3
$\begingroup$

The P-function of a state $\rho$ (focusing on the single-mode case) can be written as, using a notation analogous to the one in Gerry&Knight' book, $$P_\rho(\alpha) = \int \frac{d^2\eta}{\pi^2} \chi_N(\eta) e^{\alpha\bar\eta-\bar\alpha\eta}, \quad \chi_N(\eta)\equiv \operatorname{tr}[\rho\exp(\eta a^\dagger) \exp(-\bar\eta a)].$$ This also means that we should be able to write $P_\rho(\alpha)$ as the expectation value of some observable on $\rho$, i.e. $P_\rho(\alpha) = \operatorname{tr}(\mathcal O_P(\alpha)\rho)$, where I defined $$\mathcal O_P(\alpha) \equiv \int \frac{d^2\eta}{\pi^2} \exp(\eta A_\alpha^\dagger)\exp(-\bar\eta A_\alpha), \quad A_\alpha\equiv a-\alpha.$$ For reference, the same procedure is especially straightforward with the $Q$ function instead, and leads to $$\mathcal O_Q(\alpha) \equiv \int \frac{d^2\eta}{\pi^2} e^{-\bar\eta A_\alpha}e^{\eta A_\alpha^\dagger} = \int\frac{d^2\beta}{\pi}\int\frac{d^2\eta}{\pi^2} \mathbb{P}_\beta e^{-\bar\eta(\beta-\alpha)+\eta(\beta-\alpha)^*} = \frac1\pi \mathbb{P}_\alpha,$$ where I integrated over $\eta$ in the last step, and used the shorthand notation $\mathbb{P}_\beta\equiv|\beta\rangle\!\langle\beta|$. Of course, this recovers the well-known fact that $Q_\rho(\alpha)=\frac{\langle\alpha|\rho|\alpha\rangle}{\pi}$.

What I'm trying to figure out is whether there's any kind of similar calculation/simplification that can be done for $\mathcal O_P$. We can't simply add a $\mathbb{P}_\beta$ in between the operator exponentials, as they're in the wrong order. We can add two of them on left and right, but that would lead to $$\mathcal O_P(\alpha) = \int\frac{d^2\eta}{\pi^2} \int\frac{d^2\beta d^2\gamma}{\pi^2} \mathbb{P}_\beta\mathbb{P}_\gamma e^{\eta(\beta-\alpha)^*-\bar\eta(\gamma-\alpha)}.$$ The problem is that now the exponential over $\eta$ is problematic, and generally leads to exponential divergences unless $\beta,\gamma$ are suitably chosen. An alternative approach would be to exploit the usual commutation rules to write $$\mathcal O_P(\alpha) = \int \frac{d^2\eta}{\pi^2} e^{-\bar\eta A_\alpha}e^{\eta A_\alpha^\dagger} e^{|\eta|^2} = \int\frac{d^2\beta}{\pi}\mathbb{P}_\beta \int\frac{d^2\eta}{\pi^2} e^{\eta(\beta-\alpha)^*-\bar\eta(\beta-\alpha)+|\eta|^2}. $$ This looks slightly more "elegant", but throws the divergence problem in my face even stronger with the $\exp(|\eta|^2)$ term. Decomposed in real and imaginary parts, the argument in the exponential reads $$2i[\eta_2(\beta_1-\alpha_1)-\eta_1(\beta_2-\alpha_2)] + \eta_1^2+\eta_2^2,$$ which seems like it could never converge. Though I'm guessing convergence is still possible thanks to the exponential terms hidden $\mathbb{P}_\beta$ which might kill the $\eta$ terms. After all, we know that, for example, $\operatorname{tr}(\mathbb{P}_\gamma \mathcal O_Q(\alpha))=\delta^2(\alpha-\gamma)$.

Now, I'm aware that the $P$ function is highly irregular (can be more singular than a $\delta$ etc), so it is absolutely to be expected that $\mathcal O_P$ would be precisely as irregular as $P$. Still, singularities can often be dealt with and written concisely, at least at a formal level. Is there any way to simplify these expressions, or maybe put them in a form that makes it more evident that the singularities disappear in at least some cases?

$\endgroup$
1
  • 1
    $\begingroup$ doesn't answer the question, but I realised a similar way to define Wigner and other quasiprobability distributions in terms of expectation value wrt an observable is found in Ferrie's review, arxiv.org/abs/1010.2701, see chapter IIIA there. $\endgroup$
    – glS
    Commented Feb 25 at 18:24

1 Answer 1

0
$\begingroup$

I think I found the answer in one of the original 1969 papers by Kahill and Glauber, via some expressions I also discussed in Can we get quasiprobability distributions other than $P,Q,W$ from generalised characteristic functions?. In (Kahill and Glauber 1969, PhysRev.177.1857) the authors define (Eq. 6.6) $$T(\alpha,s) = \int\frac{d^2\xi}{\pi} \exp\left[ (\alpha-a)\bar\xi- (\bar\alpha-a^\dagger)\xi+\frac{s}{2}|\xi|^2\right],\tag{6.6}$$ and prove that this can be given the concise formal expression (Eq. 6.24) $$T(\alpha,s) = \frac{2}{1-s} \left(\frac{s+1}{s-1}\right)^{(a^\dagger-\bar\alpha)(a-\alpha)}.\tag{6.24}$$ Note that this $T$ function is essentially (a generalisation of) the observables $\mathcal O_P,\mathcal O_Q$ I defined above, and they are tied to the quasiprobability distributions via $$W_s(\alpha) \equiv\int\frac{d^2\eta}{\pi^2} \chi_s(\eta) e^{\alpha\bar\eta-\bar\alpha\eta} =\frac1\pi\operatorname{tr}[\rho T(\alpha,s)], \\ \chi_s(\eta) \equiv \operatorname{tr}[\rho\exp(\eta a^\dagger-\bar\eta a + s|\eta|^2/2)]. $$ In particular, $W_0(\alpha)=W(\alpha)$, $W_1(\alpha)=P(\alpha)$, and $W_{-1}(\alpha)=Q(\alpha)$, and thus $\mathcal O_P(\alpha)=\frac1\pi T(\alpha,1)$ and $\mathcal O_Q(\alpha)=\frac1\pi T(\alpha,-1)$. Which is compatible with them showing (Eq. 6.29) that $T(\alpha,-1)=|\alpha\rangle\!\langle\alpha|$.

It's clear from (6.24) that the $s=1$ case is particularly "troubling". This is mentioned by the authors around Eq. (7.22), and then later in their following paper (PhysRev.177.1882), where they define in (3.13, 3.15) the $P$ as $$P(\alpha) = \frac1\pi \operatorname{tr}[\rho T(\alpha,1)] \equiv \frac1\pi \lim_{s\to1^-} \operatorname{tr}[\rho T(\alpha,s)],$$ including also a discussion of its convergence.

$\endgroup$

Your Answer

By clicking “Post Your Answer”, you agree to our terms of service and acknowledge you have read our privacy policy.

Not the answer you're looking for? Browse other questions tagged or ask your own question.