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Nonconserved Dynamics

 

Furthermore, any dynamics problem is also sensitive to conservation laws, which play no role in equilibrium. We must therefore study the dynamics separately in the presence or absence of a conserved density. Consider first the case in which no conservation law applies. This is appropriate for certain CDW phases. A well studied example is the higher-temperature CDW in NBSe tex2html_wrap_inline4102 . This material has three chains in its unit cell. In a temperature range of 59K to 144K, only one of the three chains forms a CDW, and the others provide itinerant metallic carriers which coexist with it. Charge can thus be exchanged back and forth between the CDW and the Fermi sea.

Provided thermal effects can be neglected (this is far from obvious in real materials, but seems to be a good approximation in some instances), an appropriate model would appear to be simply a driven random-field XY (RFXY) model, i.e.

equation1650

where F is a uniform force, and H is the RFXY Hamiltonian,

equation1656

Here the angular brackets denote a sum over nearest neighbors, K is a stiffness constant, and tex2html_wrap_inline4110 and tex2html_wrap_inline4112 are the magnitude and direction of the random field at site i. Because this lattice form involves only periodic functions, local phase slips are allowed. We will also need the expression for the current, which is

equation1661

An argument due to Coppersmith and Millis tells us that once phase slips are allowed, this depinning transition is actually washed out even at zero temperature[16]. Let us suppose that the system is below threshold, tex2html_wrap_inline3956 . Then at long times, the system is static, and the net force on any region of the sample must be zero. This net force is the sum of the external force, the interaction forces, and the random forces acting on the region, i.e.

equation1664

where tex2html_wrap_inline2844 represents a compact region of the sample. Because the interaction forces act pairwise, the elastic forces in the interior of the region cancel. We thus have

equation1672

where tex2html_wrap_inline4120 denotes the set of boundary spins. The external elastic force on boundary spin i is

equation1680

where the prime on the sum indicates that it is taken only over nearest neighbor sites not contained in tex2html_wrap_inline2844 . Clearly, tex2html_wrap_inline3124 is bounded,

equation1686

One can now easily argue that this force balance cannot be satisfied everywhere in an infinite sample. Suppose we divide space up into regions (say cubes) of linear size L. There is some small, but finite probability that mean (spatially averaged) magnitude of the random fields in each region is less than F, no matter how small F is. If this is the case, the local random fields are not strong enough to balance the external force alone. The only hope is that the boundary interactions can complete the balance. But since this contribution only grows with the area tex2html_wrap_inline4134 of the regions, it cannot do so. Thus in some finite fraction of these regions, force balance is impossible, and some phase slip must occur. Because it occurs in a finite volume fraction of the system, the spatially averaged velocity must be non-zero for any F. In other words, there is no threshold field below which the CDW is completely pinned. The functional form of tex2html_wrap_inline4138 is, however, expected to be highly non-analytic, because it depends upons these extremely rare weakly pinned regions of the sample.


next up previous contents
Next: Conserved Dynamics Up: Driven dynamics Previous: Elastic Depinning

Leon Balents
Thu May 30 08:21:44 PDT 1996