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Theory

Dynamic Light Scattering (DLS) refers to an optical technique used for analyzing dynamic properties and size distribution of a broad variety of physical, chemical, and biological systems composed of several suspended constituents [1]. These can be colloidal particles, macromolecules, bubbles, or droplets. For simplicity, we will simply talk of particles in all three cases.

DLS is based on the extraction of spectral information derived from time-dependent fluctuations of the light scattered from a spatially limited volume within the sample. Specifically, when a suspension of particles is hit by a monochromatic coherent beam of light, generated scattered light waves spread out in all directions. Scattered waves interference in the far-field region generates a net scattered light intensity I_s(t). Due to the random motion of the suspended particles within the sample, the interference can be stochastically either constructive or destructive, hence resulting in a stochastic light intensity signal.

The suspended particles of the colloidal dispersion under investigation undergo Brownian motion. This motion results in fluctuations in the distances between the particles and hence also in fluctuations of the phase relations of the scattered light. Additionally, the number of particles within the scattering volume may vary in time. The net result is a fluctuating scattered intensity. The corresponding measured normalized intensity correlation function is written as:

g_2(q,\tau)=\frac{\left<I_s(q,t)I_s(q,t+\tau)\right>}{\left<|I_s(q,t)|\right>^2},      [1]

with τ being the time lag and q being the scattering vector module. By means of the Siegert relation can be related to the electric field correlation function g1(q,τ):

g_2(q,\tau) = 1 + \beta \left |g_1(q,\tau) \right |^2

\beta being the so-called intercept and where the field correlation function g_1(q,\tau) is defined as

g_1(q,\tau) = \frac{\left \langle E_s(q,t))E_s^*(q,t+\tau) \right \rangle}{\left \langle |E_s(q,t,)|^2 \right \rangle}

The field correlation function may be used to determine the diffusion coefficient D of the scatterers. For a monodisperse sample, is fitted to an exponential function

g_1(q,\tau)=\exp(-\Gamma \tau)

yielding the decay rate \Gamma. From its definition:

\Gamma=q^2 D

one obtains the diffusion coefficient and by using the Stokes-Einstein equation one can calculate the hydrodynamic radius

R = \frac{kT}{6 \pi \eta D}

with k the Boltzmann constant, T the temperature in Kelvins, and \eta the viscosity of the suspending medium.

It is important to note that the equation above is only true for the case of single scattered light. If the particle concentration is too high, such that the mean free path l becomes smaller than the sample dimension d, multiple scattering will occur which will render the equation invalid. 

 

[1] B.J. Berne and R. Pecora. Dynamic light scattering. Dover Publications, Mineola, 2000.


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