Math 2.0

Classical thermodynamics, heat transfer Definition

Enthalpy

Builds on Internal energyState function

Definition

Let a thermodynamic system in equilibrium have internal energy UU, pressure pp and volume VV. Its enthalpy is the state function H=U+pV.H = U + pV.

Remarks

From dU=T dS−p dVdU = T \, dS - p \, dV one gets dH=T dS+V dpdH = T \, dS + V \, dp, where TT is the temperature and SS the entropy. So the natural variables of HH are SS and pp, and T=(∂H/∂S)pT = (\partial H / \partial S)_p, V=(∂H/∂p)SV = (\partial H / \partial p)_S. In a process at constant pressure in which only expansion work is done, the heat taken in is Q=ΔHQ = \Delta H. Example: for nn moles of a monatomic ideal gas, U=32nRTU = \frac{3}{2} nRT and pV=nRTpV = nRT, so H=52nRTH = \frac{5}{2} nRT, where RR is the gas constant. Non-example: U−pVU - pV is not the enthalpy; the sign of the term pVpV matters, and U−pVU - pV has differential T dS−2p dV−V dpT \, dS - 2p \, dV - V \, dp, with no simple meaning.

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  1. Internal energy concept
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Further reading

  1. Web https://en.wikipedia.org/wiki/Enthalpy
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Kinddefinition
WritingW0 stub
MSC80A10, 80A05
DefinesEnthalpy
UsesInternal energy, State function
Changed3 November 2026

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