Ideal gas law

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File:Ideal gas isotherms.png
Isotherms of an ideal gas

The ideal gas law is the equation of state of a hypothetical ideal gas, first stated by Benoît Paul Émile Clapeyron in 1834.

The state of an amount of gas is determined by its pressure, volume, and temperature according to the equation:
<math>\ PV = nRT </math>


<math>\ P </math> is the absolute pressure of the gas,
<math>\ V </math> is the volume of the gas,
<math>\ n </math> is the number of moles of gas,
<math>\ R </math> is the universal gas constant,
<math>\ T </math> is the absolute temperature.

The value of the ideal gas constant, R, is found to be as follows.

R  8.314472 J·mol−1·K−1
8.314472 m3·Pa·K−1·mol−1
8.314472 kPa·L·mol-1·K-1
0.08205746  L·atm·K−1·mol−1
62.36367 mmHg·K−1·mol−1
10.73159 ft3·psi·°R−1·lb-mol−1
53.34 ft·lbf·°R−1·lbm−1 (for air)

The ideal gas law mathematically follows from a statistical mechanical treatment of primitive identical particles (point particles without internal structure) which do not interact, but exchange momentum (and hence kinetic energy) in elastic collisions.

Since it neglects both molecular size and intermolecular attractions, the ideal gas law is most accurate for monoatomic gases at high temperatures and low pressures. The neglect of molecular size becomes less important for larger volumes, i.e., for lower pressures. The relative importance of intermolecular attractions diminishes with increasing thermal kinetic energy i.e., with increasing temperatures. More sophisticated equations of state, such as the van der Waals equation, allow deviations from ideality caused by molecular size and intermolecular forces to be taken into account.

Alternative forms

As the amount of substance could be given in mass instead of moles, sometimes an alternative form of the ideal gas law is useful. The number of moles (<math>n\, </math>) is equal to the mass (<math>\, m </math>) divided by the molar mass (<math>\, M </math>):

<math> n = {\frac{m}{M}} </math>

Then, replacing <math>\, n </math> gives:

<math>\ PV = \frac{m}{M}RT </math>

from where

<math>\ P = \rho \frac{R}{M}T </math>.

This form of the ideal gas law is particularly useful because it links pressure, density <math> \rho = m/V</math>, and temperature in a unique formula independent from the quantity of the considered gas.

In statistical mechanics the following molecular equation is derived from first principles:

<math>\ PV = NkT .</math>

Here <math>\,k</math> is Boltzmann's constant, and <math>\,N</math> is the actual number of molecules, in contrast to the other formulation, which uses <math>\,n</math>, the number of moles. This relation implies that <math>N\,k = nR</math>, and the consistency of this result with experiment is a good check on the principles of statistical mechanics.

From here we can notice that for an average particle mass of <math> \mu </math> times the atomic mass constant <math>m_\mathrm{u}</math> (i.e., the mass is <math>\mu</math> u)

<math> N = \frac{m}{\mu m_\mathrm{u}} </math>

and since <math> \rho = m/V </math>, we find that the ideal gas law can be re-written as:

<math> p = \frac{1}{V}\frac{m}{\mu m_\mathrm{u}} kT = \frac{k}{\mu m_\mathrm{u}} \rho T .</math>

One more equation involves density where:

<math>\ PM = DRT .</math>

where M is the mass and D is the density.


Process Constant Known ratio P2 V2 T2
Isobaric process
P2 = P1 V2 = V1 (V2/V1) T2 = T1 (V2/V1)
P2 = P1 V2 = V1 (T2/T1) T2 = T1 (T2/T1)
Isochoric process
P2 = P1 (P2/P1) V2 = V1 T2 = T1 (P2/P1)
P2 = P1 (T2/T1) V2 = V1 T2 = T1 (T2/T1)
Isothermal process
P2 = P1 (P2/P1) V2 = V1 / (P2/P1) T2 = T1
P2 = P1 / (V2/V1) V2 = V1 (V2/V1) T2 = T1
Isentropic process
(Reversible adiabatic process)
EntropyTemplate:Ref label
P2 = P1 (P2/P1) V2 = V1 (P2/P1) -1/<math>\gamma</math> T2 = T1 (P2/P1)(<math>\gamma</math>-1)/<math>\gamma</math>
P2 = P1 (V2/V1) -<math>\gamma</math> V2 = V1 (V2/V1) T2 = T1 (V2/V1) 1-<math>\gamma</math>
P2 = P1 (T2/T1) <math>\gamma</math>/(<math>\gamma</math>-1) V2 = V1 (T2/T1) 1/(1-<math>\gamma</math>) T2 = T1 (T2/T1)

Template:Note label a. In an isentropic process, system entropy (Q) is constant. Under these conditions, P1 V1<math>\gamma</math> = P2 V2<math>\gamma</math>, where <math>\gamma</math> is defined as the heat capacity ratio, which is constant for an ideal gas.



The ideal gas law can be derived from combining two empirical gas laws: the combined gas law and Avogadro's law. The combined gas law states that

<math>\frac {pV}{T}= C </math>

where C is a constant which is directly proportional to the amount of gas, n (Avogadro's law). The proportionality factor is the universal gas constant, R, i.e. <math>C=nR</math>.

Hence the ideal gas law

<math> pV = nRT \,</math>


The ideal gas law can also be derived from first principles using the kinetic theory of gases, in which several simplifying assumptions are made, chief among which are that the molecules, or atoms, of the gas are point masses, possessing mass but no significant volume, and undergo only elastic collisions with each other and the sides of the container in which both linear momentum and kinetic energy are conserved.

Derivation from the statistical mechanics

Let q = (qx, qy, qz) and p = (px, py, pz) denote the position vector and momentum vector of a particle of an ideal gas,respectively, and let F denote the net force on that particle, then


\begin{align} \langle \mathbf{q} \cdot \mathbf{F} \rangle &= \Bigl\langle q_{x} \frac{dp_{x}}{dt} \Bigr\rangle + \Bigl\langle q_{y} \frac{dp_{y}}{dt} \Bigr\rangle + \Bigl\langle q_{z} \frac{dp_{z}}{dt} \Bigr\rangle\\ &=-\Bigl\langle q_{x} \frac{\partial H}{\partial q_x} \Bigr\rangle - \Bigl\langle q_{y} \frac{\partial H}{\partial q_y} \Bigr\rangle - \Bigl\langle q_{z} \frac{\partial H}{\partial q_z} \Bigr\rangle = -3k_{B} T, \end{align} </math> where the first equality is Newton's second law, and the second line uses Hamilton's equations and the equipartition theorem. Summing over a system of N particles yields


3Nk_{B} T = - \biggl\langle \sum_{k=1}^{N} \mathbf{q}_{k} \cdot \mathbf{F}_{k} \biggr\rangle. </math>

By Newton's third law and the ideal gas assumption, the net force on the system is the force applied by the walls of their container, and this force is given by the pressure P of the gas. Hence


-\biggl\langle\sum_{k=1}^{N} \mathbf{q}_{k} \cdot \mathbf{F}_{k}\biggr\rangle = P \oint_{\mathrm{surface}} \mathbf{q} \cdot \mathbf{dS}, </math>

where dS is the infinitesimal area element along the walls of the container. Since the divergence of the position vector q is


\boldsymbol\nabla \cdot \mathbf{q} = \frac{\partial q_{x}}{\partial q_{x}} + \frac{\partial q_{y}}{\partial q_{y}} + \frac{\partial q_{z}}{\partial q_{z}} = 3, </math>

the divergence theorem implies that


P \oint_{\mathrm{surface}} \mathbf{q} \cdot \mathbf{dS} = P \int_{\mathrm{volume}} \left( \boldsymbol\nabla \cdot \mathbf{q} \right) dV = 3PV, </math>

where dV is an infinitesimal volume within the container and V is the total volume of the container.

Putting these equalities together yields


3Nk_{B} T = -\biggl\langle \sum_{k=1}^{N} \mathbf{q}_{k} \cdot \mathbf{F}_{k} \biggr\rangle = 3PV, </math>

which immediately implies the ideal gas law for N particles:


PV = Nk_{B} T = nRT,\, </math>

where n=N/NA is the number of moles of gas and R=NAkB is the gas constant.

The readers are referred to the comprehensive article Configuration integral (statistical mechanics) where an alternative statistical mechanics derivation of the ideal-gas law, using the relationship between the Helmholtz free energy and the partition function, but without using the equipartition theorem, is provided.

See also


bs:Boyle-Mariotteov zakon da:Idealgasligning de:Thermische Zustandsgleichung idealer Gase el:Καταστατική εξίσωση των αερίων eo:Ekvacio de Clapeyron hi:आदर्श गैस समीकरण ko:이상 기체 상태방정식 it:Equazione di stato dei gas perfetti mr:आदर्श वायू समीकरण nl:Algemene gaswet sl:Splošna plinska enačba sv:Ideala gaslagen uk:Рівняння стану ідеального газу Template:WH Template:WS