The Helmholtz Energy

Squeeze a gas in a rigid, insulated-but-thermostatted cylinder and ask a simple question. How much useful work can it possibly deliver? Internal energy alone cannot answer this, because some of that energy is always tied up disordering the surroundings. The Helmholtz energy is the thermodynamic quantity built exactly to answer it. Chemists rarely run reactions at constant volume, but the Helmholtz energy is still indispensable. It is the natural potential for statistical mechanics, for equations of state, and for any process held at fixed temperature and fixed volume. It also sets up the more famous constant-pressure cousin, the Gibbs energy. This article defines the Helmholtz energy from the second law. It derives why it must decrease at constant TT and VV. It shows why AA equals the maximum work obtainable from a process, and works two full numerical examples.

Key takeaways
  • The Helmholtz energy is defined as A=U−TSA = U - TS, combining energy and entropy into one function.
  • At constant temperature and volume, spontaneous processes have dA≤0dA \le 0; equilibrium is the minimum of AA.
  • AA is a state function because UU, TT, and SS are all state functions.
  • −ΔA-\Delta A equals the maximum total work extractable from a process at constant TT, giving AA its name "free energy."
  • The Helmholtz energy is the natural potential for constant-volume systems; the Gibbs energy plays this role at constant pressure.
  • Key idea: A=U−TSA = U - TS packages the competition between lowering energy and raising entropy into a single quantity that must decrease for any spontaneous change at fixed TT and VV.
The core insight

The Helmholtz energy A=U−TSA = U - TS is the "energy left over" once you subtract the part of UU that entropy production forces you to give away as heat to a constant-temperature surroundings, so at fixed TT and VV spontaneous change always drives AA downward and equilibrium sits at its minimum.

The physical picture

Consider a closed system held at fixed volume, in thermal contact with a huge surroundings at temperature TT. No work of expansion is possible because the volume cannot change, but the internal energy UU can still change as heat flows across the boundary. The second law says entropy is what decides whether a change happens spontaneously, but entropy is a property of the universe — system plus surroundings — not of the system alone. That makes it awkward to use directly for predicting the behavior of a beaker sitting on a bench. The trick is to rewrite the second law entirely in terms of system properties. If the system exchanges heat dqdq with surroundings at temperature TT, the surroundings' entropy changes by −dq/T-dq/T. The Clausius inequality states that for any process,

dSsys−dqT≥0dS_{\text{sys}} - \frac{dq}{T} \ge 0

At constant volume with no non-expansion work, the first law gives dq=dUdq = dU. Substituting and rearranging turns a statement about total entropy into a statement about UU and SS of the system alone: dU−T dS≤0dU - T\,dS \le 0. Define A≡U−TSA \equiv U - TS. At constant TT, dA=dU−T dSdA = dU - T\,dS, so the condition becomes dA≤0dA \le 0. This is the entire logical content of the Helmholtz energy: it is a bookkeeping device that folds the surroundings' entropy change into a single system-only function. Physically, TSTS is the portion of the internal energy that is "entropy-locked" — energy the system must release as heat merely to keep its entropy consistent with contact at temperature TT. Subtracting TSTS from UU leaves the fraction of the energy that is, in principle, convertible to work under isothermal conditions. That is why AA has historically been called the work function (Helmholtz's own term, "Arbeit" — German for "work" — is the source of the symbol AA).

Figure
Energy partition: U splits into "locked" TS and available A at fixed T
Internal energy U at temperature T U (total internal energy) A = U − TS (available as work) TS (entropy-locked) Example: U = 500 J, T = 300 K, S = 1.20 J/K, so TS = 360 J, A = 140 J

Now picture the approach to equilibrium itself. At fixed TT and VV, a system evolves so that AA falls continuously and flattens out at a minimum — the equilibrium state. Any further fluctuation away from that point would raise AA, which the second law forbids, so the system sits there.

Figure
A versus reaction progress at constant T and V
A (Helmholtz energy) extent of reaction, ξ minimum: dA = 0, equilibrium dA less than 0 (spontaneous) dA greater than 0 (forbidden)

The core relations

A=U−TSA = U - TS

where: UU is internal energy, TT is absolute temperature, SS is entropy — all properties of the system.

dA=−S dT−p dVdA = -S\,dT - p\,dV

where: this is the natural differential form for a closed system doing only pVpV work, showing AA is naturally a function of TT and VV.

(∂A∂T)V=−S,(∂A∂V)T=−p\left(\frac{\partial A}{\partial T}\right)_V = -S, \qquad \left(\frac{\partial A}{\partial V}\right)_T = -p

where: these partial derivatives recover entropy and pressure directly from A(T,V)A(T,V).

dA≤0(constant T,V)dA \le 0 \quad (\text{constant } T, V)

where: equality holds at equilibrium; strict inequality signals a spontaneous, irreversible change.

wmax⁡=ΔA(constant T)w_{\max} = \Delta A \quad (\text{constant } T)

where: wmax⁡w_{\max} is the maximum total work (expansion plus any other form) obtainable from a process at constant temperature; the system does work when ΔA\Delta A is negative. ##

Derivation AFrom the Clausius inequality to dA ≤ 0

Goal: show that at constant temperature and volume, spontaneous change requires the Helmholtz energy to decrease, and that equilibrium corresponds to its minimum.

Step 1. Start from the Clausius inequality. For any process in a closed system exchanging heat dqdq with surroundings at temperature TT,

dS≥dqTdS \ge \frac{dq}{T}

where dSdS is the entropy change of the system. Equality holds only for a reversible process.

Step 2. Bring in the first law. For a closed system doing only expansion work,

dU=dq−p dVdU = dq - p\,dV

so dq=dU+p dVdq = dU + p\,dV. Substitute into the Clausius inequality:

dS≥dU+p dVTdS \ge \frac{dU + p\,dV}{T}

Step 3. Rearrange to isolate energy-like terms. Multiply through by TT (positive, so the inequality direction is preserved) and rearrange:

dU+p dV−T dS≤0dU + p\,dV - T\,dS \le 0

Step 4. Specialize to constant volume. If VV is fixed, dV=0dV = 0, and no expansion work occurs, leaving

dU−T dS≤0dU - T\,dS \le 0

Step 5. Introduce A at constant T. Define A≡U−TSA \equiv U - TS. Its differential is dA=dU−T dS−S dTdA = dU - T\,dS - S\,dT. At constant temperature, dT=0dT = 0, so dA=dU−T dSdA = dU - T\,dS. Combining with Step 4,

dA≤0at constant T,VdA \le 0 \quad \text{at constant } T, V

Step 6. Interpret the equality case. Equality corresponds to a reversible change, which for a system already at equilibrium means no further change occurs — AA sits at a stationary point. Since the inequality only ever pushes AA downward, that stationary point must be a minimum, not a maximum or saddle.

dA≤0 at constant T,V; equilibrium is the minimum of A\boxed{dA \le 0 \text{ at constant } T,V \text{; equilibrium is the minimum of } A}

Worked examples

Example 1 — Computing ΔA for an isothermal ideal-gas expansion. One mole of an ideal gas expands isothermally and reversibly at T=298 KT = 298\text{ K} from V1=10.0 LV_1 = 10.0\text{ L} to V2=20.0 LV_2 = 20.0\text{ L}. Find ΔU\Delta U, ΔS\Delta S, ΔA\Delta A, and the work done. For an ideal gas, UU depends only on TT. Since TT is constant,

ΔU=0\Delta U = 0

The reversible isothermal entropy change of an ideal gas is

ΔS=nRln⁡V2V1\Delta S = nR\ln\frac{V_2}{V_1}

With n=1 moln = 1\text{ mol}, R=8.314 J K−1mol−1R = 8.314\text{ J K}^{-1}\text{mol}^{-1}, and V2/V1=2.00V_2/V_1 = 2.00:

ΔS=(1)(8.314)ln⁡(2.00)=8.314×0.6931=5.763 J K−1\Delta S = (1)(8.314)\ln(2.00) = 8.314 \times 0.6931 = 5.763\text{ J K}^{-1}

Now

ΔA=ΔU−TΔS=0−(298)(5.763 J K−1)\Delta A = \Delta U - T\Delta S = 0 - (298)(5.763\text{ J K}^{-1})
ΔA=−1717 J=−1.72 kJ\Delta A = -1717\text{ J} = -1.72\text{ kJ}

Check via work: reversible isothermal work for an ideal gas is

w=−nRTln⁡V2V1=−(1)(8.314)(298)ln⁡(2.00)w = -nRT\ln\frac{V_2}{V_1} = -(1)(8.314)(298)\ln(2.00)
w=−2478×0.6931=−1717 Jw = -2478 \times 0.6931 = -1717\text{ J}

The magnitudes match exactly, since for an ideal gas at constant TT, ΔA=wrev\Delta A = w_{\text{rev}} (heat q=TΔS=+1717 Jq = T\Delta S = +1717\text{ J} flows in, and ΔU=q+w=1717−1717=0\Delta U = q + w = 1717 - 1717 = 0, consistent). The negative sign means the gas does 1.72 kJ of work on the surroundings — exactly the maximum work available, confirming wmax⁡=ΔAw_{\max} = \Delta A.

Example 2 — Spontaneity and A for a phase transition away from the normal transition temperature. Supercooled liquid water sits at −5.0 ∘C-5.0\,^\circ\text{C} (T=268.15 KT = 268.15\text{ K}) at constant volume and constant temperature (imagine a rigid, thermostatted vessel). Freezing releases ΔHfus=−6.01 kJ mol−1\Delta H_{\text{fus}} = -6.01\text{ kJ mol}^{-1} at the normal melting point Tm=273.15 KT_m = 273.15\text{ K}, with ΔSfus=ΔHfus/Tm=−22.0 J K−1mol−1\Delta S_{\text{fus}} = \Delta H_{\text{fus}}/T_m = -22.0\text{ J K}^{-1}\text{mol}^{-1} for freezing. Treating ΔH\Delta H and ΔS\Delta S as roughly temperature-independent over this small range, determine whether freezing is spontaneous at −5.0 ∘C-5.0\,^\circ\text{C} under constant T,VT,V conditions, using ΔA\Delta A. At constant volume the appropriate work-content criterion is ΔA\Delta A, and since pVpV changes are negligible for a nearly incompressible liquid/solid pair, ΔA≈ΔU−TΔS≈ΔH−TΔS\Delta A \approx \Delta U - T\Delta S \approx \Delta H - T\Delta S (ignoring the small Δ(pV)\Delta(pV) term, valid to a few J for condensed phases).

ΔAfreeze≈ΔHfus−TΔSfus\Delta A_{\text{freeze}} \approx \Delta H_{\text{fus}} - T\Delta S_{\text{fus}}
ΔAfreeze≈(−6010 J mol−1)−(268.15 K)(−22.0 J K−1mol−1)\Delta A_{\text{freeze}} \approx (-6010\text{ J mol}^{-1}) - (268.15\text{ K})(-22.0\text{ J K}^{-1}\text{mol}^{-1})
ΔAfreeze≈−6010+5899=−111 J mol−1\Delta A_{\text{freeze}} \approx -6010 + 5899 = -111\text{ J mol}^{-1}

Since ΔA<0\Delta A < 0, freezing is spontaneous at −5.0 ∘C-5.0\,^\circ\text{C} under these constant T,VT,V conditions — consistent with everyday experience that supercooled water freezes readily once nucleated. As a sanity check, at exactly Tm=273.15 KT_m = 273.15\text{ K},

ΔAfreeze=−6010−(273.15)(−22.0)=−6010+6009=−1 J mol−1≈0\Delta A_{\text{freeze}} = -6010 - (273.15)(-22.0) = -6010 + 6009 = -1\text{ J mol}^{-1} \approx 0

confirming equilibrium (melting point) is correctly recovered as the point where ΔA→0\Delta A \to 0, and that a few degrees of supercooling is enough to make freezing clearly favorable.

Limiting cases & common traps

SituationWhat to remember
Constant TT and VV, no non-expansion workdA≤0dA \le 0 is the correct spontaneity criterion; do not use ΔG\Delta G here.
Constant TT and ppUse the Gibbs energy G=A+pVG = A + pV instead; ΔA\Delta A still exists but is not the natural minimized quantity.
Ideal gas, isothermal processΔU=0\Delta U = 0, so ΔA=−TΔS\Delta A = -T\Delta S exactly; useful cross-check as in Example 1.
Reversible processdA=0dA = 0 throughout only if also at constant T,VT,V; otherwise dA=−SdT−pdVdA = -SdT - pdV can be nonzero even reversibly.
Non-expansion work present (electrical, etc.)wmax⁡w_{\max} total (all forms) equals ΔA\Delta A at constant TT, not just pVpV work.

The chemist behind it

Hermann von Helmholtz was a physician-turned-physicist whose 1847 memoir on the conservation of energy helped crystallize the first law of thermodynamics into rigorous mathematical form. Decades later, in the 1880s, he introduced the free energy function that bears his name, showing how to separate the "free" (work-available) part of a system's energy from the part inevitably dissipated as heat at a given temperature. His broader scientific range — from nerve conduction speed to acoustics to the physiology of vision — reflects a 19th-century conviction that energy conservation was a truly universal principle, applicable equally to muscles, batteries, and chemical reactions.

Origins · 1 minHermann von Helmholtz and how this was discovered
HV
Hermann von Helmholtz
1821–1894 · German physicist and physician who defined the work function A = U − TS while unifying energy conservation across physics, physiology, and chemistry

Ask the tutor: How does the Helmholtz energy connect to the Gibbs energy when a reaction produces or consumes gas, and which one should you actually use in the lab?

Why is A called a "free energy" if it usually decreases?

"Free" refers to energy that is free to be converted into work, not energy that is free of charge or increasing. The Helmholtz energy A=U−TSA = U - TS represents the part of the internal energy not tied up satisfying the entropy requirements of contact with a heat bath at temperature TT. That leftover portion is, in principle, available to do work. As a process proceeds spontaneously at constant TT and VV, AA decreases because usable work capacity is being spent, released as heat, or converted into products, until equilibrium is reached at the minimum.

How is the Helmholtz energy related to the Gibbs energy?

The Gibbs energy is defined as G=A+pV=U+pV−TS=H−TSG = A + pV = U + pV - TS = H - TS. Where AA is the natural potential for constant temperature and volume, GG plays the same role at constant temperature and pressure — the condition relevant to most laboratory chemistry done in open vessels. The two coincide numerically whenever Δ(pV)=0\Delta(pV) = 0, for instance in many condensed-phase processes with no change in moles of gas, but they differ whenever gas volume changes significantly during a process.

Does dA ≤ 0 mean A always decreases in every real process?

No — it applies specifically to processes at constant temperature and constant volume with no additional non-expansion work. Outside those conditions, AA can rise or fall; the general differential is dA=−S dT−p dVdA = -S\,dT - p\,dV, which is nonzero whenever TT or VV changes, regardless of spontaneity. The inequality dA≤0dA \le 0 is a conditional statement, valid only under the stated constraints, just as dG≤0dG \le 0 requires constant TT and pp.

Why does A equal the maximum work obtainable from a process?

From the derivation, dU−T dS≤−pextdVdU - T\,dS \le -p_{\text{ext}}dV rearranges (at constant TT) to show that the total work done by the system, −w-w, can be at most −ΔA-\Delta A. Equality is achieved only in the reversible limit, since irreversible processes waste some capacity as unrecoverable entropy production. This is why Helmholtz originally called AA the Arbeitsfunktion, or "work function" — it is a hard upper bound on extractable work at fixed temperature, reversible operation being the only way to reach it.

How does this connect to entropy and the second law I already know?

The Helmholtz energy is not a new physical law — it is a repackaging of the Clausius inequality, dSuniverse≥0dS_{\text{universe}} \ge 0, into a statement using only system properties. By defining A=U−TSA = U - TS, the surroundings' entropy change is folded into the system's own energy bookkeeping, so you never need to track the bath's entropy explicitly. This is exactly the same logical move used later to construct the Gibbs energy for constant-pressure systems.