Tunable diode laser absorption spectroscopy has been employed to measure the amount of N2O produced from laser flash photolysis of O-3/N-2/O-2 mixtures at 266 and 532 nm. In the 532 nm photolysis experiments very little N2O is observed, thus allowing an upper limit yield of 7 x 10(-8) to be established for the process O-3(+) + N-2 --> N2O + O-2, where O-3(+) is nascent O-3 that is newly formed via O(P-3(J)) + O-2 recombination (with vibrational excitation near the dissociation energy of O-3). The measured upper limit yield is a factor of similar to600 smaller than a previous literature value and is approximately a factor of 10 below the threshold for atmospheric importance. In the 266 nm photolysis experiments, significant N2O production is observed and the N2O quantum yield is found to increase linearly with pressure over the range 100-900 Torr in air bath gas. The source of N2O in the 266 nm photolysis experiments is believed to be the addition reaction O(D-1(2)) + N-2 + M -->(k6) N2O + M, although reaction of (very short-lived) electronically excited O-3 with N-2 cannot be ruled out by the available data. Assuming that all observed N2O comes from the O(D-1(2)) + N-2 + M reaction, the following expression describes the temperature dependence of k(6) (in its third-order low-pressure limit) that is consistent with the N2O yield data: k(6) = (2.8 +/- 0.1) x 10(-36)(T/300)(-(0.88+/-0.36)) cm(6) molecule(-2) s(-1), where the uncertainties are 2sigma and represent precision only. The accuracy of the reported rate coefficients at the 95% confidence level is estimated to be 30-40% depending on the temperature. Model calculations suggest that gas phase processes initiated by ozone absorption of a UV photon represent about 1.4% of the currently estimated global source strength of atmospheric N2O. However, these processes could account for a significant fraction of the oxygen mass-independent enrichment observed in atmospheric N2O, and they appear to be the first suggested photochemical mechanism that is capable of explaining the altitude dependence of the observed mass-independent isotopic signature.