12 October 1992
The Royal Swedish Academy of Sciences has decided to award the 1992 Nobel Prize in Chemistry
to Professor Rudolph A. Marcus, California Institute of Technology, Pasadena, California, USA
for his contributions to the theory of electron transfer reactions in chemical systems
A theory close to reality
Professor Rudolph A. Marcus is being rewarded for his theoretical work on electron transfer – work which has greatly stimulated experimental developments in chemistry. The processes Marcus has studied, the transfer of electrons between molecules in solution, underlie a number of exceptionally important chemical phenomena, and the practical consequences of his theory extend over all areas of chemistry. The Marcus theory describes, and makes predictions concerning, such widely differing phenomena as the fixation of light energy by green plants, photochemical production of fuel, chemiluminescence (“cold light”), the conductivity of electrically conducting polymers, corrosion, the methodology of electrochemical synthesis and analysis, and more.
From 1956 to 1965 Professor Marcus developed his theory for what is perhaps the simplest chemical elementary process, the transfer of an electron between two molecules. No chemical bonds are broken in such a reaction, but changes take place in the molecular structure of the reacting molecules and their nearest neighbours. This molecular change enables the electrons to jump between the molecules.
Professor Marcus found simple mathematical expressions for how the energy of the molecular system is affected by these changes. With these he was able to calculate and explain the greatly varying rates measured for electron transfer reactions. In the mathematical connection the Marcus theory makes between theoretical and experimental quantities, experimental chemists gained a valuable tool. The theory has proved useful in the interpretation of many chemical phenomena, even though it was initially controversial at some points. Certain predictions turned out to conflict with what the chemists had expected, and were also difficult to confirm experimentally. We had to wait for the final experimental confirmation until the latter part of the 1980s.
When two molecules in a solution exchange one or more electrons, there is a reduction/oxidation process (redox process) in which one molecule accepts the electrons (reduction) and the other loses them (oxidation). Several different mechanisms can underlie such reactions. The simplest is the transfer of one single electron from one molecule to another. Changes take place in the structure, both in the reacting molecules and in those of the solution medium. Because of all these changes the energy of the molecular system rises temporarily and enables the electron to jump between the molecules. Energy must thus be supplied for the electron to be able to cross an energy barrier. The size of the energy barrier determines the speed of the reaction. An electron transfer of this kind is the simplest chemical elementary process, and is eminently suitable for theoretical studies.
At the beginning of the 1950s it was possible to determine the speed of a number of electron transfers between inorganic ions. Some of the reactions turned out to be very slow, which was surprising in view of the fact that only one electron changed places. It was considered at the time that such an insignificant change should not give rise to any large energy barrier.
The prizewinner’s contributions
From 1956 to 1965 Marcus published a series of papers on electron transfer reactions. His work led to the solution of the problem of greatly varying reaction rates.
Marcus made two assumptions about the reacting molecules. First, they had to be very loosely bonded to each other during the course of the reaction for classical physical-chemical theory to apply. Secondly, he assumed that it is the solvent molecules in the immediate vicinity that change their positions, thus increasing the energy in the molecular system. The electron can only jump between two states that have the same energy, and this condition can be fulfilled only by increasing the energy for both molecules. Marcus found a simple mathematical formula for calculating this energy change and was thus also able to calculate the size of the energy barrier. Somewhat later he extended the theory to include the energy associated with changes in the bonds of the reacting molecules.
In addition, Marcus further developed his model by showing that energy barriers could be calculated as a sum of two terms characterising each of the two components of the reaction. Lastly, he derived a general connection between electron transfer speed and the free energy change of the reaction, its “driving force”.
The general equation is quadratic and describes a parabola (see figure). The formula has the interesting consequence, unexpected by the chemist’s intuition, that, for a sufficiently large driving force, the reaction ought to take place more slowly the larger the driving force becomes. This area even received a special name, “the inverted region”. In the 1960s this prediction ran completely counter to chemists’ expectations and, in addition, it was difficult to study reactions of this type experimentally. Marcus himself proposed in 1965 that chemiluminescence reactions of a certain type ought to represent the inverted region, but it was not until the end of the 1980s that other, more convincing, experimental verifications could be made.
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See them all presented here.