First order correlation function and power spectrum

The set of operators that are needed to compute the correlator of interest, namely $ \langle\ud{b}(t)b(t+\tau)\rangle $, are the most general set $ \{C_{\{m,n\}}=\ud{b}^mb^n\}$, differently than for the harmonic oscillator in Section 2.6. The regression matrix $ M$ is defined by the following rules:

\begin{subequations}\begin{align}&M_{\substack{mn\\ mn}}=i\omega_b(m-n)+i\frac{U...
...iU(m-n)\,,\\ &M_{\substack{mn\\ m-1,n-1}}=P_bmn\,. \end{align}\end{subequations}

Figure 5.1: Chain of correlators--indexed by  $ \{\eta\}=(m,n)$--linked by the Hamiltonian dynamics with pump and decay for one AO. On the left (resp., right), the set  $ \mathcal{N}_k$ (resp., $ \tilde{\mathcal{N}}_k$) involved in the equations of the two-time (resp., single-time) correlators. In green is shown the first manifold. The equation of motion  $ \langle
\ud{b}(t)C_{\{\eta\}}(t+\tau)\rangle$ with $ \eta\in\mathcal{N}_1$ requires for its initial value the correlator  $ \langle
C_{\{\tilde\eta\}}\rangle$ with  $ \{\tilde\eta\}\in\tilde{\mathcal{N}}_1$ defined from  $ \{\eta\}=(m,n)$ by  $ \{\tilde\eta\}=(m+1,n)$, as seen on the diagram. The arrows show the connections due to the incoherent pumpings $ P_b$ (in green) and the interactions (in red). The sense of the arrows indicates which element is ``calling'' which in its equations. The self-coupling of each node to itself is shown in violet circular arrow (affected by $ \omega_b$, $ \Gamma_b$ and $ U$). These links are obtained from the rules in Eq. (5.2a). The dimension of the manifolds is always one. A manifold $ k$ is only linked directly to $ k\pm 1$ in this model.
\includegraphics[width=.45\linewidth]{chap5/AO/fig1-correlator.ps}

This gives rise to an infinite set of coupled equations for any general correlator. $ \langle\ud{b}(t)b(t+\tau)\rangle $ is linked to all correlators of the kind:

$\displaystyle C_n(t,t+\tau)=\langle\ud{b}(t)(\ud{b}^{n-1}b^n)(t+\tau)\rangle$ (5.3)

with $ n=1$, 2, ... (see Fig. 5.1), through the general equation:
\begin{subequations}\begin{align}\frac{d}{d\tau}C_n(t,t+\tau)=&-\big[i\omega_b+i...
...-iUC_{n+1}(t,t+\tau)+n(n-1)P_bC_{n-1}(t,t+\tau)\,. \end{align}\end{subequations}

$ \Gamma_b=\gamma_b-P_b$ is the effective boson broadening, that we have already encountered many times.5.2Also here, we can write the general equation in a matrix form, $ d\mathbf{v}(t,\tau)/d\tau=-\mathbf{M}_1\mathbf{v}(t,\tau)$ where $ \mathbf{v}$ is the vector of the ordered correlators $ C_n(t,t+\tau)$ ($ n=1$, 2, ...) and $ \mathbf{M}_1$ the corresponding nondiagonal regression matrix extracted from Eq. (5.4). Finally, we integrate $ C_n(t,t+\tau)=e^{-\mathbf{M}_1\tau}\,C_n(t,t)$. The initial average values for the correlators $ C_n(t,t)=\langle\ud{b}^nb^n\rangle (t)$ can be found through the density matrix,

$\displaystyle C_n(t,t)=\sum_{j=n}^{\infty}\frac{j!}{(j-n)!}\rho_{jj}(t)\,,$ (5.5)

or applying again the quantum regression formula. The second set of equations,

$\displaystyle \frac{d}{dt}C_n(t,t)=-n\Gamma_bC_n(t,t)+n^2P_bC_{n-1}(t,t)\,,$ (5.6)

are easily solved in the two cases we are interested in. The steady state (SS) is, as we said, the thermal state [Eqs. (2.34)-(2.35)] for which $ C_n^\mathrm{SS}=n!n_b^n$ and $ n_b=P_b/\Gamma_b$. The spontaneous decay (SE) from an initial state defined by $ C_n^0=\langle\ud{b}^n b^n\rangle (0)$ gives simply $ C_n^\mathrm{SE}(t,t)=e^{-n\gamma_b t}C_n^0$. In both cases, the mean single-time values do not depend on the interactions. They are the same than for the HO.

The correlators $ C_n(t,t+\tau)$ cannot be found analytically in the general case with pump because the Hilbert space is infinite ( $ n \in
[1,\infty)$). The formula (2.105) of the spectra must be kept in general terms for the SS emission.



Subsections
Elena del Valle ©2009-2010-2011-2012.