Thermal field theory and imaginary time
Derive the thermal boundary condition from a trace and connect Matsubara frequencies with equilibrium occupations.
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The question for today
What you’ll understand
- Derive the KMS identity with an explicit time-evolution convention.
- Obtain bosonic and fermionic imaginary-time frequencies from boundary conditions.
- Separate equilibrium Euclidean information from real-time transport claims.
Temperature changes the state in which a quantum theory is evaluated. Instead of a vacuum expectation value, an equilibrium observable is weighted by a thermal density matrix. The trace behind that weighting becomes a boundary condition in imaginary time. We set Boltzmann's constant, Planck's constant, and the speed of light to one, assume zero chemical potential, and work in thermal equilibrium.
A trace explains the imaginary-time circle
For Hamiltonian , define and with . Real-time evolution is . Analytically continuing to inserts on the left of and on the right. Cyclicity of the trace then moves the remaining thermal factor past the second operator.
This produces the Kubo–Martin–Schwinger relation. The raw operator trace identity does not acquire a universal fermionic minus sign; anticommutation signs enter when one defines time-ordered fermionic correlators and moves fields through the ordering operation. The analytic continuation assumes the correlators have the needed strip of analyticity. In field theory it is understood through appropriately defined correlation functions rather than arbitrary unbounded operators manipulated without domains.
Boundary conditions quantize imaginary-time frequencies
The Euclidean path integral for the trace joins initial and final configurations across an interval of length . Bosonic fields are periodic on that circle. Fermionic fields are antiperiodic in the thermal path integral, reflecting the Grassmann trace construction. Fourier modes must respect those conditions. A bosonic factor returns to itself at , whereas a fermionic factor returns with a minus sign.
Solving those elementary phase conditions gives integer and half-integer Matsubara frequencies. A zero bosonic frequency is allowed; there is no fermionic zero frequency in this thermal setup. This distinction matters at high temperature, where soft bosonic modes can dominate long-distance behavior and demand resummation or a lower-dimensional effective description. The mere discreteness of these Euclidean frequencies does not imply that real-time emitted particles have only those discrete energies.
Occupations are simple; dynamics can still be hard
A single bosonic oscillator of energy spacing has occupation weights proportional to for nonnegative integer . Summing a geometric series and differentiating its logarithm gives the Bose occupation . The zero-point factor cancels from the normalized occupation. A fermionic mode allows only zero or one occupation, producing instead. These formulas describe noninteracting quasiparticle modes when that description applies.
Interactions can change masses, widths, screening, and the validity of a quasiparticle picture. Even a small microscopic coupling does not ensure every thermal momentum scale is perturbative: infrared enhancements require a scale-by-scale analysis. Euclidean correlators also do not directly hand over a viscosity or relaxation rate. Those require real-time spectral information, and reconstructing it from finite noisy Euclidean data is an ill-conditioned inverse problem. Equilibrium thermodynamics, screening, and transport should be treated as related but different targets.
Work it through
Compare statistics at the same excitation energy
For βω = log 2, compute the bosonic and fermionic occupations. Then double βω and compare again.
At βω = log 2, the exponential is two. The Bose occupation is 1/(2 − 1) = 1, while the Fermi occupation is 1/(2 + 1) = 1/3.
At βω = 2 log 2 the exponential is four. The occupations become 1/3 and 1/5 respectively.
Increasing βω suppresses both occupations. A bosonic mean above one is permitted because many quanta can occupy a mode; a single fermionic mode remains bounded by one.
The distinction comes from the allowed occupation spectrum, not from a classical picture of hot particles moving on the imaginary-time circle.
The living notebook
Explore the model
Interactive lab · spectral
Explore a truncated periodic mode expansion
Change mode count N and decay p in the finite sum Σ sin(nx−t)/nᵖ. Inspect how more harmonics resolve shorter features. This is an analogy for a discrete Fourier expansion; its spatial harmonics are not a computed thermal propagator, Matsubara sum, or real-time spectral density.
- Sum at x = π/2
- 0.867
- Smallest wavelength
- 2π / 5
- Highest-mode coefficient
- 0.2
A finite sum of sin(nx − t)/nᵖ. Playback changes t; increasing the cutoff includes finer spatial scales. This is not a proof about a continuum limit or renormalization. Parameter changes pause playback and recompute the model at the current elapsed time. Reset restores both parameters and returns time to zero. Playback starts paused. Adjust either parameter, then choose Play or Step.
Look forA periodic domain supplies discrete Fourier labels, while the physical coefficients and correlation functions require a separate theory calculation.
Pause & reason
Check your understanding
Your turn
Try it yourself
Starting from a bosonic Fourier factor exp(iωτ), impose periodicity across β and derive its allowed frequencies. Explain why this alone cannot determine a transport coefficient.
Take a moment to make a prediction or work it out on paper. Open a hint when you need one.
Give me a hint
Require exp(iωβ) = 1; then distinguish a basis from the correlator expanded in that basis.
Compare with the solution
Periodicity gives , so . This specifies allowed Euclidean Fourier labels, but not the interacting correlator's values or its real-time low-frequency spectral behavior. Transport needs that additional dynamical information and a justified continuation or real-time calculation.
Keep the idea
Take it with you
- The thermal trace leads to KMS relations and imaginary-time boundary conditions.
- Bosonic and fermionic Matsubara frequencies encode different thermal boundary conditions.
- Real-time transport needs more than a formal Euclidean Fourier expansion.
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