Glauber–Sudarshan P representation
The Glauber–Sudarshan P representation is a suggested way of writing down the phase space distribution of a quantum system in the phase space formulation of quantum mechanics. The P representation is the quasiprobability distribution in which observables are expressed in normal order. In quantum optics, this representation, formally equivalent to several other representations, is sometimes championed over alternative representations to describe light in optical phase space, because typical optical observables, such as the particle number operator, are naturally expressed in normal order. It is named after George Sudarshan and Roy J. Glauber, who were working on the topic in 1963. It was the subject of a controversy when Glauber was awarded a share of the 2005 Nobel Prize in Physics for his work in this field and George Sudarshan's contribution was not recognized. Despite many useful applications in laser theory and coherence theory, the Glauber–Sudarshan P representation has the drawback that it is not always positive, and therefore is not a true probability function.
We also wish to construct the function such that the expectation value of a normally ordered operator satisfies the optical equivalence theorem. This implies that the density matrix should be in anti-normal order so that we can express the density matrix as a power series
Inserting the identity operator
we see that
and thus we formally assign
and then take the Fourier transform
Another useful integral formula for P is
Note that both of these integral formulas do not converge in any usual sense for "typical" systems . We may also use the matrix elements of in the Fock basis . The following formula shows that it is always possible to write the density matrix in this diagonal form without appealing to operator orderings using the inversion (given here for a single mode),
where r and θ are the amplitude and phase of α. Though this is a full formal solution of this possibility, it requires infinitely many derivatives of Dirac delta functions, far beyond the reach of any ordinary tempered distribution theory.
If the quantum system has a classical analog, e.g. a coherent state or thermal radiation, then P is non-negative everywhere like an ordinary probability distribution. If, however, the quantum system has no classical analog, e.g. an incoherent Fock state or entangled system, then P is negative somewhere or more singular than a Dirac delta function. (By a theorem of Schwartz, distributions that are more singular than the Dirac delta function are always negative somewhere.) Such "negative probability" or high degree of singularity is a feature inherent to the representation and does not diminish the meaningfulness of expectation values taken with respect to P. Even if P does behave like an ordinary probability distribution, however, the matter is not quite so simple. According to Mandel and Wolf: "The different coherent states are not [mutually] orthogonal, so that even if behaved like a true probability density [function], it would not describe probabilities of mutually exclusive states."
The P representation of the black body is
In other words, every mode of the black body is normally distributed in the basis of coherent states. Since P is positive and bounded, this system is essentially classical. This is actually quite a remarkable result because for thermal equilibrium the density matrix is also diagonal in the Fock basis, but Fock states are non-classical.
Highly singular example
Even very simple-looking states may exhibit highly non-classical behavior. Consider a superposition of two coherent states
where c0 , c1 are constants subject to the normalizing constraint
Note that this is quite different from a qubit because and are not orthogonal. As it is straightforward to calculate , we can use the Mehta formula above to compute P,
Despite having infinitely many derivatives of delta functions, P still obeys the optical equivalence theorem. If the expectation value of the number operator, for example, is taken with respect to the state vector or as a phase space average with respect to P, the two expectation values match:
- Quasiprobability distribution#Characteristic functions
- Nonclassical light
- Wigner quasiprobability distribution
- Husimi Q representation
- Nobel Prize controversies
- L. Cohen (1966). "Generalized phase-space distribution functions". J. Math. Phys. 7 (5): 781–786. Bibcode:1966JMP.....7..781C. doi:10.1063/1.1931206.
- L. Cohen (1976). "Quantization problem and variational principle in the phase space formulation of quantum mechanics". J. Math. Phys. 17 (10): 1863–1866. Bibcode:1976JMP....17.1863C. doi:10.1063/1.522807.
- E. C. G. Sudarshan (1963). "Equivalence of semiclassical and quantum mechanical descriptions of statistical light beams". Phys. Rev. Lett. 10 (7): 277–279. Bibcode:1963PhRvL..10..277S. doi:10.1103/PhysRevLett.10.277.
- R. J. Glauber (1963). "Coherent and incoherent states of the radiation field". Phys. Rev. 131 (6): 2766–2788. Bibcode:1963PhRv..131.2766G. doi:10.1103/PhysRev.131.2766.
- Zhou, Lulu (2005-12-06). "Scientists Question Nobel". The Harvard Crimson. Retrieved 2016-04-28.
- C. L. Mehta; E. C. G. Sudarshan (1965). "Relation between quantum and semiclassical description of optical coherence". Phys. Rev. 138 (1B): B274–B280. Bibcode:1965PhRv..138..274M. doi:10.1103/PhysRev.138.B274.
- C. L. Mehta (1967). "Diagonal coherent-state representation of quantum operators". Phys. Rev. Lett. 18 (18): 752–754. Bibcode:1967PhRvL..18..752M. doi:10.1103/PhysRevLett.18.752.
- Mandel & Wolf 1995, p. 541