2.4.4 · D2Thermodynamics & Statistical Mechanics (Advanced)

Visual walkthrough — Gibbs-Helmholtz equation

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Everything on this page is a slow-motion replay of the result on the parent Gibbs–Helmholtz note.


Step 0 — The three characters, drawn

Before any algebra, meet the players. Each is just a number attached to a system at some temperature.

Figure — Gibbs-Helmholtz equation

Look at the stacked bar. The blue bar is the full enthalpy . The orange slice, , is the "temperature tax" — entropy multiplied by temperature . Whatever is left, the green bar, is the Gibbs energy . That picture is the equation:

  • — what's left over to actually "spend."
  • — the total pile.
  • — temperature; taller when hotter, so the orange tax grows with heat.
  • — entropy; how big the tax is per degree.

Why start here? Because everything below is just this one equation, viewed from clever angles.


Step 1 — How does the budget change when we warm it up?

WHAT. We nudge the temperature by a tiny amount and watch respond, holding pressure fixed.

WHY. We want to catch , but is hidden inside . To dig it out we need to know how moves with . The rate of that movement is written — read aloud: "how fast changes as changes, keeping pressure constant."

PICTURE.

Figure — Gibbs-Helmholtz equation

The blue curve is plotted against temperature . The red tangent line is its slope. A remarkable fact of thermodynamics is that this slope equals minus the entropy:

  • Left side — the slope of the blue curve.
  • — negative because : increasing makes the orange tax bigger, so slides downward. More entropy ⇒ steeper downhill slope.

Where did this come from? From the differential (derived on the parent note and part of the Maxwell relations family). At constant the term dies, leaving slope .


Step 2 — Trap using that slope

WHAT. Substitute the slope-fact into the definition to isolate .

WHY. In the unknowns are and . Step 1 gave us , purely in terms of . Swap it in and is gone — only remains unknown.

Rearranging for :

H \;=\; G \;-\; T\left(\frac{\partial G}{\partial T}\right)_P \tag{$\star$}

PICTURE.

Figure — Gibbs-Helmholtz equation

Read the figure geometrically. At temperature :

  • the green dot is ;
  • the red tangent has slope ;
  • extend that tangent back to . Its intercept on the vertical axis is exactly (the orange dot).

That is what says: is the "back-project the tangent to " recipe. It works, but it needs both the value and the slope. The next step makes it prettier.

  • — the intercept of the tangent.
  • — the height of the curve at .
  • — how far the tangent climbs back as we walk from down to .

Step 3 — The magic division: differentiate , not

WHAT. Instead of studying , we study the ratio and take its slope.

WHY. Formula is clumsy. But notice the shape . That exact combination is what pops out of the quotient rule applied to . Nature is hinting: divide first.

Apply the quotient rule with , (so ):

  • Numerator — this is just , which is by .
  • Denominator — comes from the quotient rule's .

PICTURE.

Figure — Gibbs-Helmholtz equation

The left panel plots (its tangent hides both and ). The right panel plots — and the annotation shows the entropy term collapsing to a constant that the derivative erases. Watch the orange "" tag get crossed out.


Step 4 — The result appears

WHAT. Combine the last two lines.

WHY. We just showed the numerator equals . Divide by :

  • The slope of versus — measurable.
  • — the enthalpy, cleanly, no entropy in sight.

The minus sign is honest: as rises, shrinks, and (for positive ) climbs. No entropy anywhere. Mission accomplished.


Step 5 — The friendlier form: plot against

WHAT. Change the horizontal axis from to , so we read off a straight-line slope.

WHY. That awkward disappears under a change of variable. Let . A tiny calculus fact: (because ). Substituting kills the and flips the minus:

PICTURE.

Figure — Gibbs-Helmholtz equation

Now plotted against is (for constant ) a straight line whose slope is simply — the green triangle's rise-over-run. This is exactly the plot chemists use, and feeding into it produces the van 't Hoff equation.

  • Horizontal axis — "inverse temperature," small when hot.
  • Slope of the line — the enthalpy (or for a reaction).
  • No minus sign — the reason we prefer this form.

Step 6 — Edge cases: don't get burned

Every scenario, so the reader never hits a surprise.


The one-picture summary

Figure — Gibbs-Helmholtz equation

One frame compressing all six steps: start from the stacked bar (left), divide by to shed the entropy (middle), and read as the slope of versus (right). Follow the arrows and you have re-derived Gibbs–Helmholtz from nothing.

Recall Feynman: tell the whole walkthrough to a 12-year-old

Your spendable pocket money is your total savings minus a "heat tax" that gets bigger when the day is hotter — the tax is temperature times messiness . If you just watch your pocket money change as it warms up, you're mostly watching the tax wobble, so you can't see your real savings. Clever move: look at money-per-degree, . Dividing by the temperature cancels the temperature inside the tax, so the tax turns into a flat number that stops changing. Now when you watch how shifts as the day changes, the tax sits still and only your real savings show through. Plot against "one-over-temperature" and the steepness of that straight line hands you on a plate. That steepness-reading is the Gibbs–Helmholtz equation.

Recall Quick self-check
  • Why does slope downward with ? ::: because slope , and entropy is positive.
  • Which combination made the quotient rule useful? ::: .
  • What is the slope of vs ? ::: the enthalpy .
  • What happens at ? ::: the relation diverges; use the Third Law instead.

Connections

  • Gibbs free energy — the budget we start from.
  • Enthalpy — the prize the trick extracts.
  • Entropy — the term that cancels under .
  • Maxwell relations — source of the slope fact.
  • van 't Hoff equation — the plot applied to .
  • Kirchhoff's law (thermochemistry) — fixes drifting .
  • Helmholtz free energy — the constant-volume twin.