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Program - Brookhaven National Laboratory

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We measured the isomeric yield ratio for the photonuclear reaction of nat Sm (γ,xn) 143m,g Sm by using the<br />

activation method with bremsstrahlung beam. The high purity natural Sm foil in disc shape was irradiated<br />

with beam of energy range from 40 to 60 MeV. The experiment was performed at the 100-MeV electron<br />

linac of Pohang Accelerator <strong>Laboratory</strong>. The induced activity in the irradiated Sm foil was measured by<br />

the high-purity germanium detector (HPGe) and the experimental data was analyzed through the Gamma<br />

Vision program. The present results are the first measurement at bremsstrahlung energies above the giant<br />

dipole resonance region and the obtained data was compared with the corresponding values found in the<br />

literature. The study of isomeric yield ratio is useful for understanding of nuclear reaction mechanism,<br />

approaching of nuclear structure and testing of theoretical nuclear models.<br />

Corresponding author: Guinyun Kim<br />

PB 6 5:15 PM<br />

New Measurements of the 241 Am(n,2n) 240 Am Cross Section<br />

A. Kalamara, M. Diakaki, R. Vlastou, M. Kokkoris, N.G. Nicolis , A. Tsinganis<br />

Department of Physics, <strong>National</strong> Technical University of Athens, 157 80 Athens, Greece<br />

S. Ashley, M. Axiotis and A. Lagoyannis<br />

Institute of Nuclear Physics, NCSR ”Demokritos”, 153 10 Aghia Paraskevi, Greece<br />

The study of 241 Am(n,2n) 240 Am reaction is important as Am is one of the most abundant isotopes in the<br />

spent fuel cycle and one of the most highly radiotoxic among the actinides. Five recent works provide data<br />

from threshold to 20 MeV, with severe discrepancies among them in the energy region 10 to 12 MeV [1,5].<br />

In order to resolve these discrepancies between the existing data, new measurements have been performed<br />

at the 5 MV Tandem T11/25 accelerator laboratory of NCSR “Demokritos,” with a high purity Am target<br />

provided by JRC-IRMM, Belgium. Due to its high radioactivity (5 GBq), the Am target was placed inside<br />

a 3 mm lead cylindrical shielding and was irradiated with 10.4 and 10.8 MeV neutrons. Gamma-ray spectra<br />

were taken at a distance of 10 cm from a Ge detector, before and after the irradiation, to ensure that there is<br />

no contamination in the 987.8 keV photopeak from the decay of the 240 Am residual nucleus. The efficiency<br />

of the detection setup, including the extended geometry of the Am sample, was extracted by using two<br />

different techniques, an experimental and a simulated one. The cross section has thus been deduced with<br />

respect to the 27 Al(n,α) 24 Na, 93 Nb(n,2n) 92m Nb and 197 Au(n,2n) 196 Au reference reactions, implementing<br />

the activation technique. This research has been co-financed by the European Union (European Social Fund<br />

– ESF) and Greek national funds through the Operational <strong>Program</strong> “Education and Lifelong Learning”<br />

of the <strong>National</strong> Strategic Reference Framework (NSRF) - Research Funding <strong>Program</strong>: Heracleitus II.<br />

Investing in knowledge society through the European Social Fund.<br />

Corresponding author: R. Vlastou<br />

[1] A. A. Filatenkov and S. V. Chuvaev, Phys. At. Nucl. 63, 1504(2000). [2] R. W. Lougheed, W.<br />

Webster, M. N. Namboodiri, D. R. Nethaway, K. J. Moody, J. H. Landrum, R. W. Hoff, R. J. Dupzyk,<br />

J. H. McQuaid, R. Gunnink., Radiochim. Acta90, 833 (2002). [3] G. Perdikakis, C. T. Papadopoulos,<br />

R. Vlastou, A. Lagoyannis, A. Spyrou, M. Kokkoris, S. Galanopoulos, N. Patronis, D. Karamanis, C.<br />

Zarkadas, Phys. Rev. C 73, 067601(2006). [4] A. P. Tonchev, C. T. Angell, M. Boswell, A. S. Crowell,<br />

B. Fallin, S. Hammond, C. R. Howell, A. Hutcheson, H. J. Karwowski, J. H. Kelley, Phys. Rev. C 77,<br />

054610 (2008). [5] C. Sage, V. Semkova, O. Bouland, P. Dessagne, A. Fernandez, F. Gunsing, C. Nastren,<br />

G. Noguere, H. Ottmar, A. J. M. Plompen, P. Romain, G. Rudolf, J. Somers, and F. Wastin. Phys. Rev.C<br />

81, 064604 (2010).<br />

PB 7 5:30 PM<br />

226

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