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Entropy Production

Entropy production measures irreversibility. In open quantum systems it is the part of the entropy balance that cannot be assigned merely to heat exchanged with ideal reservoirs. It is the quantity that becomes nonnegative in a thermodynamically consistent Markovian model and that appears in fluctuation theorems as the log ratio of forward and reverse probabilities.

The most common weak-coupling convention is:

Σ˙=dSdt−∑αQ˙αTα,Σ˙≥0.\dot\Sigma = \frac{dS}{dt} - \sum_\alpha \frac{\dot Q_\alpha}{T_\alpha}, \qquad \dot\Sigma\ge0.

Here Q˙α\dot Q_\alpha is heat current into the system from bath α\alpha. With this sign convention, the entropy change of bath α\alpha is −Q˙α/Tα-\dot Q_\alpha/T_\alpha. The formula is powerful only when the currents and temperatures are defined by a physically consistent system-bath model.

The von Neumann entropy of a density operator is

S(ρ)=−kBTr⁡(ρln⁡ρ).S(\rho) = -k_B\operatorname{Tr}(\rho\ln\rho).

For trace-preserving differentiable dynamics,

dSdt=−kBTr⁡[ρ˙ln⁡ρ],\frac{dS}{dt} = -k_B \operatorname{Tr} \left[ \dot\rho\ln\rho \right],

with the usual support qualifications when ρ\rho has zero eigenvalues.

A closed system evolving unitarily has

ρ˙=−iℏ[H,ρ].\dot\rho = - \frac{i}{\hbar}[H,\rho].

Its eigenvalues are constant, so S(ρ)S(\rho) is constant. Entropy production for a reduced system appears because one traces out degrees of freedom, coarse-grains records, couples to reservoirs, or uses an irreversible effective equation.

For a Markovian open system,

ρ˙=−iℏ[H,ρ]+∑αLα(ρ),\dot\rho = - \frac{i}{\hbar}[H,\rho] + \sum_\alpha \mathcal L_\alpha(\rho),

the unitary commutator does not change S(ρ)S(\rho). The entropy balance is governed by the dissipators.

When Lα\mathcal L_\alpha represents a thermal bath at temperature TαT_\alpha, the standard heat current into the system is

Q˙α=Tr⁡[H Lα(ρ)].\dot Q_\alpha = \operatorname{Tr} \left[ H\,\mathcal L_\alpha(\rho) \right].

This definition assumes that HH is the Hamiltonian used by the bath rates and that interaction energy can be neglected or consistently absorbed into a renormalized Hamiltonian. It is safest for weak-coupling, secular, global thermal master equations. See Thermal Master Equations and Detailed Balance.

With heat currents into the system, the entropy flux from the reservoirs into the system is

Φ˙=∑αQ˙αTα.\dot\Phi = \sum_\alpha \frac{\dot Q_\alpha}{T_\alpha}.

The entropy balance is often written

dSdt=Σ˙+Φ˙,\frac{dS}{dt} = \dot\Sigma+\dot\Phi,

or equivalently

Σ˙=dSdt−Φ˙.\dot\Sigma = \frac{dS}{dt} - \dot\Phi.

The notation varies across books. The sign convention should always be stated before comparing formulas.

Spohn’s inequality is the standard positivity statement for quantum dynamical semigroups. Let L\mathcal L be a Gorini–Kossakowski–Sudarshan–Lindblad generator with stationary state π\pi:

L(π)=0.\mathcal L(\pi)=0.

Then

−Tr⁡[L(ρ)(ln⁡ρ−ln⁡π)]≥0- \operatorname{Tr} \left[ \mathcal L(\rho) \left( \ln\rho-\ln\pi \right) \right] \ge0

under the usual finite-dimensional support assumptions. Multiplying by kBk_B gives a nonnegative entropy-production rate associated with the relaxation generated by L\mathcal L:

Σ˙=−kBTr⁡[L(ρ)(ln⁡ρ−ln⁡π)]≥0.\dot\Sigma = - k_B \operatorname{Tr} \left[ \mathcal L(\rho) \left( \ln\rho-\ln\pi \right) \right] \ge0.

For a thermal generator with

π=ρβ=e−βHZ,\pi=\rho_\beta = \frac{e^{-\beta H}}{Z},

this becomes the familiar Clausius form. Since

ln⁡ρβ=−βH−ln⁡Z,\ln\rho_\beta = -\beta H-\ln Z,

and Tr⁡[L(ρ)]=0\operatorname{Tr}[\mathcal L(\rho)]=0, one finds

Σ˙=−kBTr⁡[L(ρ)ln⁡ρ]−1TTr⁡[HL(ρ)].\dot\Sigma = - k_B \operatorname{Tr} \left[ \mathcal L(\rho)\ln\rho \right] - \frac{1}{T} \operatorname{Tr} \left[ H\mathcal L(\rho) \right].

The first term is the dissipative contribution to dS/dtdS/dt, and the second is −Q˙/T-\dot Q/T. Thus

Σ˙=dSdt−Q˙T≥0\dot\Sigma = \frac{dS}{dt} - \frac{\dot Q}{T} \ge0

for a single thermal bath.

If each bath contribution Lα\mathcal L_\alpha has its own Gibbs stationary state for the same Hamiltonian HH,

ρβα=e−βαHZα,\rho_{\beta_\alpha} = \frac{e^{-\beta_\alpha H}}{Z_\alpha},

then the total entropy-production rate is

Σ˙=−kB∑αTr⁡[Lα(ρ)(ln⁡ρ−ln⁡ρβα)]≥0.\dot\Sigma = - k_B \sum_\alpha \operatorname{Tr} \left[ \mathcal L_\alpha(\rho) \left( \ln\rho-\ln\rho_{\beta_\alpha} \right) \right] \ge0.

Using the same heat-current convention, this reduces to

Σ˙=dSdt−∑αQ˙αTα.\dot\Sigma = \frac{dS}{dt} - \sum_\alpha \frac{\dot Q_\alpha}{T_\alpha}.

At a nonequilibrium steady state, dS/dt=0dS/dt=0, so

Σ˙ss=−∑αQ˙αTα.\dot\Sigma_{\mathrm{ss}} = - \sum_\alpha \frac{\dot Q_\alpha}{T_\alpha}.

For two baths with heat current JJ entering the system from the hot bath and leaving into the cold bath,

Q˙h=J,Q˙c=−J.\dot Q_h=J, \qquad \dot Q_c=-J.

Then

Σ˙ss=J(1Tc−1Th),\dot\Sigma_{\mathrm{ss}} = J \left( \frac{1}{T_c} - \frac{1}{T_h} \right),

which is nonnegative for Th>TcT_h>T_c and J≥0J\ge0. This is the Clausius statement that heat flows spontaneously from hot to cold.

The quantum relative entropy is

D(ρ∥σ)=Tr⁡[ρ(ln⁡ρ−ln⁡σ)],D(\rho\Vert\sigma) = \operatorname{Tr} \left[ \rho(\ln\rho-\ln\sigma) \right],

when the support of ρ\rho lies inside the support of σ\sigma. For a time-independent thermal semigroup with stationary state π\pi, Spohn’s inequality says that

ddtD(ρ(t)∥π)≤0.\frac{d}{dt} D(\rho(t)\Vert\pi) \le0.

The entropy-production rate is

Σ˙=−kBddtD(ρ(t)∥π)≥0.\dot\Sigma = - k_B \frac{d}{dt} D(\rho(t)\Vert\pi) \ge0.

Thus relaxation to equilibrium is monotonic in relative entropy, not necessarily in every intuitive distance or every observable. This is one reason relative entropy appears so often in rigorous thermodynamic statements.

For a thermal state ρβ\rho_\beta, the relative entropy identity

F(ρ)−F(ρβ)=kBT D(ρ∥ρβ)F(\rho)-F(\rho_\beta) = k_B T\,D(\rho\Vert\rho_\beta)

shows the same structure in equilibrium: dissipative relaxation lowers nonequilibrium free energy.

The ensemble rate Σ˙\dot\Sigma is not the only useful object. In quantum-jump or continuous-measurement descriptions, one can assign a trajectory entropy production

σ[γ]=ln⁡PF[γ]PR[γ~].\sigma[\gamma] = \ln \frac{P_F[\gamma]}{P_R[\tilde\gamma]}.

Its average gives the ensemble entropy production in the appropriate limit:

⟨σ⟩=ΣkB.\langle\sigma\rangle = \frac{\Sigma}{k_B}.

This is the bridge to Fluctuation Theorems. Individual trajectories may have σ<0\sigma\lt0, but the average is nonnegative when the forward and reverse ensembles satisfy the theorem’s assumptions.

For jump unravelings, local detailed balance of jump rates is essential. Without a physical identification of the jumps with reservoir energy exchange, a trajectory entropy-production formula may be only formal.

Quantum entropy production is not only about population relaxation. Pure dephasing can produce entropy without exchanging energy if the Hamiltonian is fixed and the dissipator destroys coherence in the energy basis. Then

Q˙=0,Σ˙=dSdt\dot Q=0, \qquad \dot\Sigma=\frac{dS}{dt}

for a consistent infinite-temperature or nondemolition dephasing model.

This does not mean coherence is “just entropy.” Coherence can be a resource for work extraction under suitable controls, can be converted into correlations, and can be hidden by the measurement scheme used to define work. The entropy-production statement depends on which operations, reservoirs, and records are included.

For a system coupled to a single initially thermal bath, suppose the initial state is factorized,

ρSB(0)=ρS(0)⊗ρBβ,\rho_{SB}(0) = \rho_S(0)\otimes\rho_B^\beta,

and the total evolution is unitary. If heat into the system is Q=−ΔEBQ=-\Delta E_B, the entropy production over a finite process is

ΣkB=ΔSSkB−βQ.\frac{\Sigma}{k_B} = \frac{\Delta S_S}{k_B} - \beta Q.

Under the same assumptions, this can be written as

ΣkB=IS:B(t)+D(ρB(t)∥ρBβ),\frac{\Sigma}{k_B} = I_{S:B}(t) + D(\rho_B(t)\Vert\rho_B^\beta),

where

IS:B=S(ρS)+S(ρB)−S(ρSB)kBI_{S:B} = \frac{ S(\rho_S)+S(\rho_B)-S(\rho_{SB}) }{k_B}

is the mutual information. The two terms on the right are nonnegative: irreversibility comes from system-bath correlations and from the bath being displaced away from its initial thermal state.

This identity is useful because it shows what a Markovian reservoir approximation discards. In the ideal reservoir limit the bath disturbance is unobserved and correlations are continuously coarse-grained, leaving an effective entropy-production rate for the reduced system.

The formula

Σ˙=dSdt−∑αQ˙αTα\dot\Sigma = \frac{dS}{dt} - \sum_\alpha \frac{\dot Q_\alpha}{T_\alpha}

is not automatically valid for every reduced equation. Problems arise when:

  • the interaction energy is not negligible;
  • the bath is finite or far from equilibrium;
  • the dissipator is local but the system Hamiltonian has strong internal coupling;
  • the generator is not derived from thermal correlations;
  • memory effects make heat temporarily reside in structured environmental modes;
  • initial system-bath correlations make the reduced map preparation-dependent.

At strong coupling one may need an enlarged system boundary, a reaction-coordinate mapping, an inclusive energy balance, or a Hamiltonian of mean force. For memory effects, see CP Divisibility and Reaction-Coordinate Mapping.

  • Identifying dS/dtdS/dt with entropy production even when heat flows are present.
  • Forgetting that Q˙α\dot Q_\alpha must have a sign convention.
  • Applying Spohn’s inequality to a dissipator without checking its stationary state.
  • Calling a positive-rate Lindblad equation thermodynamic without detailed balance.
  • Using local dissipators for an interacting system and assuming the second law follows automatically.
  • Treating negative trajectory entropy production as a violation of the second law.
  • Ignoring system-bath correlations in strong-coupling or non-Markovian regimes.
  • Mixing entropy in units of kBk_B with dimensionless entropy production without saying which is used.

Show that a closed quantum system evolving under ρ˙=−i[H,ρ]/ℏ\dot\rho=-i[H,\rho]/\hbar has constant von Neumann entropy.

Solution

Unitary evolution has the form

ρ(t)=U(t)ρ(0)U†(t).\rho(t) = U(t)\rho(0)U^\dagger(t).

Unitary conjugation preserves the eigenvalues of ρ\rho. Since

S(ρ)=−kB∑npnln⁡pnS(\rho) = -k_B\sum_n p_n\ln p_n

depends only on those eigenvalues, S(ρ(t))S(\rho(t)) is constant.

For a single thermal generator with stationary state ρβ=e−βH/Z\rho_\beta=e^{-\beta H}/Z, show that Spohn’s expression gives Σ˙=dS/dt−Q˙/T\dot\Sigma=dS/dt-\dot Q/T.

Solution

Start from

Σ˙=−kBTr⁡[L(ρ)(ln⁡ρ−ln⁡ρβ)].\dot\Sigma = - k_B \operatorname{Tr} \left[ \mathcal L(\rho) \left( \ln\rho-\ln\rho_\beta \right) \right].

Use

ln⁡ρβ=−βH−ln⁡Z.\ln\rho_\beta=-\beta H-\ln Z.

Because L\mathcal L is trace preserving,

Tr⁡[L(ρ)]=0,\operatorname{Tr}[\mathcal L(\rho)]=0,

so the ln⁡Z\ln Z term drops out. Then

Σ˙=−kBTr⁡[L(ρ)ln⁡ρ]−kBβTr⁡[HL(ρ)].\dot\Sigma = - k_B \operatorname{Tr}[\mathcal L(\rho)\ln\rho] - k_B\beta \operatorname{Tr}[H\mathcal L(\rho)].

The first term is dS/dtdS/dt from the dissipator, and

kBβ=1T.k_B\beta = \frac{1}{T}.

With Q˙=Tr⁡[HL(ρ)]\dot Q=\operatorname{Tr}[H\mathcal L(\rho)],

Σ˙=dSdt−Q˙T.\dot\Sigma = \frac{dS}{dt} - \frac{\dot Q}{T}.

A system in a steady state absorbs heat current JJ from a hot bath at ThT_h and dumps the same heat current into a cold bath at TcT_c. Compute Σ˙\dot\Sigma.

Solution

At steady state dS/dt=0dS/dt=0. With heat into the system as positive,

Q˙h=J,Q˙c=−J.\dot Q_h=J, \qquad \dot Q_c=-J.

Therefore

Σ˙=−JTh−−JTc=J(1Tc−1Th).\dot\Sigma = - \frac{J}{T_h} - \frac{-J}{T_c} = J \left( \frac{1}{T_c} - \frac{1}{T_h} \right).

For Th>TcT_h>T_c and J≥0J\ge0, this is nonnegative.

For an initially factorized system and thermal bath, explain why entropy production can be written as mutual information plus bath relative entropy.

Solution

The total entropy is conserved by unitary evolution. Starting from a product state, this gives

IS:B(t)=ΔSS+ΔSBkB.I_{S:B}(t) = \frac{\Delta S_S+\Delta S_B}{k_B}.

For the bath,

D(ρB(t)∥ρBβ)=−ΔSBkB+βΔEB.D(\rho_B(t)\Vert\rho_B^\beta) = - \frac{\Delta S_B}{k_B} + \beta\Delta E_B.

With heat into the system Q=−ΔEBQ=-\Delta E_B,

D(ρB(t)∥ρBβ)=−ΔSBkB−βQ.D(\rho_B(t)\Vert\rho_B^\beta) = - \frac{\Delta S_B}{k_B} - \beta Q.

Adding the two equations gives

IS:B(t)+D(ρB(t)∥ρBβ)=ΔSSkB−βQ=ΣkB.I_{S:B}(t) + D(\rho_B(t)\Vert\rho_B^\beta) = \frac{\Delta S_S}{k_B} - \beta Q = \frac{\Sigma}{k_B}.

Both terms on the left are nonnegative, so the finite-process entropy production is nonnegative.

  • H. Spohn, “Entropy production for quantum dynamical semigroups,” Journal of Mathematical Physics 19, 1227-1230 (1978).
  • H. Spohn and J. L. Lebowitz, “Irreversible thermodynamics for quantum systems weakly coupled to thermal reservoirs,” Advances in Chemical Physics 38, 109-142 (1978).
  • R. Alicki, “The quantum open system as a model of the heat engine,” Journal of Physics A: Mathematical and General 12, L103-L107 (1979).
  • H.-P. Breuer, “Quantum jumps and entropy production,” Physical Review A 68, 032105 (2003).
  • H.-P. Breuer and F. Petruccione, The Theory of Open Quantum Systems, Oxford University Press (2002).
  • M. Esposito, U. Harbola, and S. Mukamel, “Nonequilibrium fluctuations, fluctuation theorems, and counting statistics in quantum systems,” Reviews of Modern Physics 81, 1665-1702 (2009).
  • M. Esposito and C. Van den Broeck, “Three detailed fluctuation theorems,” Physical Review Letters 104, 090601 (2010).
  • R. Kosloff, “Quantum thermodynamics: A dynamical viewpoint,” Entropy 15, 2100-2128 (2013).
  • U. Seifert, “Stochastic thermodynamics, fluctuation theorems and molecular machines,” Reports on Progress in Physics 75, 126001 (2012).