The literature contains three definitions of superradiant lifetime, standing in the ratio 1:2:4. The first may be defined by τRE=T₁Nμ, where μ is the geometrical factor of Rehler and Eberly. The second appears naturally in Dicke's equation ̇ \.φ=(τD)^-1sinφ. The third may be defined, following Arecchi and Courtens, by I=ω₀τAC for a maximally superradiant sample. For large Fresnel number, μ=(38π)λ²A; the numerical coefficient has been calculated incorrectly by some authors, so that the resulting formulas for superradiant lifetime do not match the definitions. The many superradiant lifetimes in current use are identified with the above three.
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Friedberg et al. (1976) studied this question.
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