On the standard form of the Bloch equation
✍ Scribed by Gérard G. Emch; Joseph C. Varilly
- Book ID
- 104757872
- Publisher
- Springer
- Year
- 1979
- Tongue
- English
- Weight
- 181 KB
- Volume
- 3
- Category
- Article
- ISSN
- 0377-9017
No coin nor oath required. For personal study only.
✦ Synopsis
The requirement is often made in non-equilibrium statistical mechanics that a transport equation should be derived as that which governs the subdynamics relative to a (small) part of a (large) conservative dynamical system close to equilibrium. We show that such a requirement on the Markovian relaxation of a 89 imposes that this process be described by a Bloch equation of a very specific form, which we call standard. We show that this reduced dynamics is quasi-free if, and only if, the relaxation time is maximally anisotropic.
The Bloch equation for a 89 reads:
k=l with ~-/(0) being the usual Paul/matrices. We say that this equation is standard if there exists a unitary transformation U on r such that o/(t) = Ur/(t)U -1 satisfies (d/dt)cq (t) = -~ol (t) -cooz(t), (d/dt)o 2 (t) = + wol (t) -~,o~ (t), (2) (d/d0 [03(0 -el] = -g [ o 3 ( t ) -el], with -1 < e < 1, co real, and 0 ~<# ~< 2•. e is the equilibrium value (03) of the component 03 of the spin, whereas (oa) = (02) = 0; co is the transverse frequency; there are only two relaxation times TII =//-1, and T• = X-1, which moreover satisfy the very remarkable relation TII ) T• Favre and Martin [6] seem to have been the first authors to argue that the Bloch equation would take this standard form whenever the 1-spin system is 'weakly coupled' to a bath at 'high' temperature. More recently Gorini et al. [7, 15] gave a thermodynamical, model-independent argument showing that if T/-1 = X/is the inverse relaxation time relative to the ]th component of *Research supported in part by NSF grant MCS 76 07286.
📜 SIMILAR VOLUMES
The generalized Bloch equations in the rotating frame are solved in Cartesian space by an approach that is different from the earlier Torrey solutions. The solutions are cast into a compact and convenient matrix notation, which paves the way for a direct physical insight and comprehension of the evo