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• W2076002032 abstract "Using the decay of 16.1-day ${mathrm{Rh}}^{99}$, the half-life of the 90-keV state in ${mathrm{Ru}}^{99}$ has been measured by observing delayed coincidences for the (354-90)- and the (529-90)-keV cascades. The result ${t}_{frac{1}{2}}=(20.7ifmmodepmelsetextpmfi{}0.3)$ nsec, is very suitable for a measurement of the Larmor precession in this level by means of the time-differential angular-correlation technique. To overcome the difficult problem of correcting for paramagnetic shielding, the $g$ factor was determined with the Ru atoms in three magnetically different environments: (1) with a liquid source, (2) with Ru embedded in a copper lattice, and (3) with Ru dissolved in Ni. In the last case the product $g{H}_{mathrm{eff}}$ was measured as a function of an external polarizing field, yielding both the $g$ factor and the magnetic hyperfine field of Ru in Ni. The method of using cubic metal lattices [case (2) above] is demonstrated to be a reliable way of measuring $g$ factors of excited nuclear states, as there are no interfering perturbation effects due to time-dependent and/or static quadrupole interactions. The final result for the $g$ factor is $g=ensuremath{-}0.189ifmmodepmelsetextpmfi{}0.004$, which gives, with a spin of $frac{3}{2}$ for the 90-keV level, a magnetic moment of $ensuremath{mu}=ensuremath{-}0.284ifmmodepmelsetextpmfi{}0.006$ nm. Paramagnetic shielding in liquid sources of transition elements is discussed, and $g$ factors previously determined for such sources are shown to be in doubt by 5 to 10%." @default.
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• W2076002032 date "1965-08-09" @default.
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• W2076002032 title "<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>g</mml:mi></mml:math>Factor of the 90-KeV Level in<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mrow><mml:msup><mml:mrow><mml:mi mathvariant=normal>Ru</mml:mi></mml:mrow><mml:mrow><mml:mn>99</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math>and the Paramagnetic Correction in Transition Atoms" @default.
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• W2076002032 doi "https://doi.org/10.1103/physrev.139.b532" @default.
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