Abstract
The vacuum-ultraviolet photolysis of acetylene isolated in Ar, Ne, and N2 matrices at 4° and at 14°K is shown to lead to the appearance of a number of visible-ultraviolet absorption bands which may be assigned to the species C2, as well as to an 1848 cm−1 infrared absorption assigned, with the aid of isotopic substitution studies, to the free radical HC2. The (0, 0) band of the Mulliken system of C2 is observed with great intensity at 2382 Å (Ar matrix) or at 2323 Å (Ne matrix) and the (2, 0), (3, 0), and (4, 0) bands of the Phillips system of C2 are observed in an Ar matrix at 8700, 7675, and 6880 Å, respectively, indicating that the x 1Σg+ state of C2 is the ground state of this species not only in the gas phase but also in the matrix. Features assigned by previous workers to the Swan transition of triplet C2 appear at 5206 and 4725 Å. A third member of the progression, not previously observed, appears at 4334 Å. Experiments utilizing C2D2 and C2H2 (58% 13C) support the assignment of these features to C2. The 5206-Å band system decreases in intensity and finally disappears when the sample is subjected to radiation of wavelength near 2500 Å. Problems associated with the assignment of these features are discussed, and a possible mechanism for their photolytic destruction is suggested.
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