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Photofission of 197Au and 209Bi at intermediate energies

  • Session 2: Nuclear Analytical Methods
  • Published:
Czechoslovak Journal of Physics Aims and scope

Abstract

Recoil properties and yields of radionuclides formed in the photofission of 197Au and 209Bi by bremsstrahlung of end-point energies (E 0) from 300 to 1100 MeV have been investigated using the thick-target thick-catcher method. The kinetic energies T of the residual nuclei were deduced based on the two-step vector model and discussed by comparing with the reported results on protoninduced reactions as well as those on photospallation. The charge distribution was reproduced by a Gaussian function with the most probable charge Zp expressed by a linera function of the product mass number A and with the A-independent width FWHM CD. Based on the charge distribution parameters, the symmetric mass yield distribution with the most probable mass A p of 92 m.u. and the width FWHM MD of 39 m.u. was obtained for 197Au at E 0≥600 MeV. The A p value for 209Bi was larger by 4 m.u. than that for 197Au and the FWHM MD was smaller by 6 m.u. A comparison with the calculations using the Photon-induced Intranuclear Cascade Analysis 3 code combined with the Generalized Evaporation Model code (PICA3/GEM) was also performed.

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Haba, H., Sakamoto, K., Igarashi, M. et al. Photofission of 197Au and 209Bi at intermediate energies. Czech J Phys 53 (Suppl 1), A265–A271 (2003). https://doi.org/10.1007/s10582-003-0034-7

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  • DOI: https://doi.org/10.1007/s10582-003-0034-7

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