2.2.1. Particle Control Equation
The DEM model applies Newton’s second law to describe particle motion [
10]. Each particle is treated as a discrete unit, and its motion is described by translational and rotational equations. The translational equation for rod-shaped particles is similar to that for spherical particles:
where
is the mass of the particle (kg);
is the velocity of the particle (m/s);
is the contact force (N);
is the gravitational force (N);
is the drag force (N);
is the lift force (N);
is the pressure gradient force (N);
is the extended Derjaguin–Landau–Verwey–Overbeek (XDLVO) force (N);
is the Brownian force (N); and
is the flagellar propulsive force (N).
For the rotational motion of rod-shaped particles, the following equation is used to account for orientation-dependent characteristics:
where g is the gravitational acceleration;
is the moment of inertia of the particle in the local coordinate system (
);
is the angular velocity of the particle in the local coordinate system (rad/s);
is the contact torque caused by the tangential contact force in the local coordinate system (
) [
11].
2.2.2. Fluid Interaction Model
In two-phase liquid-solid systems, the forces between particles and the fluid include drag, lift, and pressure gradient forces [
12]. The drag force on particles can be computed using the following equation:
For non-spherical particles, the drag coefficient is computed using the method of Ganser [
13], which is determined by the sphericity of the particles
, where
is the surface area of an equivalent sphere having the same volume as the particle and
is the actual surface area of the particle.
The lift force experienced by particles is calculated using the Saffman lift force equation:
where
is the equivalent radius of the particle (m);
G is the fluid shear rate (
); and
is the volume of the particle (
) [
14].
The pressure gradient force acting on the particle is defined as:
2.2.3. Particle–Particle/Wall Interaction Forces
In this study, the multi-sphere method is employed to construct the rod-shaped bacterial particle model. The contact force and torque acting on each individual particle are the sums of the forces and torques applied to the spherical elements constituting the rod-shaped particle [
15]. Particle–particle collisions are modeled using the Hertz–Mindlin contact model, where normal forces follow Hertzian contact theory, and tangential forces are described by the Mindlin–Deresiewicz theory. For particle-wall interactions, XDLVO theory is introduced to describe the adhesion process between bacterial particles and the substrate surface [
16]. The total interaction energy between bacteria (B) and the substrate surface (S) in the liquid phase (L) is the sum of Lifshitz-Van der Waals (LW), electrostatic double layer (EL), and acid-base (AB) interaction energies:
where
R is the radius of the bacteria;
d is the distance between the bacterial surface and the substrate surface;
A is the Hamaker constant, which is specific to the material interaction;
and
are the interaction energies when the two surfaces are in contact at the minimum equilibrium cut-off distance
;
is the permittivity of water;
and
are the zeta potentials of the bacterial and substrate surfaces, set to −0.012 V and −0.053 V respectively, based on experimental data [
17];
k is the reciprocal of the Debye length (
) [
18]; and
is the characteristic decay length of AB interactions in water [
19].
and
can be calculated from a series of surface energy formulas:
where
is the total surface energy of the material;
is the Lifshitz-Van der Waals (dispersive) component;
is the acid-base (polar) component;
is the electron-acceptor parameter, and
is the electron-donor parameter.
is the measured contact angle. The subscript
s denotes the solid (PTFE material),
b denotes the bacteria, and
l denotes the liquid (water).
The detailed surface energy components are listed in
Table 1.
Based on the aforementioned XDLVO parameters, the total interaction potential energy (
) between a
P. aeruginosa cell and the PTFE surface is calculated. As shown in
Figure 1, a distinct energy barrier exists at a separation distance of approximately 1.1 nm. This indicates that bacteria initially experience a repulsive force as they approach the PTFE surface before falling into the primary potential well for irreversible adhesion.
To account for potential uncertainties in physicochemical properties, a sensitivity analysis was performed by varying the Hamaker constant (A). Specifically, the potential energy curves were recalculated for , (baseline), and . The results show that for , the energy barrier is J with a primary minimum of J; for , the barrier is J and the minimum is J; and for , the barrier is J and the minimum is J. Although a 10% fluctuation in the Hamaker constant micro-adjusts the adhesion strength, the magnitude of the energy barrier remains stable without order-of-magnitude changes. This demonstrates that the spatial distribution trends of bacterial adhesion and the relative performance of different groove geometries are robust against parameter variations.
In this study, we adopt an idealized irreversible adhesion criterion: bacteria are deemed to have achieved irreversible adhesion once they cross the energy barrier and enter the primary potential well (the first deep energy minimum) of the XDLVO interaction. This criterion is a widely accepted simplification in numerical investigations of the initial bacterial adhesion stage. It should be clarified that this study focuses on the initial stage of bacterial adhesion, where XDLVO interaction forces and near-wall flow field characteristics are the dominant factors governing bacterial adhesion behavior; thus, the aforementioned simplification is physically justified. Nevertheless, this criterion remains an idealized assumption in real-world scenarios. For one thing, adherent bacteria may undergo detachment under extreme hydrodynamic shear. For another, bacteria can form stronger and more stable irreversible adhesion through pili/flagellar anchoring, as well as complex viscoelastic forces arising from the secretion and proliferation of extracellular polymeric substances (EPS). None of the above processes are included in the scope of this study.
The total interaction force is obtained by differentiating the interaction energy with respect to the separation distance:
2.2.5. Flagellar Propulsion Force
In this study, the flagellar propulsion force is simplified as a constant driving force aligned with the length axis of the bacterial particle. The force is modeled based on the experimental results of Chattopadhyay et al. [
21]. The propulsive force of the flagella is set to
, with its direction consistent with the major axis vector of the particle. Although the propulsion force value (
) is originally derived from
E. coli, applying it to
P. aeruginosa in our model is physically reasonable. Both are Gram-negative, rod-shaped bacteria with similar geometric aspect ratios. Furthermore, their typical swimming speeds in water are on the same order of magnitude (20–30
for
E. coli and 25–50
for
P. aeruginosa). According to Stokes’ drag law, the thrust required to maintain this swimming speed for a micron-sized body is on the order of 0.1–1.0 pN. Thus, the adopted value of 0.6 pN provides a kinematically consistent representation of the active motility of
P. aeruginosa without distorting the overall force balance.