A sphere rotating around a fixed axis will rotate in two
dimensions only and can be viewed from above the fixed axis as a circle. In this example, a sphere which is fixed on the vertical axis rotates around that axis only, meaning that the particle can have a θ value of 0 through 360 degrees, or 2π Radians, before having a net rotation of 0 again. These directions can be placed onto a graph which covers the entirety of the possible positions for the
face to be at relative to the starting point, through 2π radians, starting with -π radians through 0 to π radians. Assuming all particles begin with single orientation of 0, the first measurement of directions taken will resemble a
delta function at 0 as all particles will be at their starting, or 0th, position and therefore create an infinitely steep single line. Over time, the increasing amount of measurements taken will cause a spread in results; the initial measurements will see a thin peak form on the graph as the particle can only move slightly in a short time. Then as more time passes, the chance for the molecule to rotate further from its starting point increases which widens the peak, until enough time has passed that the measurements will be evenly distributed across all possible directions. The distribution of orientations will reach a point where they become
uniform as they all randomly
disperse to be nearly equal in all directions. This can be visualized in two ways. •
For a single particle with multiple measurements taken over time. A particle which has an area designated as its face pointing in the starting orientation, starting at a time t0 will begin with an orientation distribution resembling a single line as it is the only measurement. Each successive measurement at time greater than t0 will widen the peak as the particle will have had more time to rotate away from the starting position. •
For multiple particles measured once long after the first measurement. The same case can be made with a large number of molecules, all starting at their respective 0th orientation. Assuming enough time has passed to be much greater than t0, the molecules may have fully rotated if the forces acting on them require, and a single measurement shows they are near-to-evenly distributed.
Basic equations For rotational diffusion about a single axis, the mean-square angular deviation in time t is : \left\langle\theta^2\right\rangle = 2 D_r t, where D_r is the rotational diffusion coefficient (whose units are radians2/s). The angular drift velocity \Omega_d = (d\theta/dt)_{\rm drift} in response to an external torque \Gamma_{\theta} (assuming that the flow stays non-
turbulent and that inertial effects can be neglected) is given by : \Omega_d = \frac{\Gamma_\theta}{f_r}, where f_r is the frictional drag coefficient. The relationship between the rotational diffusion coefficient and the rotational frictional drag coefficient is given by the
Einstein relation (or Einstein–Smoluchowski relation): :D_r = \frac{k_{\rm B} T}{f_r}, where k_{\rm B} is the
Boltzmann constant and T is the absolute temperature. These relationships are in complete analogy to translational diffusion. The rotational frictional drag coefficient for a sphere of radius R is : f_{r, \textrm{sphere}} = 8 \pi \eta R^3 where \eta is the
dynamic (or shear) viscosity. The rotational diffusion of spheres, such as nanoparticles, may deviate from what is expected when in complex environments, such as in polymer solutions or gels. This deviation can be explained by the formation of a depletion layer around the nanoparticle.
Langevin dynamics Collisions with the surrounding fluid molecules will create a fluctuating torque on the sphere due to the varied speeds, numbers, and directions of impact. When trying to rotate a sphere via an externally applied torque, there will be a systematic drag resistance to rotation. With these two facts combined, it is possible to write the
Langevin-like equation: \frac{dL}{dt} = {I}\, \cdot \frac{d^2{\theta}}{dt^2} = - {\zeta}^{r} \cdot \frac{d{\theta}}{dt} + TB(t) Where: •
L is the angular momentum. • \frac{dL}{dt} is
torque. •
I is the moment of inertia about the rotation axis. •
t is the time. •
t0 is the start time. •
θ is the angle between the orientation at
t0 and any time after,
t. •
ζr is the rotational friction coefficient. •
TB(t) is the fluctuating Brownian torque at time
t. The overall Torque on the particle will be the difference between: TB(t) and ({\zeta}^{r} \cdot \frac{d{\theta}}{dt}) . This equation is the rotational version of
Newtons second equation of motion. For example, in standard translational terms, a
rocket will experience a boosting force from the engine while simultaneously experiencing a
resistive force from the air it is travelling through. The same can be said for an object which is rotating. Due to the random nature of rotation of the particle, the
average Brownian torque is equal in both directions of rotation. symbolised as: \left \langle TB(t) \right \rangle = 0 This means the equation can be averaged to get: \frac{d \left \langle L \right \rangle}{dt} = - {\zeta}^{r} \cdot \left \langle \frac{d{\theta}}{dt} \right \rangle = -\frac{\zeta^r}{I} \left \langle L \right \rangle Which is to say that the first derivative with respect to time of the average Angular momentum is equal to the negative of the Rotational friction coefficient divided by the moment of inertia, all multiplied by the average of the angular momentum. As \frac{d \left \langle L \right \rangle}{dt} is the rate of change of angular momentum over time, and is equal to a negative value of a coefficient multiplied by \left \langle L \right \rangle , this shows that the angular momentum is decreasing over time, or decaying with a decay time of: {\tau{_L}} = \frac{I}{\zeta^r} . For a sphere of mass
m, uniform density
ρ and radius
a, the moment of inertia is: I = \frac{2ma^2}{5} = \frac{8{\pi}{\rho}a^5}{15} . As mentioned above, the rotational drag is given by the
Stokes friction for rotation: {\zeta^r} = 8\pi\eta a^3 Combining all of the equations and formula from above, we get: {\tau{_L}} = \frac{\rho a^2}{15\eta} = \frac{3}{10}\tau_p where: • \tau_p is the momentum relaxation time •
η is the
viscosity of the Liquid the sphere is in.
Example: Spherical particle in water Let's say there is a virus which can be modelled as a perfect sphere with the following conditions: •
Radius (a) of 100 nanometres,
a = 10−7m. • Density:
ρ = 1500 kg m−3 • Orientation originally facing in a direction denoted by
π. • Suspended in water. • Water has a viscosity of
η = 8.9 × 10−4 Pa·s at 25 °C • Assume uniform mass and density throughout the particle First, the mass of the virus particle can be calculated: m = \frac {4\rho\pi a^{3}} {3} = \frac {4 \times 1500 \times \pi \times (10^{-7})^3} {3} = 6.3 \times 10^{-18} \mathrm{kg} From this, we now know all the variables to calculate moment of inertia: I = \frac {2ma^{2}} {5} = \frac {2 \times (6.3\times10^{-18}) \times (10^{-7})^2} {5} = 2.5 \times 10^{-32} \mathrm{kg} \cdot \mathrm{m}^2 Simultaneous to this, we can also calculate the rotational drag: \zeta^{r} = 8 \pi \eta a^{3} = 8 \times \pi \times (8.9\times10^{-4}) \times (10^{-7})^3 = 2.237 \times 10^{-23} \mathrm{Pa} \cdot \mathrm{s} \cdot \mathrm{m}^3 Combining these equations we get: \tau_L = \frac {I} {\zeta^r} = \frac {2.5 \times 10^{-32} \mathrm{kg} \cdot \mathrm{m}^2} {2.2 \times 10^{-23} \mathrm{Pa} \cdot \mathrm{s} \cdot \mathrm{m}^3} = 1.1 \times 10^{-9} \mathrm{kg} \cdot \mathrm{Pa}^{-1} \cdot \mathrm{s}^{-1} \cdot \mathrm{m}^{-1} As the
SI units for
Pascal are kg⋅m−1⋅s−2 the units in the answer can be reduced to read: \tau_L = 1.1 \times 10^{-9} \mathrm{s} For this example, the decay time of the virus is in the order of nanoseconds. == Smoluchowski description of rotation ==