I was playing with Bloch's optical equations for a quantum system with two energetic levels in an external sinusoidal perturbation under Rotating Wave Approximation. Letting Feynman's vector $\vec R$ be $$\vec R=(2\Re\{\rho_{12}e^{i\omega t}\}, -2\Im\{\rho_{12}e^{i\omega t}\}, \rho_{11}-\rho_{22}),$$ one finds $$\dot{\vec R}=\vec R \times \vec B,$$ where $\vec B$ is a constant vector depending on $\omega$, on the eigenvalues of the unperturbed system, and on the strenght of the perturbation.
Clearly, the equation above expresses a rotation of $\vec R$, and, in particular, implies the conservation of its norm, so I evaluated it: $$\|\vec R\|^2=(\rho_{11}-\rho_{22})^2+4|\rho_{12}|^2=(\rho_{11}+\rho_{22})^2-4(\rho_{11} \rho_{22}-|\rho_{12}|^2).$$ The latter rearrangement clearly show that the conserved quantity is equal to $(\mathrm{tr} \rho)^2-4 \det(\rho)$. Now, of course one has $\mathrm{tr}\rho=1$, so I conclude that, in this case, $\det \rho$ is conserved.
Then I tried to figure out whether this is a general property of the density matrix. Given the usual Schrödinger Equation, it seems to me that it is verified at least in the finite-dimensional case. One in fact has $$i \hbar \dot \rho =[H, \rho],$$ whence, since the derivative of the determinant is given by $$\frac{\mathrm{d}}{\mathrm{d}t} A(t)=\det A(t) \mathrm{tr} (A(t)^{-1} \dot A(t)),$$ it follows that $$i \hbar \frac{\mathrm{d}}{\mathrm{d}t} \rho= \det \rho \mathrm{tr} (\rho^{-1} [H, \rho]) =\det\rho \mathrm{tr}(\rho^{-1}H\rho-H)=0,$$ the last equality following from ciclicity if trace.
Is it right what I've done here? Does the statement hold in more general conditions? Does anybody know where could I learn more about it or about related topics?