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By Herbert Jaeger, Matthew O. Zacate

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81 (2010), p. 073501. 58. A. R. Arends, C. Hohenemser, F. Pleiter, H. De Waard, L. Chow, and R. M. Suter: Hyperfine Interact. Vol. 8 (1980), p. 191. 59. For example, H. Frauenfelder, R. M. Steffen, S. R. De Groot, H. A. Tolhoek, and W. J. Huiskamp, in: Alpha-, Beta-, and Gamma-Ray Spectroscopy, vol. 2, edited by Kai Siegbahn, North-Holland Publishing Company, Amsterdam (1965). 60. M. O. Zacate and G. S. Collins: Phys. Rev. B Vol. 69 (2004), p. 174202. 61. P. Wodniecki, A. Kulińska, B. Wodniecka, and M.

18. R. M. Steffen and K. Alder, in: The Electromagnetic Interaction in Nuclear Spectroscopy, edited by W. D. Hamilton, North-Holland Publishing Company, Amsterdam (1965). 19. H Frauenfelder and R. M. Steffen, in: Alpha-, Beta- and Gamma-Ray Spectroscopy, edited by K. Siegbahn, North-Holland Publishing Company, Amsterdam (1965). 20. Artur Wilson Carbonari, José Mestnik-Filho, and Rajendra Narain Saxena: current volume. 21. T. Butz: Hyperfine Interact. Vol. 52 (1989), p. 189. 22. L. A. Mendoza-Zélis, A.

The effect of the hyperfine interaction on this Herbert Jaeger and Matthew O. Zacate 45 intermediate state lifts the energy degeneracy, splitting it in sublevels. In Table 1 the properties for three probe nuclei commonly used in PAC spectroscopy to measure magnetic hyperfine interactions are shown. PAC spectroscopy measures the hyperfine interaction via the time evolution of the emission pattern of the second gamma-ray ( γ 2 ) in the cascade from a set of nuclei whose intermediate state have been selected by measuring the direction of the first gamma-ray ( γ 1 ).

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