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Possible use of accelerator driven subcritical reactors for minor actinides incineration

Authors :
H. Nifenecker
Sylvain David
O Meplan
Laboratoire de Physique Subatomique et de Cosmologie (LPSC)
Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS)
Institut de Physique Nucléaire d'Orsay (IPNO)
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 :
Comptes Rendus de l'Academie des Sciences. Série IV, Physique, Astronomie, Comptes Rendus de l'Academie des Sciences. Série IV, Physique, Astronomie, Elsevier, 2001, 2, pp.163-184. ⟨10.1016/S1296-2147(00)01146-X⟩
Publication Year :
2001
Publisher :
HAL CCSD, 2001.

Abstract

The possible interest of accelerator driven subcritical reactors for minor actinides incineration is examined. The physics of neutron multiplying systems is recalled. The differences between critical and subcritical reactors' control are described, with emphasis on the importance of the delayed neutrons fraction. The minor actinides fuel evolution is studied with the conclusion that fast neutron spectra are clearly more efficient then thermal neutron spectra. It is, also, shown that characteristic times for incineration should be in the order of 10 years. The number of minor actinides incinerators necessary for 60 PWRs is estimated to be about 6 with total thermal power of 9 GW. These reactors will, also, be able to transmute essentially all 99 Tc and 129 I produced by the 60 PWR. The excess electricity cost for MA incineration is estimated to be about 5%.

Details

Language :
English
Database :
OpenAIRE
Journal :
Comptes Rendus de l'Academie des Sciences. Série IV, Physique, Astronomie, Comptes Rendus de l'Academie des Sciences. Série IV, Physique, Astronomie, Elsevier, 2001, 2, pp.163-184. ⟨10.1016/S1296-2147(00)01146-X⟩
Accession number :
edsair.doi.dedup.....9c26f9336c8386a87ec9aebee1b26d17
Full Text :
https://doi.org/10.1016/S1296-2147(00)01146-X⟩