Theory of Nuclear Magnetic Relaxation by Spin-Rotational Interactions in Liquids

Paul S. Hubbard
Phys. Rev. 131, 1155 – Published 1 August 1963
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Abstract

The contribution of spin-rotational interactions to the nuclear magnetic relaxation of identical spin-½ nuclei at equivalent positions in spherical liquid molecules is calculated by use of the semiclassical form of the density-operator theory of relaxation, and the result is compared with the contributions of intra- and intermolecular dipole-dipole interactions. The angular velocity of a molecule is treated classically by assuming that it obeys an equation analogous to the Langevin equation that is postulated in treatments of translational Brownian motion. The change in orientation of a molecule is assumed to be due to isotropic rotational Brownian motion. By use of this model the correlation functions of components of the angular velocity of a molecule are calculated, and are found to have an exponentially decaying time dependence with a time constant (correlation time) τ1 that is quite different in its temperature dependence than the correlation time τ2 of the dipole-dipole interactions. In typical situations τ1 is much smaller than τ2. Use is made of this fact to evaluate the correlation functions of the functions of the orientation and angular velocity that occur in the tensor spin-rotational interactions. The result that τ1τ2 explains the experimentally observed "quenching" of the relaxation effect of spin-rotational interactions in liquids, and the result that τ1T increases as the temperature increases explains the experimentally observed temperature dependence of the relaxation effect of spin-rotational interactions in liquids.

  • Received 21 March 1963

DOI:https://doi.org/10.1103/PhysRev.131.1155

©1963 American Physical Society

Authors & Affiliations

Paul S. Hubbard*

  • Department of Physics, University of North Carolina, Chapel Hill, North Carolina

  • *Alfred P. Sloan Research Fellow.

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Vol. 131, Iss. 3 — August 1963

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