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Product yields for the photo-fission of 209Bi with 2.5 GeV bremsstrahlung
The mass-yield distribution of fission products in the 2.5 GeV bremsstrahlung-induced fission of 209Bi have been determined by using the recoil catcher and the off-line γ-spectrometry technique in the high energy electron linac at the Pohang Accelerator Laboratory. The mass-yield determination invol...
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Published in: | Nuclear instruments & methods in physics research. Section B, Beam interactions with materials and atoms Beam interactions with materials and atoms, 2009-06, Vol.267 (11), p.1891-1898 |
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Main Authors: | , , , , , , , , , , , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The mass-yield distribution of fission products in the 2.5
GeV bremsstrahlung-induced fission of
209Bi have been determined by using the recoil catcher and the off-line γ-spectrometry technique in the high energy electron linac at the Pohang Accelerator Laboratory. The mass-yield determination involves the measurements of cumulative yields for 32 fission products and independent yields of 17 fission products in the photo-fission of
209Bi nuclei. It was found that the mass-yield distribution of fission products in
209Bi is symmetric with an average mass of 95
±
0.5 and a FWHM of 51
±
2.0 mass units. Present data at 2.5
GeV along with the literature data at 1
GeV, 700–600
MeV, and 85–28
MeV were interpreted from the point of increase of multi-chance fission and multi-nucleon emission probabilities with an increase in excitation energy. It was found that the average mass of the mass-yield distribution of the fission products decreases from 103
±
0.5 at 28–85
MeV to 95
±
0.5 at 2.5
GeV. On the other hand, the FWHM of the mass-yield distribution increases from 19 mass units at 28–40
MeV to 51 mass units at 2.5
GeV. It was also found that the nuclear structure effect observed at the photo-fission of
209Bi with 28–85
MeV bremsstrahlung is washed out at higher energy. |
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ISSN: | 0168-583X 1872-9584 |
DOI: | 10.1016/j.nimb.2009.04.001 |