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lammps/examples/USER/lb/dragforce/in.defaultgamma_drag
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in.defaultgamma_drag
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#===========================================================================#
# Drag force on a single sphere. #
# #
# Here, gamma (used in the calculation of the particle-fluid interaction #
# force) is calculated by default. The resulting equilibrium drag force #
# should correspond to the Stokes drag force on a sphere with a slightly #
# larger "hydrodynamic" radius, than that given by the placement of the #
# particle nodes. #
# #
# Sample output from this run can be found in the file: #
# 'defaultgamma_drag.out' #
#===========================================================================#
units micro
dimension 3
boundary p p f
atom_style atomic
#----------------------------------------------------------------------------
# Need a neighbor bin size smaller than the lattice-Boltzmann grid spacing
# to ensure that the particles belonging to a given processor remain inside
# that processors lattice-Boltzmann grid.
# The arguments for neigh_modify have been set to "delay 0 every 1", again
# to ensure that the particles belonging to a given processor remain inside
# that processors lattice-Boltzmann grid. However, these values can likely
# be somewhat increased without issue. If a problem does arise (a particle
# is outside of its processors LB grid) an error message is printed and
# the simulation is terminated.
#----------------------------------------------------------------------------
neighbor 1.0 bin
neigh_modify delay 0 every 1
read_data data.one_radius16d2
#----------------------------------------------------------------------------
# None of the particles comprising the spherical colloidal object should
# interact with one another.
#----------------------------------------------------------------------------
pair_style lj/cut 2.45
pair_coeff * * 0.0 0.0 2.45
neigh_modify exclude type 1 1
#----------------------------------------------------------------------------
# Need to use a large particle mass in order to approximate an infintely
# massive particle, moving at constant velocity through the fluid.
#----------------------------------------------------------------------------
mass * 10000.0
timestep 3.0
velocity all set 0.0 0.0001 0.0 units box
#---------------------------------------------------------------------------
# Create a lattice-Boltzmann fluid covering the simulation domain.
# All of the particles in the simulation apply a force to the fluid.
# Use the standard LB integration scheme, a fluid density = 1.0,
# fluid viscosity = 1.0, lattice spacing dx=4.0, and mass unit, dm=10.0.
# Use the default method to calculate the interaction force between the
# particles and the fluid. This calculation requires the surface area
# of the composite object represented by each particle node. By default
# this area is assumed equal to dx*dx; however, since this is not the case
# here, it is input through the setArea keyword (i.e. particles of type 1
# correspond to a surface area of 10.3059947).
# Use the trilinear interpolation stencil to distribute the force from
# a given particle onto the fluid mesh (results in a smaller hydrodynamic
# radius than if the Peskin stencil is used).
# Print the force and torque acting on the particle to the screen at each
# timestep.
#----------------------------------------------------------------------------
fix 1 all lb/fluid 1 1 1.0 1.0 setArea 1 10.3059947 dx 4.0 dm 10.0 trilinear calcforce 10 all
#---------------------------------------------------------------------------
# For this simulation the colloidal particle moves at a constant velocity
# through the fluid. As such, we do not wish to apply the force from
# the fluid back onto the object. Therefore, we do not use any of the
# viscous_lb, rigid_pc_sphere, or pc fixes, and simply integrate the
# particle motion using one of the built-in LAMMPS integrators.
#---------------------------------------------------------------------------
fix 2 all nve
run 100000
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