photochemical equivalence law
- photochemical equivalence law
-
fundamental principle relating to chemical reactions (
chemical reaction) induced by
light, which states that for every
quantum of
radiation that is absorbed, one
molecule of the substance reacts. A quantum is a unit of
electromagnetic radiation with energy equal to the product of a constant ( Planck's constant,
h) and the frequency of the radiation, symbolized by the Greek letter nu (ν). In chemistry, the quantitative measure of substances is expressed in terms of gram moles (
mole), one gram mole comprising 6.02214179 × 10
23 ( Avogadro's number) molecules. Thus, the photochemical equivalence law is restated as: for every mole of a substance that reacts 6.02214179 × 10
23 quanta of light are absorbed.
The photochemical equivalence law applies to the part of a light-induced reaction that is referred to as the primary process; that is, the initial chemical change that results directly from the absorption of light. In most photochemical reactions (
photochemical reaction) the primary process is usually followed by so-called secondary processes that are normal interactions between reactants not requiring absorption of light. As a result such reactions do not appear to obey the one quantum–one molecule reactant relationship. The law is further restricted to conventional photochemical processes using light sources with moderate intensities; high-intensity light sources such as those used in flash
photolysis and in
laser experiments are known to cause so-called biphotonic processes;
i.e., the absorption by a molecule of a substance of two photons (
photon) of light.
The photochemical equivalence law is also sometimes called the Stark–Einstein law after the German-born physicists Johannes Stark (
Stark, Johannes) and Albert Einstein (
Einstein, Albert), who independently formulated the law between 1908 and 1913.
* * *
Universalium.
2010.
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