Mössbauer effect

The Mössbauer effect (German: Mößbauer [Meß-Bauer]), a physical phenomenon discovered by Rudolf Mößbauer in 1957, refers to the resonant and recoil-free emission and absorption of gamma rays by atoms bound in a solid form.

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Description

The emission and absorption of x-rays by gases had been observed previously, and it was expected that a similar phenomenon would be found for gamma rays, which are created by nuclear transitions (as opposed to x-rays, which are produced by electronic transitions). However, attempts to observe gamma-ray resonance in gases failed due to energy being lost to recoil, preventing resonance (the Doppler effect also broadens the gamma-ray spectrum). Mössbauer was able to observe resonance in solid iridium, which raised the question of why gamma-ray resonance was possible in solids, but not in gases. Mössbauer proposed that, for the case of atoms bound into a solid, under certain circumstances a fraction of the nuclear events could occur essentially without recoil. He attributed the observed resonance to this recoil-free fraction of nuclear events. This discovery was rewarded with the Nobel Prize in Physics in 1961 together with Robert Hofstadter's research of electron scattering in atomic nuclei.   In general, gamma rays are produced by nuclear transitions: from an unstable high-energy state, to a stable low-energy state. The energy of the emitted gamma ray corresponds to the energy of the nuclear transition, minus an amount of energy that is lost as recoil to the emitting atom. If the lost "recoil energy" is small compared with the energy linewidth of the nuclear transition, then the gamma ray energy still corresponds to the energy of the nuclear transition, and the gamma ray can be absorbed by a second atom of the same type as the first. This emission and subsequent absorption is called resonance. Additional recoil energy is also lost during absorption, so in order for resonance to occur the recoil energy must actually be less than half the linewidth for the corresponding nuclear transition.

The amount of lost energy is described by the equation:

where E_R is the energy lost as recoil, E_γ is the energy of the gamma ray, M is the mass of the emitting or absorbing body, and c is the speed of light. In the case of a gas the emitting and absorbing bodies are atoms, so the mass is quite small, resulting in a large recoil energy, which prevents resonance. (Note that the same equation applies for recoil energy losses in x-rays, but the photon energy is much less, resulting in a lower energy loss, which is why gas-phase resonance could be observed with x-rays.)

In a solid, the nuclei are bound to the lattice and do not recoil in the same way as in a gas. The lattice as a whole recoils but the recoil energy is negligible because the M in the above equation is the mass of the whole lattice. However, the energy in a decay can be taken up (or supplied by) lattice vibrations. The energy of these vibrations is quantised in units known as phonons. The Mössbauer effect occurs because there is a finite probability of a decay occurring involving no phonons. Thus in a fraction of the nuclear events (the recoil-free fraction), the entire crystal acts as the recoiling body, and these events are essentially recoil-free. In these cases, since the recoil energy is negligible, the emitted gamma rays have the appropriate energy and resonance can occur.

In general (depending on the half-life of the decay), gamma rays have very narrow linewidths. This means they are very sensitive to small changes in the energies of nuclear transitions. In fact, gamma rays can be used as a probe to observe the effects of interactions between a nucleus and its electrons and those of its neighbors. This is the basis for Mössbauer spectroscopy, which combines the Mossbauer effect with the Doppler effect to monitor such interactions.

Zero-phonon optical transitions, a process closely analogous to the Mössbauer effect, can be observed in lattice-bound chromophores at low temperatures.

See also

• Alpha decay
• Beta decay
• Gamma decay
• Pound-Rebka experiment

Further reading

• R.L. Mössbauer, Gammastrahlung in Ir¹⁹¹, Z. Physik 151, 124 (1958). (in German)
• H. Frauenfelder, The Mössbauer Effect, W. A. Benjamin, New York, 1962.
• The beginnings of Mössbauer spectroscopy, Education in Chemistry, July 2002.
• G. Vandergrift and B. Fultz (July 1998). "The Mössbauer effect explained". American Journal of Physics 66 (7): 593-596. AAPT. doi:10.1119/1.18911.

• J. Hesse (Jan 1973). "Simple Arrangement for Educational Mössbauer-Effect Measurements". American Journal of Physics 41 (1): 127-129. AAPT. doi:10.1119/1.1987142.

• F. Ninio (May 1973). "The Forced Harmonic Oscillator and the Zero-Phonon Transition of the Mössbauer Effect". American Journal of Physics 41 (5): 648-649. AAPT. doi:10.1119/1.1987323.

• Leonard Eyges (Oct 1965). "Physics of the Mössbauer Effect". American Journal of Physics 33 (10): 790-802. AAPT. doi:10.1119/1.1970986.