3
$\begingroup$

I see this question was asked several times before but I don't think any answer can explain the issue perfectly. I am studying many body theory and encounters finite temperature Green's function. At first glance, it seems to me that the correct time dependence of, let's say a greater green's function, would be

$$ \begin{align*} G^{>}\left(\vec{r},\sigma,t;\vec{r}',\sigma',t'\right)&=-i\left\langle c_{\vec{r},\sigma}(t),c_{\vec{r}',\sigma'}^{\dagger}(t')\right\rangle \\ &=-\frac{i}{Z}\mathrm{tr}\left[e^{-\beta\left(\hat{H}-\mu\hat{N}\right)}e^{i\hat{H}t}c_{\vec{r},\sigma}e^{-i\hat{H}t}e^{i\hat{H}t'}c_{\vec{r}',\sigma'}^{\dagger}e^{-i\hat{H}t'}\right] \end{align*} $$

However, some texts used the "grand canonical Hamiltonian" $H_{G}=H-\mu N$ for the operators. Some said it is a natural way to "define" the time evolution, some don't even say anything at the beginning and include $\mu$ in all the Hamiltonian, some say it is merely a parameter but not chemical potential.

Of course if $\left[\hat{H},\hat{N}\right]=0$, such a change in Hamiltonian just introduces an extra phase factor like $e^{i\mu\left(t-t'\right)}$ to the Green's function and the change can be reversed at the final result easily. BUT if $\left[\hat{H},\hat{N}\right]\neq 0$ like a BCS hamiltonian, diagonalizing $\hat{H}$ and diagonalizing $\hat{H}_{G}$ give two completely different set of "eigen-operators" like $$ \begin{align*} \hat{H}&=\sum_{i\sigma}E_{i\sigma}\hat{\gamma}^{\dagger}_{i\sigma}\hat{\gamma}_{i\sigma}\\ \hat{H}_{G}&=\sum_{i\sigma}\tilde{E}_{i\sigma}\hat{\tilde{\gamma}}^{\dagger}_{i\sigma}\hat{\tilde{\gamma}}_{i\sigma} \end{align*} $$ In this case, changing $H$ to $H_G$ in the green's function will not just produce a phase factor but instead you are really calculating something very different.

Is there some theoretical reason that requires the time evolution is generated by $H_G$ instead of $H$?

$\endgroup$

1 Answer 1

0
$\begingroup$

Well, I remember, that I wasn't satisfied, when I saw the motivation of introducing this Hamiltonian in Landau&Lifshitz. Maybe the possible way to proceed is to start, from the grand-canocical ensemble, for which formula can be derived on the grounds of MaxEntropy method (maximisation of entropy subject to the conditions of conserved charges having fixed values). $$ Z = \text{Tr} e^{-\beta (H - \mu N)} $$ Where $\beta$ is Lagrange multiplier for conserved energy $E$, and $-\beta \mu$ for the number of particles. Having fixed these factors, one then proceeds with analogy to the evolution operator in Euclidean time: $$ e^{-\tau \hat{H}} $$

$\endgroup$

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.