The Mandel Q parameter measures the departure of the occupation number distribution from Poissonian statistics. It was introduced in quantum optics by Leonard Mandel. It is a convenient way to characterize non-classical states with negative values indicating a sub-Poissonian statistics, which have no classical analog. It is defined as the normalized variance of the boson distribution:
Q = ⟨ ( Δ n ^ ) 2 ⟩ − ⟨ n ^ ⟩ ⟨ n ^ ⟩ = ⟨ n ^ 2 ⟩ − ⟨ n ^ ⟩ 2 ⟨ n ^ ⟩ − 1 = ⟨ n ^ ⟩ ( g ( 2 ) ( 0 ) − 1 ) {\displaystyle Q={\frac {\left\langle (\Delta {\hat {n}})^{2}\right\rangle -\langle {\hat {n}}\rangle }{\langle {\hat {n}}\rangle }}={\frac {\langle {\hat {n}}^{2}\rangle -\langle {\hat {n}}\rangle ^{2}}{\langle {\hat {n}}\rangle }}-1=\langle {\hat {n}}\rangle \left(g^{(2)}(0)-1\right)}
where n ^ {\displaystyle {\hat {n}}} is the photon number operator and g ( 2 ) {\displaystyle g^{(2)}} is the normalized second-order correlation function as defined by Glauber.
Non-classical value Negative values of Q corresponds to state which variance of photon number is less than the mean (equivalent to sub-Poissonian statistics). In this case, the phase space distribution cannot be interpreted as a classical probability distribution.
− 1 ≤ Q < 0 ⇔ 0 ≤ ⟨ ( Δ n ^ ) 2 ⟩ ≤ ⟨ n ^ ⟩ {\displaystyle -1\leq Q<0\Leftrightarrow 0\leq \langle (\Delta {\hat {n}})^{2}\rangle \leq \langle {\hat {n}}\rangle }
The minimal value Q = − 1 {\displaystyle Q=-1} is obtained for photon number states (Fock states), which by definition have a well-defined number of photons and for which Δ n = 0 {\displaystyle \Delta n=0} .
Examples For black-body radiation, the phase-space functional is Gaussian. The resulting occupation distribution of the number state is characterized by a Bose–Einstein statistics for which Q = ⟨ n ⟩ {\displaystyle Q=\langle n\rangle } . Coherent states have a Poissonian photon-number statistics for which Q = 0 {\displaystyle Q=0} .
References
Further reading L. Mandel, E. Wolf Optical Coherence and Quantum Optics (Cambridge 1995) R. Loudon The Quantum Theory of Light (Oxford 2010)
