Figure 2
From: On the statistical background of quantum mechanics: generalities and a concrete example
Probability of emission of the next fluorescence photon at time t after an emission at time 0, denoted \(\ell (\tau )\) in the text. Solid lines for our Kolmogorov model, dashed lines for the radiative cascade description, Eq. (4) in Ref. [2], or Eq. (2.14) in Ref. [6]. (a) strong-damping regime, \(\gamma =10 \Omega \). (b) \(\gamma =\Omega \). (c) strong-pumping regime, \(\gamma =0.2 \Omega \). The characteristic times of the distributions approximately agree in (c), whereas they noticeably diverge in (a), see a possible explanation in the text. Our coefficient γ corresponds to Γ defined in [6] and [2]