Mesoscale simulations: Lattice Boltzmann and particle algorithms

PHYSICA A 369:1 (2006) 159-184

Abstract:

I introduce two mesoscale algorithms, lattice Boltzmann and stochastic rotation dynamics, and show how they can be used to investigate the hydrodynamics of complex fluids. For each method I describe the algorithm, show that it solves the Navier-Stokes equations, and then discuss physical problems where it is particularly applicable. For lattice Boltzmann the examples I choose are phase ordering in a binary fluid and drop dynamics on a chemically patterned surface. For stochastic rotation dynamics I consider the hydrodynamics of dilute polymer solutions, concentrating on shear thinning and translocation across a barrier. (c) 2006 Elsevier B.V. All rights reserved.

Hydrodynamic interactions and Brownian forces in colloidal suspensions: Coarse-graining over time and length scales

Physical Review E 74 (2006) 031402 29pp

Authors:

AA Louis, J.T. Padding

A nu=2/5 Paired Wavefunction

(2006)

Authors:

Steven H Simon, EH Rezayi, NR Cooper, I Berdnikov

Generalized Quantum Hall Projection Hamiltonians

(2006)

Authors:

Steven H Simon, EH Rezayi, NR Cooper

Capacity of differential versus nondifferential unitary space-time modulation for MIMO channels

IEEE Transactions on Information Theory 52:8 (2006) 3622-3634

Authors:

AL Moustakas, SH Simon, TL Marzetta

Abstract:

Differential unitary space-time modulation (DUSTM) and its earlier nondifferential counterpart, USTM, permit high-throughput multiple-input multiple-output (MIMO) communication entirely without the possession of channel state information by either the transmitter or the receiver. For an isotropically random unitary input we obtain the exact closed-form expression for the probability density of the DUSTM received signal, permitting the straightforward Monte Carlo evaluation of its mutual information. We compare the performance of DUSTM and USTM through both numerical computations of mutual information and through the analysis of low- and high-signal-to-noise ratio (SNR) asymptotic expressions. In our comparisons the symbol durations of the equivalent unitary space-time signals are equal to T. For DUSTM the number of transmit antennas is constrained by the scheme to be M = T/2, while USTM has no such constraint. If DUSTM and USTM utilize the same number of transmit antennas at high SNRs the normalized mutual information of the two schemes expressed in bits/s/Hz are asymptotically equal, with the differential scheme performing somewhat better. At low SNRs the normalized mutual information of DUSTM is asymptotically twice the normalized mutual information of USTM. If, instead, USTM utilizes the optimum number of transmit antennas then USTM can outperform DUSTM at sufficiently low SNRs. © 2006 IEEE.