Table of thermodynamic equations


Common thermodynamic equations and quantities in thermodynamics, using mathematical notation, are as follows:

Definitions

Many of the definitions below are also used in the thermodynamics of chemical reactions.

General basic quantities

Quantity symbol/sSI unitDimension
Number of moleculesN11
Amount of substancenmolN
TemperatureTKΘ
Heat EnergyQ, qJML2T−2
Latent heatQLJML2T−2

General derived quantities

Quantity symbol/sDefining equationSI unitDimension
Thermodynamic beta, inverse temperatureβJ−1T2M−1L−2
Thermodynamic temperatureτJML2T−2
EntropyS
,
J⋅K−1ML2T−2Θ−1
PressurePPaML−1T−2
Internal EnergyUJML2T−2
EnthalpyHJML2T−2
Partition FunctionZ11
Gibbs free energyGJML2T−2
Chemical potential μi
, where is not proportional to because depends on pressure.
, where is proportional to because depends only on temperature and pressure and composition.
JML2T−2
Helmholtz free energyA, FJML2T−2
Landau potential, Landau free energy, Grand potentialΩ, ΦGJML2T−2
Massieu potential, Helmholtz free entropyΦJ⋅K−1ML2T−2Θ−1
Planck potential, Gibbs free entropyΞJ⋅K−1ML2T−2Θ−1

Thermal properties of matter

Quantity symbol/sDefining equationSI unitDimension
General heat/thermal capacityCJ⋅K−1ML2T−2Θ−1
Heat capacity CpJ⋅K−1ML2T−2Θ−1
Specific heat capacity CmpJ⋅kg−1⋅K−1L2T−2Θ−1
Molar specific heat capacity CnpJ⋅K−1⋅mol−1ML2T−2Θ−1N−1
Heat capacity CVJ⋅K−1ML2T−2Θ−1
Specific heat capacity CmVJ⋅kg−1⋅K−1L2T−2Θ−1
Molar specific heat capacity CnVJ⋅K⋅−1 mol−1ML2T−2Θ−1N−1
Specific latent heatLJ⋅kg−1L2T−2
Ratio of isobaric to isochoric heat capacity, heat capacity ratio, adiabatic index, Laplace coefficientγ11

Thermal transfer

Quantity symbol/sDefining equationSI unitDimension
Temperature gradientNo standard symbolK⋅m−1ΘL−1
Thermal conduction rate, thermal current, thermal/heat flux, thermal power transferPWML2T−3
Thermal intensityIW⋅m−2MT−3
Thermal/heat flux density qW⋅m−2MT−3

Equations

The equations in this article are classified by subject.

Thermodynamic processes

Physical situationEquations
Isentropic process
For an ideal gas




Isothermal process
For an ideal gas
Isobaric processp1 = p2, p = constant
Isochoric processV1 = V2, V = constant
Free expansion
Work done by an expanding gasProcess

Net work done in cyclic processes

Kinetic theory

Physical situationNomenclatureEquations
Ideal gas lawp = pressureV = volume of containerT = temperature n = amount of substanceR = gas constantN = number of moleculesk = Boltzmann constant

Pressure of an ideal gasm = mass of one moleculeMm = molar mass

Ideal gas

QuantityGeneral EquationIsobaric
Δp = 0
Isochoric
ΔV = 0
Isothermal
ΔT = 0
Adiabatic
Work
W
Heat Capacity
C


Internal Energy
ΔU
Enthalpy
ΔH
Entropy
Δs
Constant

Entropy

Statistical physics

Below are useful results from the Maxwell–Boltzmann distribution for an ideal gas, and the implications of the Entropy quantity. The distribution is valid for atoms or molecules constituting ideal gases.
Physical situationNomenclatureEquations
Maxwell–Boltzmann distributionv = velocity of atom/molecule,m = mass of each molecule,γ = Lorentz factor as function of momentum
  • Ratio of thermal to rest mass-energy of each molecule:
K2 is the modified Bessel function of the second kind.
Non-relativistic speeds

Relativistic speeds
Entropy Logarithm of the density of statesPi = probability of system in microstate i
  • Ω = total number of microstates

where:
Entropy change
Entropic force
Equipartition theoremdf = degree of freedomAverage kinetic energy per degree of freedom
Internal energy

Corollaries of the non-relativistic Maxwell–Boltzmann distribution are below.
Physical situationNomenclatureEquations
Mean speed
Root mean square speed
Modal speed
Mean free pathσ = effective cross-sectionn = volume density of number of target particles = mean free path

Quasi-static and reversible processes

For quasi-static and reversible processes, the first law of thermodynamics is:
where δQ is the heat supplied to the system and δW is the work done by the system.

Thermodynamic potentials

The following energies are called the thermodynamic potentials,
and the corresponding fundamental thermodynamic relations or "master equations" are:
PotentialDifferential
Internal energy
Enthalpy
Helmholtz free energy
Gibbs free energy

Maxwell's relations

The four most common Maxwell's relations are:
Physical situationNomenclatureEquations
Thermodynamic potentials as functions of their natural variables

More relations include the following.
Other differential equations are:
NameHUG
Gibbs–Helmholtz equation

Quantum properties

where N is number of particles, h is that Planck constant, I is moment of inertia, and Z is the partition function, in various forms:
Degree of freedomPartition function
Translation
Vibration
Rotation
  • where:σ = 1 σ = 2

Thermal properties of matter

CoefficientsEquation
Joule-Thomson coefficient
Compressibility
Coefficient of thermal expansion
Heat capacity
Heat capacity

Derivation of heat capacity

Since
Derivation of heat capacity

Since
,

Thermal transfer

Physical situationNomenclatureEquations
Net intensity emission/absorptionTexternal = external temperature Tsystem = internal temperature ε = emissivity
Internal energy of a substanceCV = isovolumetric heat capacity of substance
  • ΔT = temperature change of substance
Meyer's equationCp = isobaric heat capacityCV = isovolumetric heat capacityn = amount of substance
Effective thermal conductivitiesλi = thermal conductivity of substance iλnet = equivalent thermal conductivity
Series
Parallel

Thermal efficiencies

Physical situationNomenclatureEquations
Thermodynamic enginesη = efficiencyW = work done by engineQH = heat energy in higher temperature reservoirQL = heat energy in lower temperature reservoirTH = temperature of higher temp. reservoirTL = temperature of lower temp. reservoir
Thermodynamic engine:

Carnot engine efficiency:
RefrigerationK = coefficient of refrigeration performanceRefrigeration performance
Carnot refrigeration performance