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The gamma-ray strength function for gamma energies in the 1-7 MeV region hasbeen measured for 161,162-Dy and 171,172-Yb using the (3-He,alpha gamma)reaction. Various models are tested against the observed gamma-ray strengthfunctions. The best description is based on the Kadmenskii, Markushev andFurman E1 model with constant temperature and the Lorentzian M1 model. Agamma-ray bump observed at E_gamma=3 MeV is interpreted as the so-called pygmyresonance, which has also been observed previously in (n,gamma) experiments.The parameters for this resonance have been determined and compared to theavailable systematics.Comment: 11 pages, including 4 figures and 2 table

physical review. c. nuclear physics/physical review. c, nuclear physics

<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi>γ</mml:mi></mml:math>-ray strength function and pygmy resonance in rare earth nuclei

γ-ray strength function and pygmy resonance in rare earth nuclei