Partition function of quantum mechanics

In summary, there is a mathematical connection between the partition function in quantum mechanics and the partition function in thermodynamics. This is expressed by the fact that inverse temperature is an imaginary time, and is also crucial for many-body quantum field theory in thermal equilibrium. In the imaginary-time or Matsubara formulation, time becomes purely imaginary and the fields are subject to periodic or antiperiodic boundary conditions. This leads to the same Feynman rules for perturbation theory, but with some changes compared to the vacuum case. This has been explored in detail in the context of relativistic thermal quantum field theory.
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In quantum mechanics, we have the partition function Z[j] = e-W[j] = ∫ eiS+ jiOi. The propagator between two points 1 and 2 can be calculated as

## \frac{\delta}{\delta j_1}\frac{\delta}{\delta j_2} Z = \langle O_1 O_2 \rangle##

The S in the path integral has been replaced by S → S + jiOi. Similarly we have what is also called the partition function in thermodynamics, Z[β] = e-F = tr e-βH, where F = E - TS is the free energy. The average energy can be calculated as

## \langle E \rangle = \frac{\partial Z}{\partial \beta} ##

When you add heat to a gas at constant pressure, the change in the enthalpy H = U + PV is equal to the heat added. The gas has to expand to keep the pressure constant. The work PdV done by this expansion is automatically accounted for by the definition of H, which is analogous to the above formula for the transformation of S. What is the connection between these two types of partition functions?
 
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The connection is mathematical, but I don't think that there is a deep physical connection. The mathematical connection is sometimes expressed concisely by saying that inverse temperature is an imaginary time.
 
  • #3
To the contrary this similarity is crucial for many-body quantum field theory in thermal equilibrium. It's used in the socalled imaginary-time or Matsubara formulation of thermal field theory. The only difference to the vacuum case is that time becomes purely imaginary, ##t=-\mathrm{i} \tau## with ##\tau \in (0,\beta)## with ##\beta=1/(k_{\text{B}} t)## and the fields are subject to periodic (bosons) or antiperiodic (fermions) boundary conditions. You get the same Feynman rules for perturbation theory with some changes compared to the vacuum case: Instead of energy integrals you have sums over the Matsubara frequencies ##\omega_k=2 \pi k_{\text{B}} T k## (bosons) or ##\omega_k = \pi(2 k+1) k_{\text{B}} T## with ##k \in \mathbb{Z}## (I've chosen natural units with ##\hbar=c=1##).

For details (relativistic thermal QFT), see

https://itp.uni-frankfurt.de/~hees/publ/off-eq-qft.pdf
 
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FAQ: Partition function of quantum mechanics

What is the partition function in quantum mechanics?

The partition function in quantum mechanics is a mathematical tool used to calculate the thermodynamic properties of a quantum system. It takes into account the energy levels and degeneracy of the system to determine the probability of each energy state being occupied.

How is the partition function calculated?

The partition function is calculated by summing over all possible energy states of the system, weighted by the Boltzmann factor, which takes into account the temperature and energy of each state. This sum is then multiplied by the degeneracy of each state.

What is the significance of the partition function?

The partition function is a key concept in statistical mechanics and is used to calculate important thermodynamic quantities such as the free energy, entropy, and specific heat of a quantum system. It also provides insights into the behavior of complex systems and helps in understanding phase transitions.

How does the partition function relate to the density of states?

The partition function is directly related to the density of states, which is a measure of the number of energy states available to a system. The partition function takes into account the degeneracy of each energy state, which is included in the density of states.

Can the partition function be extended to classical systems?

Yes, the partition function can be extended to classical systems by using the classical Boltzmann factor, which takes into account the classical energy levels and temperature. However, in the classical limit, the partition function reduces to the classical partition function.

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