Partition function of quantum mechanics

Click For Summary
SUMMARY

The discussion focuses on the partition function in quantum mechanics, defined as Z[j] = e-W[j] = ∫ eiS+ jiOi, and its connection to thermodynamics, where Z[β] = e-F = tr e-βH. The average energy is calculated using the formula ⟨E⟩ = ∂Z/∂β. The mathematical relationship between these partition functions is highlighted, particularly in the context of many-body quantum field theory in thermal equilibrium, utilizing the imaginary-time or Matsubara formulation. Key differences include the treatment of time as imaginary and the application of periodic or antiperiodic boundary conditions for fields.

PREREQUISITES
  • Understanding of quantum mechanics principles
  • Familiarity with statistical mechanics concepts
  • Knowledge of path integrals in quantum field theory
  • Basic grasp of thermodynamic functions such as free energy
NEXT STEPS
  • Study the derivation of the partition function in quantum mechanics
  • Learn about the Matsubara formalism in thermal field theory
  • Explore the implications of imaginary time in quantum mechanics
  • Investigate the role of boundary conditions in quantum field theories
USEFUL FOR

Physicists, particularly those specializing in quantum mechanics and quantum field theory, as well as students and researchers interested in the mathematical foundations of thermodynamics and statistical mechanics.

PGaccount
Messages
85
Reaction score
25
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The S in the path integral has been replaced by S → S + jiOi.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?
 
Physics news on Phys.org
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.
 
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
 
  • Like
Likes   Reactions: dextercioby

Similar threads

  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 4 ·
Replies
4
Views
494
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 6 ·
Replies
6
Views
3K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 1 ·
Replies
1
Views
2K
  • · Replies 9 ·
Replies
9
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K