to measure the γ -rays. The highly efficient setup was installed at the PF1B beam line of the Institut Laue Langevin (ILL). We have successfully measured the γ -ray spectrum up to about 20 MeV for the fist time in neutron-induced fission.

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Cited by 6 publications
(10 citation statements)
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References 17 publications
(16 reference statements)
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“…60 Therefore, it is important to evaluate the potential contribution of γ-rays to the observed NC scintillation. The calculated γ-ray attenuation cross sections σ γ-ray of the NCs scintillator materials, averaged with respect to the prompt gamma ray spectrum of 235 U, 5,61 range from 0.14 cm 2 /g in CuInS 2 to 0.28 cm 2 /g for FAPbBr 3 and CsPbBr 3 (Table 1), consistent with the photon stopping power provided by the high Pb content of the latter compounds. The attenuation coefficients a γ-ray of these NC samples, which account for the concentration by dividing by the NC density in the colloidal solution, vary from 0.2 × 10 −3 cm −1 for the more dilute CsPbBrCl 2 :Mn NCs to 9.8 × 10 −3 cm −1 for the more concentrated CsPbBr 3 NCs (Table 1).…”
Section: Resultssupporting
confidence: 65%
“…60 Therefore, it is important to evaluate the potential contribution of γ-rays to the observed NC scintillation. The calculated γ-ray attenuation cross sections σ γ-ray of the NCs scintillator materials, averaged with respect to the prompt gamma ray spectrum of 235 U, 5,61 range from 0.14 cm 2 /g in CuInS 2 to 0.28 cm 2 /g for FAPbBr 3 and CsPbBr 3 (Table 1), consistent with the photon stopping power provided by the high Pb content of the latter compounds. The attenuation coefficients a γ-ray of these NC samples, which account for the concentration by dividing by the NC density in the colloidal solution, vary from 0.2 × 10 −3 cm −1 for the more dilute CsPbBrCl 2 :Mn NCs to 9.8 × 10 −3 cm −1 for the more concentrated CsPbBr 3 NCs (Table 1).…”
Section: Resultssupporting
confidence: 65%
“…60 Therefore, it is important to evaluate the potential contribution of γ-rays to the observed NC scintillation. The calculated γ-ray attenuation cross sections σ γ-ray of the NCs scintillator materials, averaged with respect to the prompt gamma ray spectrum of 235 U, 5,61 range from 0.14 cm 2 /g in CuInS 2 to 0.28 cm 2 /g for FAPbBr 3 and CsPbBr 3 (Table 1), consistent with the photon stopping power provided by the high Pb content of the latter compounds. The attenuation coefficients a γ-ray of these NC samples, which account for the concentration by dividing by the NC density in the colloidal solution, vary from 0.2 × 10 −3 cm −1 for the more dilute CsPbBrCl 2 :Mn NCs to 9.8 × 10 −3 cm −1 for the more concentrated CsPbBr 3 NCs (Table 1).…”
Section: Acs Nano Wwwacsnanoorgsupporting
confidence: 64%
“…The blocking experiment implemented for the spatial resolution provides a modulated light yield due to neutron and gamma attenuation of the metal blocks, thus the ratio R b of the light intensity in the blocked and unblocked regions can be used to estimate the gamma sensitivity. This ratio can be expressed as Gamma attenuation coefficients of the metal blocks were averaged with respect to the 235 U γ-ray spectrum, 61 while the fast neutron attenuation coefficients were estimated using the calculated neutron fission spectrum. 11 Note that these values will overestimate the neutron stopping power due to the lower average energy of the calculated fission neutron spectrum (1.…”
Section: Acs Nano Wwwacsnanoorgmentioning
confidence: 99%
“…Delayed γ lines starting from the prompt γ peak can also be seen, and are associated with isomeric decays of particular fission fragments, e.g., 1769 keV γ line with lifetime 54 ns can be a candidate for 146 Ce [23]. Other lines originate from neutron inelastic scattering (n, n ′ γ ) on materials inside the detectors, e.g., γ -ray decay of the first excited states of 139 La (165.86 keV), 79 Br (217.07 keV), and 81 Br (275.99 keV), or materials close to the γ detectors and the ionization chamber, e.g., γ -ray decay of the first excited states of 27 Al (843.76 keV) and 56 Fe (846.78 keV). A continuous γ background exists along the whole axis associated with uncorrelated decays in FIG.…”
Section: B Pfg Selectionmentioning
confidence: 99%
“…The latter cover a wide range of energies from a few tens keV up to 10 MeV. At even higher energies, the deexcitation of giant resonance (GR) of the fragments may be observed [26,27]. In the case of fast-neutron-induced fission, where the cross section is three orders of magnitude lower than thermal-neutron-induced fission, the limited statistics above 6 MeV constrain the study of high-energy γ rays (see Fig.…”
Section: Emission Spectrum Shapementioning
confidence: 99%