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High-energy quasi-monoenergetic neutron fields: existing facilities and future needs
S. Pomp, DT. Bartlett, S. Mayer, G. Reitz, S. Röttger, M. Silari, FD. Smit, H. Vincke, H. Yasuda,
Jazyk angličtina Země Velká Británie
Typ dokumentu časopisecké články, práce podpořená grantem
PubMed
24153422
DOI
10.1093/rpd/nct259
Knihovny.cz E-zdroje
- MeSH
- částice - urychlovače * MeSH
- dávka záření MeSH
- neutrony MeSH
- počítačová simulace MeSH
- protony MeSH
- radiační ochrana metody MeSH
- radiometrie metody MeSH
- spektrofotometrie metody MeSH
- Publikační typ
- časopisecké články MeSH
- práce podpořená grantem MeSH
- Geografické názvy
- Česká republika MeSH
- Francie MeSH
- Japonsko MeSH
- Jihoafrická republika MeSH
- Švédsko MeSH
The argument that well-characterised quasi-monoenergetic neutron (QMN) sources reaching into the energy domain >20 MeV are needed is presented. A brief overview of the existing facilities is given, and a list of key factors that an ideal QMN source for dosimetry and spectrometry should offer is presented. The authors conclude that all of the six QMN facilities currently in existence worldwide operate in sub-optimal conditions for dosimetry. The only currently available QMN facility in Europe capable of operating at energies >40 MeV, TSL in Uppsala, Sweden, is threatened with shutdown in the immediate future. One facility, NFS at GANIL, France, is currently under construction. NFS could deliver QMN beams up to about 30 MeV. It is, however, so far not clear if and when NFS will be able to offer QMN beams or operate with only so-called white neutron beams. It is likely that by 2016, QMN beams with energies >40 MeV will be available only in South Africa and Japan, with none in Europe.
Department of Physics and Astronomy Uppsala University Box 516 75120 Uppsala Sweden
German Aerospace Center Cologne Germany
iThemba Laboratory for Accelerator Based Sciences Somerset West 7129 South Africa
Paul Scherrer Institut Radiation Metrology Section CH 5232 Villigen PSI Switzerland
Citace poskytuje Crossref.org
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