The intensity of the recoilless and nonrecoilless resonant scattering of Mössbauer gamma rays for single line Lorentzian energy distributions is calculated. The scattered intensities are expressed in terms of a scattering function which contains the parameters of the scatterer. This scattering function has been evaluated for a wide range of values of the recoilless fraction, electronic absorption, thickness, and linewidth of the scatterer. It can be used to determine source and scatterer recoilless fractions from the total scattered intensities. If the recoilless fraction is sufficiently large the recoilless and the nonrecoilless part of the resonantly scattered intensity can be determined, with the aid of numerical calculations given, from a measurement of the transmission of the scattered gamma rays through a resonant absorber. The ratio of the recoilless to the nonrecoilless part of the resonantly scattered intensity does not depend very sensitively upon the properties of the source and can be used to determine unambiguously the recoilless fraction of the scatterer.

1.
A few scattering experiments have been performed with the 14.4‐keV transition of Fe57. The recoilless part of the resonance scattering cross section has been studied by
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Interference effects have been investigated by
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5.
In recent Mössbauer scattering experiments with the 103‐keV and the 145‐keV transitions of Eu153 and Pr141, respectively, NT/B was 10 times larger than the recoilless fraction. [R. J. Morrison, thesis, University of Illinois (1964, unpublished)].
6.
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11.
The nuclear resonance cross section is defined
, where ƛ is the reduced wavelength and Γnat is the natural width of the level.
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