Isothermal Processes

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isothermal constant-temperature Boyles-law work heat

Core Idea

An isothermal process occurs at constant temperature. For an ideal gas, ΔU = 0 in any isothermal process (since U depends only on T), so by the first law, Q = W. The work done by the gas in expanding isothermally from V₁ to V₂ is W = nRT ln(V₂/V₁). On a PV diagram, an isotherm follows the hyperbola PV = constant. Isothermal processes require slow, quasi-static changes with continuous heat exchange to maintain constant temperature.

How It's Best Learned

Derive the isothermal work integral from W = ∫P dV with P = nRT/V. Evaluate for specific numbers (e.g., 1 mol of gas at 300 K doubling its volume). Compare to the work that would be done in a free expansion — which is zero and is not quasi-static.

Common Misconceptions

Explainer

You already know that thermodynamic processes are constrained by which state variables are held fixed. An isothermal process holds temperature T constant throughout. For an ideal gas, this single constraint has a powerful consequence via the ideal gas law: if T is fixed, then PV = nRT = constant, so pressure and volume move in inverse proportion along a hyperbola on the PV diagram. As you expand the gas, pressure drops; as you compress, pressure rises — always staying on the same isotherm.

The first law, ΔU = Q − W, becomes especially transparent here. For an ideal gas, internal energy U depends only on temperature (from the equipartition theorem you know from prerequisites). Since T is constant, ΔU = 0 for any isothermal process on an ideal gas. The first law then requires Q = W: every joule of work done by the expanding gas must be supplied as heat from the reservoir, and every joule of work done on a compressed gas must be expelled as heat. Temperature stays flat because the reservoir absorbs or supplies heat as needed — which is exactly why isothermal processes require continuous thermal contact with a reservoir.

The work integral W = ∫ P dV with P = nRT/V gives W = nRT ∫(V₁ to V₂) dV/V = nRT ln(V₂/V₁). Notice the logarithm: the work is not simply P·ΔV (which would be appropriate for a constant-pressure process) but depends on the ratio of volumes. Doubling the volume at 300 K for 1 mole of gas gives W = (8.314)(300) ln(2) ≈ 1729 J. This is less work than a constant-pressure expansion over the same volume range, because pressure drops continuously during the isothermal expansion.

The isothermal process appears in the Carnot cycle (your next topic) as the reversible heat exchange steps. Its reversibility is precisely why it requires infinite slowness: a truly quasi-static isothermal expansion allows the system to remain in equilibrium at every point, with no temperature gradients, no viscous dissipation, and no irreversibilities. Real industrial processes approach isothermal behavior when the working fluid is in good thermal contact with a large heat reservoir and changes are slow relative to thermal equilibration timescales — a useful approximation for slow compression of gases in heat exchangers.

Practice Questions 5 questions

Prerequisite Chain

Counting to 10Counting to 20Understanding ZeroThe Number ZeroCounting to FiveOne-to-One CorrespondenceCombining Small Groups Within 5Addition Within 10Addition Within 20Two-Digit Addition Without RegroupingTwo-Digit Addition with RegroupingAddition Within 100Repeated Addition as MultiplicationMultiplication Facts Within 100Division as Equal SharingDivision as Grouping (Measurement Division)Division: Grouping (Repeated Subtraction) ModelDivision: Fair Sharing ModelDivision as Equal SharingDivision as GroupingBasic Division FactsDivision Facts Within 100Two-Digit by One-Digit DivisionDivision with RemaindersRemainders and Quotients in DivisionDivision Word ProblemsIntroduction to Long DivisionFactors and MultiplesPrime and Composite NumbersEquivalent FractionsRelating Fractions and DecimalsDecimal Place ValueReading and Writing DecimalsComparing and Ordering DecimalsAdding and Subtracting DecimalsMultiplying DecimalsDividing DecimalsDividing FractionsMixed Number ArithmeticOrder of OperationsInteger Order of OperationsVariable ExpressionsCombining Like TermsOne-Step EquationsTwo-Step EquationsSolving Multi-Step EquationsEquations with Variables on Both SidesAngle Pairs: Complementary, Supplementary, and VerticalParallel Lines and TransversalsCorresponding AnglesAlternate Interior AnglesTriangle Angle Sum TheoremExterior Angle TheoremTriangle Inequality TheoremSimilar Triangles: AA SimilaritySimilar Triangles: SSS and SAS SimilarityProportions in Similar TrianglesRight Triangle Trigonometry IntroductionTrigonometric Ratios ReviewRadian MeasureConverting Between Degrees and RadiansThe Unit CircleGraphing Sine and CosineGraphing Tangent and Reciprocal Trigonometric FunctionsDerivatives of Trigonometric FunctionsAntiderivativesIterated Integrals and Fubini's TheoremDouble Integrals in Cartesian CoordinatesDouble Integrals over Rectangular RegionsDouble Integrals in Polar CoordinatesDouble Integrals: Definition and SetupIterated Integrals and Fubini's TheoremDouble Integrals over Rectangular RegionsDouble Integrals over General RegionsApplications of Double Integrals: Area, Mass, and MomentsCenter of MassConservation of Linear MomentumElastic CollisionsInelastic CollisionsCoefficient of RestitutionCollision Analysis and Real-World ApplicationsTwo-Body Collisions in the Center-of-Mass FrameReduced Mass and Two-Body ProblemsKinematics in Two DimensionsProjectile MotionCircular Motion: KinematicsRotational KinematicsTorqueMoment of InertiaRotational Kinetic EnergyThe Work-Energy TheoremConservation of Mechanical EnergyFirst Law of ThermodynamicsThermodynamic Processes and the PV DiagramIsothermal Processes

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