Abstract
At the present time, our understanding of macromolecular photochemistry is guided by the recognition that the overall photolysis reaction is attributed to a combination of mechanisms each of which would have to be studied independently for a proper understanding of the photoelimination process. Isolation of each mechanism is often experimentally difficult to achieve, and the need often arises for an analytical method which can predict and explain the behavior of complex photochemical systems. Our initial1 analytical description of the course of photoelimination reactions was concerned primarily with the rates of production and annihilation of electronically excited intermediates, rather than with the energy content and electronic configuration of the separate states. The basis for the earlier kinetic description was that the quantum yield of product formation, ØPC,2 is given by the summation equation,
where ØT is the triplet yield, ØI is the singlet and triplet radia-tionless relaxation yield, ØL is the total luminescence yield, and ØREV represents relaxation via reversible processes yielding no net photochemical reaction. The magnitude of each of these competing processes and the yield for product formation could be readily estimated by the kinetic analysis.1
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Reinisch, R.F., Gloria, H.R., Androes, G.M. (1970). Photoelimination Reactions of Macromolecules. In: Reinisch, R.F. (eds) Photochemistry of Macromolecules. Springer, Boston, MA. https://doi.org/10.1007/978-1-4684-8035-1_16
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