Undergrad Doubt about partition functions in QFT and in stat Mechanics

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The discussion revolves around the relationship between the partition functions in statistical mechanics for a fermion gas and in quantum field theory (QFT) for a Dirac action. The user expresses confusion about how these two seemingly analogous systems, which share Hamiltonians, relate to each other. A key point made is that the Wick rotation and periodic time lead to a connection between the two partition functions, with the QFT result resembling the Fermi-Dirac partition function but with an energy shift and different normalization. The user also contemplates the implications of Grassmann variables in the context of these calculations. Overall, the conversation highlights the intricate connections between statistical mechanics and QFT, emphasizing the importance of understanding these relationships in theoretical physics.
Iliody
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Hi, I was studying for my final exam on statistical physics and a doubt raised on my head that was truly strong and disturbing (at least, for me), and that I couldn't answer to myself by now.

The doubt is: Given that we have in d dimensions a fermion non interacting gas, the statistical mechanics partition function will be

Z=∏p∈R^{d+1}, spin∈Z2 (1+e^{-β√(p2+m2)}))
"=det(1+e^{-β√(p2+m2)}))",
and in (d-1)+1 dimensions for a Dirac action will have as wick-rotated partition function

Z(β)=det(β(iγ⋅∂+m))

Are both related in some way?

I mean, they are systems with the same Hamiltonians, and given that there is a lot of analogies between the formalisms of QFT and statistical physics I though that both needed to be a little more similar...

Is there a relation between the two that I am not seeing? What's wrong with my intuition? I will be very grateful for any answer (if it isn't on the line of "Quantum Field Theory is a myth, the real thing is Aliens").

Sorry if this question was against the rules (I don't know for now if it could be).

(After posting this question here, I posted in phys*** st**kexc***ge, but I deleted from that place... Is that wrong? Sorry)
 
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Because I can't edit the post (I know that there are good reasons for that), I will retype the mathematical expressions using LaTex, for making them more understandable:
1-Fermi-Dirac in Statistical mechanics:
Z_{F-D}=\prod_{p\in \mathbb{R}^{d+1}} \prod_{s\in\{-\frac{1}{2},\frac{1}{2}\}} (1+e^{-\beta\sqrt{p^2+m^2}})
Z_{F-D}=det(1+e^{-\beta\sqrt{p^2+m^2}})
2-Dirac in QFT
Z_{Dirac-QFT}=det(\beta(m+i \displaystyle{\not} \partial))
 
Explaining a little more:
-The trouble I hace is un the difference between \sum_n \rangle n | e^{-\beta \hat{H}} | n \langle [\tex] and \int \prod_{i\in fieldcomponents} e^{-\beta H} [\tex]<br /> <br /> If a field is grassman-like, in the first case we sum between "mide is turn on"+" mode is turn off", but in the other case we only take into account the case un which it's turn con only?<br /> Something similar appears to happen in the bosonic case (difference of partition function "per mode")
 
Homer simpson doh:
I remembered today, talking with a friend, that this thing was there in the advanced qft course that we had taken. It's useful that I post here the answer in a few days, if someone has the same question? Or it's better for this post to be deleted and be burned in the oblivion ice's?

Cheers to the community.
 
In my opinion, posting the solution would be more useful.
 
OK, well... this is a pretty standard thermal QFT calculation:

*First: When we do the Wick rotation and make the time periodic (With time period = \hbar \beta), we have as log of partition function <br /> log Z_{Dirac-QFT}=Tr[ln(\prod_{n+1\in 2\mathbb{Z}} \beta(m+i \gamma \cdot \nabla + \gamma_0 \frac{2\pi n}{\beta}))]=\frac{1}{2}Tr[ln(\prod_{n+1\in 2\mathbb{Z}} (\beta^2(m^2+p^2)+4\pi^2 n^2))]=Tr[ln(\prod_{n-1\in 2\mathbb{N}} (\frac{\beta^2(m^2+p^2)}{4\pi^2 n^2}+1))]+const=Tr[ln(cosh(\frac{\beta\sqrt{m^2+p^2}}{2}))]+const=Tr[ln(1+exp(-\beta\sqrt{m^2+p^2}))]+Tr[ln(exp(\frac{\beta\sqrt{m^2+p^2}}{2}))]+const<br />. The former is equal to the fermi-dirac partition function plus an energy shift and with a different normalization.
 
Time reversal invariant Hamiltonians must satisfy ##[H,\Theta]=0## where ##\Theta## is time reversal operator. However, in some texts (for example see Many-body Quantum Theory in Condensed Matter Physics an introduction, HENRIK BRUUS and KARSTEN FLENSBERG, Corrected version: 14 January 2016, section 7.1.4) the time reversal invariant condition is introduced as ##H=H^*##. How these two conditions are identical?

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