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Practice of Kinetics (Comprehensive Chemical Kinetics, Volume 1)

Practice of Kinetics (Comprehensive Chemical Kinetics, Volume 1)

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334 DETECTION AND ESTIMATION OF INTERMEDIATESSolid state spectra are, in general, broader than the corresponding gas-phasespectra, and there may be some frequency shift <strong>of</strong> the various spectroscopicfeatures. Thus some care must be exercised before absorptions in the solid phaseare ascribed to particular species on the basis <strong>of</strong> gas-phase identifications. Furthercomplications introduced by the matrix include splittings and changes in oscillatorstrength <strong>of</strong> optical transitions, but these effects may not themselves interferewith correct identification <strong>of</strong> the absorbing species. The nature <strong>of</strong> thematrix shifts is not understood, although some empirical data has been collected.McCarty and Robinson305 examined the matrix shifts in different matrices <strong>of</strong> the3P1-'S0 resonance line <strong>of</strong> atomic mercury, and this work has been extended byBrewer et aL306. Meyer3" finds that the absorption features <strong>of</strong> atomic sodiumor potassium in argon, krypton or xenon matrices are shifted to the blue, andthat there are signs <strong>of</strong> a triplet structure. If the matrix sample be warmed up, theabsorptions broaden and shift to the red. Barger and Broida308n309 have madesimilar studies <strong>of</strong> radical species in the region 3000-4500 A. A Knudsen cell wasused to produce a molecular beam <strong>of</strong> known density <strong>of</strong> C, C2 and C,. In the case308<strong>of</strong> C3 trapped in Ar, Kr, Xe, O,, N,, CO, and SF6 matrices it was found that theline widths <strong>of</strong> the 'n, t 'El transition varied from 40 to 500 cm-', while theline shifts were in the range 410 to 1065 cm-' (all positive, except with a carbondioxide matrix, in which a red shift was observed). There was no definite effect <strong>of</strong>temperature, nor did there appear to be any great effect <strong>of</strong> the matrix on intensities.Experiments309 on the species C, were less successful, and identifications werepossible only for the species trapped in carbon dioxide. With this matrix, 5 bands<strong>of</strong> the A34 t X3n, (Swan) system, and 4 bands <strong>of</strong> the forbidden A3nU t X'Z;system were observed.The blue solid prepared by trapping the pyrolysis (or electric discharge) products<strong>of</strong> HN, has been mentioned already, and the solid was one <strong>of</strong> the lirstsubjects <strong>of</strong> infrared matrix isolation study. Dows et d310 were able to ascribe most<strong>of</strong> the infrared absorption features <strong>of</strong> the solid to HN,, NH,N, and NH,, andfrom the behaviour <strong>of</strong> the spectrum on warming the solid up from 90"K, theywere able to show that further absorption bands were associated with the species(NH),(x > 2 and may be 4). During the warming up process, di-imide, N2H2,appears, and the presence <strong>of</strong> imidogen, NH, at 90" K was inferred. Milligan andJacox3" obtained the infrared absorption <strong>of</strong> NH and DH by the photolysis <strong>of</strong>HN3 and DN, in Ar, N, and CO matrices at 4" K, 14" K and 20" K. It wasshown that an appreciable concentration <strong>of</strong> NH was present in the ground, 'Z-,state, and from the reactivity observed in the CO matrix it was inferred that aside reaction is the appearance <strong>of</strong> H atoms by rupture <strong>of</strong> the H-N bond in HN3.Identification <strong>of</strong> NH and N,H, in the photolysis <strong>of</strong> HN,-N, matrices at 20" Khas been made unequivocal by studying the effect <strong>of</strong> substitution in HN, <strong>of</strong> H byD and 14N by 15N in the different positions312. Both cis- and trans-forms <strong>of</strong> N2H2were observed. NH appears as well as NH2 in the vacuum ultraviolet photolysis3'

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