research26 min studyLesson 77 in Physics

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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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 HH, define Z=Tr⁡e−βHZ=\operatorname{Tr}e^{-\beta H} and ⟨O⟩β=Z−1Tr⁡(e−βHO)\langle O\rangle_\beta=Z^{-1}\operatorname{Tr}(e^{-\beta H}O) with β=1/T\beta=1/T. Real-time evolution is A(t)=eiHtAe−iHtA(t)=e^{iHt}Ae^{-iHt}. Analytically continuing to t−iβt-i\beta inserts eβHe^{\beta H} on the left of A(t)A(t) and e−βHe^{-\beta H} 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.

⟨A(t−iβ)B(0)⟩β=⟨B(0)A(t)⟩β,Z=Tr⁡e−βH\langle A(t-i\beta)B(0)\rangle_\beta=\langle B(0)A(t)\rangle_\beta,\qquad Z=\operatorname{Tr}e^{-\beta H}
KMS identity for the stated Heisenberg convention and ordinary thermal trace at zero chemical potential. Fermionic time-ordering conventions must be handled separately.↔ Scroll wide equations horizontally.

Boundary conditions quantize imaginary-time frequencies

The Euclidean path integral for the trace joins initial and final configurations across an interval of length β\beta. 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 eiωnτe^{i\omega_n\tau} returns to itself at τ+β\tau+\beta, 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.

ωn(B)=2πnT,ωn(F)=(2n+1)πT,n∈Z\omega_n^{(B)}=2\pi nT,\qquad \omega_n^{(F)}=(2n+1)\pi T,\qquad n\in\mathbb Z
These are Fourier frequencies for periodic bosonic and antiperiodic fermionic Euclidean fields on 0 ≤ τ < β, at zero chemical potential.↔ Scroll wide equations horizontally.

Occupations are simple; dynamics can still be hard

A single bosonic oscillator of energy spacing ω>0\omega>0 has occupation weights proportional to e−βωne^{-\beta\omega n} for nonnegative integer nn. Summing a geometric series and differentiating its logarithm gives the Bose occupation 1/(eβω−1)1/(e^{\beta\omega}-1). The zero-point factor cancels from the normalized occupation. A fermionic mode allows only zero or one occupation, producing 1/(eβω+1)1/(e^{\beta\omega}+1) 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.

nB(ω)=1eβω−1,nF(ω)=1eβω+1n_B(\omega)=\frac{1}{e^{\beta\omega}-1},\qquad n_F(\omega)=\frac{1}{e^{\beta\omega}+1}
Mean occupation of a free bosonic or fermionic mode of positive excitation energy at zero chemical potential. These are not complete interacting thermal spectral functions.↔ Scroll wide equations horizontally.

Compare statistics at the same excitation energy

For βω = log 2, compute the bosonic and fermionic occupations. Then double βω and compare again.

  1. 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.

  2. At βω = 2 log 2 the exponential is four. The occupations become 1/3 and 1/5 respectively.

  3. 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 result

The distinction comes from the allowed occupation spectrum, not from a classical picture of hot particles moving on the imaginary-time circle.

Explore the model

Interactive lab

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.

Explore a truncated periodic mode expansionA 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. Current readings: Sum at x = π/2: 0.867; Smallest wavelength: 2π / 5; Highest-mode coefficient: 0.2. All parameters are adjustable with the labeled controls below.01.573.144.716.28−2.56−1.2801.282.56x · radiansFinite sine sum
Finite sumHighest included mode
Sum at x = π/2
0.867
Smallest wavelength
2π / 5
Highest-mode coefficient
0.2
t = 0 s

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.

Check your understanding

What is the zero-frequency distinction in the usual equilibrium imaginary-time formalism?

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 ωβ=2πn\omega\beta=2\pi n, so ω=2πnT\omega=2\pi nT. 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.

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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