Diffusion: general

 

Principle

 

Diffusion is the net action of particles  (molecules, atoms, electrons, etc.), heat, momentum, or light whose end is to minimize a concentration gradient. A concentration gradient is the difference between the high concentration and the low concentration. It also includes the speed of the process. Diffusion can be quantified by measuring the concentrations gradient.

More formally, diffusion is defined as the process through which speed a thermodynamic system at local thermodynamic equilibrium returns to global thermodynamic equilibriums, through the homogenization of the values of its intensive parameters (or bulk parameters, such as viscosity, density, melting point etc.).

 

In all cases of diffusion, the net flux of the transported quantity (atoms, energy, or electrons) is equal to a physical property (diffusivity, thermal conductivity, electrical conductivity) multiplied by a gradient (a concentration, thermal, electric field gradient). So:

  Diffusion ≡ some conductivity times a gradient.

Noticeable transport occurs only if there is a gradient. For example, if the temperature is constant, heat will move as quickly in one direction as in the other, producing no net heat transport or change in temperature.

 

The process of diffusion minimizes free energy and is thus a spontaneous process. An example of diffusion is the swelling of pasta, where water diffuses into the sponge-like structure of the dry and stiff pasta.

The different forms of diffusion can be modeled quantitatively using the diffusion equation, (see More Info) which goes by different names depending on the physical situation. For instance - steady-state bi-molecular diffusion is governed by Fick's law, steady-state thermal diffusion is governed by Fourier's law. The generic diffusion equation is time dependent, and as such applies to non-steady-state situations as well.

 

The second law of thermodynamics states that in a spontaneous process, the entropy of the universe increases. Entropy is a measure of how far a spontaneous physical process of smoothing-out differences has progressed, for instance a difference in temperature or in concentration (see further Entropy). Change in entropy of the universe is equal to the sum of the change in entropy of a system and the change in entropy of the surroundings. A system refers to the part of the universe being studied; the surrounding is everything else in the universe. Spontaneous change results in dispersal of energy. Spontaneous processes are not reversible and only occur in one direction. No work is required for diffusion in a closed system. Reversibility is associated with equilibrium. Work can be done on the system to change equilibrium. Energy from the surroundings decrease by the amount of work expended from surroundings. Ultimately, there will be a greater increase in entropy in the surroundings than the decrease of entropy in the system working accordingly with the second law of thermodynamics.

 

Types of diffusion

Diffusion includes all transport phenomena occurring within thermodynamic systems under the influence of thermal fluctuations (i.e. under the influence of disorder; this excludes transport through a hydrodynamic flow, which is a macroscopic, ordered phenomenon). Well known types are the diffusion of atoms and molecules, of electrons, (resulting in electric current), Brownian motion (e.g. of a single particle in a solvent), collective diffusion (the diffusion of a large number of (possibly interacting) particles), effusion of a gas through small holes, heat flow (thermal diffusion), osmosis, isotope separation with gaseous diffusion.

 

 

Application

 

Application, i.e. occurrence, in nature, dead and alive, can be found nearly everywhere. In living bodies it is found interstitionally as well as in living cells. Many man made apparatus, also for medical purposes, make use of the principle of diffusion. Some very obvious examples of applications are in the techniques of chromatography, electrophoresis, oxygen analysis, spectroscopy, thermography, the calculation of body heat conduction and dissipation (see Body heat conduction and Newton’s Law of cooling) etc.

 

Diffusion in biological systems

Specific examples in biological systems are diffusion across biological membranes, of ion through ion channels, in the alveoli of mammalian lungs across the alveolar-capillary membrane. In the latter process the diffusion is Knudson-like diffusion, in other words it is also dependent on space restrictions (the small size of the providing (alveoli) and recipient (capillaries) volumes. Another type is facilitated diffusion (passive transport across a membrane, with the assistance of transport proteins)

Numeric example

By knowing the diffusion coefficient of oxygen in watery tissue, the distance of diffusion and the diffusion gradient, then the time required for the diffusion of oxygen from the alveoli to the alveolar capillaries can be calculated. It appears to be some 0.6 ms (see More Info).

 

More Info

 

Diffusion equation

The diffusion equation is a partial differential equation, which describes the density fluctuations in a material undergoing diffusion. It is also used in population genetics to describe the 'diffusion' of alleles in a population.

The equation is usually written as:

                (1)

where φ is the density of the diffusing material, t is time, D is the collective diffusion coefficient, is the spatial coordinate and the nabla symbol φ represents the vector differential operator del (see also Fick’s Laws). If the diffusion coefficient depends on the density then the equation is nonlinear. If D is a constant, however, then the equation reduces to the following linear equation:

,                          (2)

also called the heat equation.

 

Diffusion displacement

The diffusion displacement can be described by the following formula:

  <rk2> = 2kD’t,

where k is the dimensions of the system and can be one, two or three. D’ is the diffusion coefficient, but now also per unit of concentration difference of the particles and t is time. For the three-dimensional systems the above equation will be:

   <x2> +  <y2> +  <z2> =  <r32> = 6D’t,

where < > indicates the mean of the squared displacement of the individual particles.

 

Biological numeric example

Calculate the time required for O2 diffusion across the alveolar-capillar membrane. By knowing D’ of oxygen in watery tissue (suppose 15x10-10 m2s-1bar-1), the 1D-distance of diffusion x (suppose the distance between alveolar and capillary volume is0.4 μm) and the O2 diffusion gradient Δp is 0.09 bar (suppose partial pressures of 0.14 bar in alveoli and 0.05 bar in A. pulmonalis) and supposing that the system is ideal (half infinite at both sides and a constant gradient), then the time required for the diffusion of O2 from the alveoli to the alveolar capillaries can be calculated:

 t = x2/(2DΔp) = 0.16x10-12/(2x15x10-10x0.09) = 0.6x10-3 s.

 

See further Fick's laws, for the diffusion equations and Grahams Law for particle velocity of diffusing particles.