However, in the PSDW, the holes are hopping on the square lattice, as shown in44 , the microscopic origin of the drag is due to the correlated character of hopping transports of the vacancies between the active and passive layers, it leads to a very large drag.
Mutual Composite Fermion and composite Boson approaches to balanced and imbalanced bilayer quantum Hall system: an electronic analogy of the Helium 4 system
We wish to model a polluant evolving by two mechanisms: a passive transport by the velocity ﬁeld, and collisions with the other ﬂuid particles modeled by random centered and independent increments {(αn , βn ) ∈ Z × Zd , n ∈ N}, independent of the velocity ﬁeld.
Self-Intersection Times for Random Walk, and Random Walk in Random Scenery in dimensions d>4
The velocity ﬁeld deﬁned above is an axisymmetric generalisation of the isotropic random ﬂow introduced by Kraichnan (1968) in the context of passive turbulent transport.
Orientation of non-spherical particles in an axisymmetric random flow
Davis, Modeling eddy transport of passive tracers, J.
Nonlocal Dynamics of Passive Tracer Dispersion with Random Stopping
Metallicity ﬂuctuations are summarized, and the theory of turbulent transport of passive tracers is reviewed.
Interstellar Turbulence II: Implications and Effects
There are many methods for studying passive scalar turbulent transport.
Interstellar Turbulence II: Implications and Effects
The various terms that may enter into deﬁning the time-derivative are divided into “source” terms Si , terms that are local in some sense (e.g., the pressure gradient) and “transport” terms Ti , terms that describe advection (e.g., the terms describing the passive transport of momentum or energy with the ﬂow).
General Relativistic MHD Jets
Hydraulic, tracer, and geophysical measurements of transport parameters will be made during cavern enlargement, and instrumentation arrays will be installed in the finished cavities to monitor the long-term passive response in the stable zone surrounding the detectors.
Reference Design Project Book: NUSEL-Homestake
As a ﬁrst step we perform a test of passive cosmic ray transport along the magnetic ﬁeld, which is directed along the x-axis, assuming K⊥ = 0 and a static medium, i.e v = 0.
Incorporation of cosmic ray transport into the ZEUS MHD code. Application for studies of Parker instability in the ISM
The passive transport means that the cosmic ray gas has no dynamical inﬂuence onto the motion of thermal gas.
Incorporation of cosmic ray transport into the ZEUS MHD code. Application for studies of Parker instability in the ISM
The difference between the passive and active cosmic ray transport is remarkable.
Incorporation of cosmic ray transport into the ZEUS MHD code. Application for studies of Parker instability in the ISM
In order to check the presented method we compared results of the diffusive passive transport of cosmic rays with analytical solutions of the diffusion equation.
Incorporation of cosmic ray transport into the ZEUS MHD code. Application for studies of Parker instability in the ISM
Thus, conventional wisdom leads to considering the magnetic ﬁeld as dynamically irrelevant—a passive contaminant simply frozen into the background ﬂuid and transported by purely hydrodynamic motions.
Saturation of the Magnetothermal Instability in Three Dimensions
However, in ideal MHD, due to ideal Ohm’s law, the magnetic ﬁeld undergoes a passive transport by the ﬂuid velocity and its topology is preserved.
Well-posedness for Hall-magnetohydrodynamics
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