“…It was proposed as a suitable method for lifetimes in atoms and molecules by Brannen et aZ(1955) and was used by them to obtain the value 11.2 k 0.2 ns for the lifetime of the 73S1 state of mercury. The method has since been used by Pardies (1968) and Camhy-Val and Dumont (1970) to measure this same lifetime in mercury, by Kaul (1966), Nussbaum andPipkin (1967) and Popp et aZ(l970) to measure the lifetime of the 63P1 level of mercury, by Camhy-Val, Dumont and co-workers (Camhy-Val and Dumont 1968b, Camhy-Val et a1 1969b, Dumont et aZ 1970 to measure five lifetimes in Ar 11, by Masterson and Stoner (1973) to measure the lifetime of the 3d' 2G7,2,9,8 levels in 0 11, and by Yamagishi and Inaba (1974) to measure the lifetimes of the 2pg and 2pg levels in Ne I, but these experiments (with the exception of that of Popp et aZ(l970)) have suffered from either a poor statistical accuracy or (in the case of the experiments of Camhy-Val, Dumont and co-workers) a high source pressure (of the order of 0.1 Torr or higher) and consequent possible systematic errors from radiation trapping and collisional de-excitation (see 991.3 and 5.6.1). It is only following the more recent work of Holt and Pipkin (1974) on the lifetime of the 73s1 level of Hg, of King et aZ(1975b) on the lifetime of the a 3&+ state of Hz, and of King et a2 (1976) on the lifetime of the 4p *D;iz level of Ar II that the full potential of the photon-photon coincidence method has become apparent.…”