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Practice of Kinetics (Comprehensive Chemical Kinetics, Volume 1)

Practice of Kinetics (Comprehensive Chemical Kinetics, Volume 1)

Practice of Kinetics (Comprehensive Chemical Kinetics, Volume 1)

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332 DETECTION AND ESTIMATION OF INTERMEDIATESConsideration will be given now to the requirements <strong>of</strong> a matrix that radicalstabilisation may occur and to the ways in which radicals may be introduced intothe matrix. In order that stabilisation <strong>of</strong> active species may occur, it is desirablethat the matrix material(i) is inert with respect to the active species;(ii) is sufficiently rigid to prevent diffusion <strong>of</strong> the active species; and(iii) has sites or holes suitable for the accommodation <strong>of</strong> the active species.The vapour pressure <strong>of</strong> the matrix must be low at the operating temperature(< 10- ’ torr), although it may be convenient if the vapour pressure is high enoughat room temperature to permit handling as a gas. Further restrictions on thematrix material are imposed by the method <strong>of</strong> detection which is to be employed.In particular, for spectroscopic investigation the matrix material must not absorbappreciably, and scattering must be reduced to a minimum. Some degree <strong>of</strong> compromisemay have to be accepted in the properties required. Thus glasses <strong>of</strong> etherisopentane-alcohol(EPA) are clear, and may be used for near-ultraviolet studies <strong>of</strong>trapped aromatic radicals2”, although the glass may absorb too strongly for usein infrared studies, and it may be too reactive to act as a good matrix for aliphaticradicals. On the other hand, the inert gases and nitrogen, which are chemicallyideal, frequently form highly scattering microcrystalline deposits when frozen.The temperature at which the matrix is formed may affect its scattering properties:Becker and PimentelZ9* find, for example, that xenon forms a fairly transparentmatrix if deposited at 60” K, but a highly scattering one if formed below 50°K.Scattering may be less <strong>of</strong> a problem in infrared studies than it is in visible or ultravioletexperiments, although against the reduced scattering must be set the muchsmaller oscillator strength <strong>of</strong> vibrational, rather than electronic, transitions.Radicals may be trapped in inert gas matrices in one <strong>of</strong> two main ways. First,the radicals may be prepared by a gas-phase reaction (i.e. by photochemical,thermal, electrical or chemical processes) and allowed to condense in the presence<strong>of</strong> the matrix material on a cold surface. Secondly, a matrix containing a precursor<strong>of</strong> the radical may be deposited, and the radical produced in the matrix by asolid-phase reaction. Photolysis <strong>of</strong> the precursor is the most controlled way <strong>of</strong>forming the radical, although the precursors are then restricted to photosensitivematerials. Again, the excess energy available in a photochemical reaction may besufficient for the radical(s) to escape from the matrix cage and primary recombinationmay occur. Gamma ray or X-ray radiolysis, or electron bombardment, <strong>of</strong>the solid is not restricted to photosensitive precursors, nor is the excess energylikely to be insufficient to allow the radicals to escape from the cage. In general,however, radiolysis and electron bombardment are too indiscriminating in theirattack, and photolysis remains the method <strong>of</strong> choice.Radicals may be produced also by secondary reactions with a reactive matrix<strong>of</strong> the radicals fist produced. For example, Milligan and Jacox2” have preparedHCO (DCO) by the photolysis <strong>of</strong> HI (DI) or H,S (D,S) in a matrix <strong>of</strong> solid carbon

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