equation

ideal gas law

The ideal gas law relates the pressure, volume, temperature, and number of moles of an ideal gas through the equation PV = nRT.
6 related articles · 6 formulas

Description

In 1834, Émile Clapeyron combined the experimental laws of Boyle, Charles, and Gay-Lussac into the single equation pV = nRT. This elegant formula describes the equilibrium state of an ideal gas — a model where molecules are considered point-like and non-interacting. It works as a 'switch' between the volume, pressure, and temperature of a gas, allowing prediction of the behavior of real gases under ordinary conditions.

History

The experiments of Robert Boyle (1662) and Edme Mariotte showed the inverse proportionality of pressure and volume (pV=const at constant T). Jacques Charles (1787) and Joseph Gay-Lussac (1802) established the dependence of volume on temperature. Amedeo Avogadro in 1811 hypothesized that equal volumes of gases contain equal numbers of molecules under the same conditions. Émile Clapeyron in 1834 combined these laws into a single equation, later generalized by Dmitri Mendeleev with the inclusion of the universal gas constant.

How it works

Widely applied from internal combustion engine calculations to atmospheric modeling. Limits of applicability: the equation is not applicable at high densities and low temperatures, when intermolecular interactions and the finite size of molecules become significant — there, Van der Waals equations with corrections are used.

In practice

From inflating tires to weather forecasting: the relationship between pressure, volume, and temperature governs engines, balloons, and breathing.

Fun fact

If you leave a ball in the sun, it inflates itself — not magic, but the temperature increase raises the pressure with almost constant volume.

Concept graph →

Formulas

$$t = \frac{1}{\lambda} \ln \left( \frac{N_0}{N} \right)$$
Time elapsed from initial to current isotope ratio.
What is in the formula
tvariableelapsed time — time second
λvariabledecay constant — decay constant per second
N_0variableinitial number of radioactive nuclei — number of nuclei
Nvariablecurrent number of radioactive nuclei — number of nuclei
lnoperatornatural logarithm of the ratio — natural logarithm
t=\frac{1}{λ}\ln(\frac{(^{26}{al}/^{27}{al})_0}{(^{26}{al}/^{27}{al})_{{sample}}}) · 2606.04529v1
$$L_H \propto \frac{dL_S}{dt}$$
Relates instantaneous non-thermal emission to plasma heating rate.
What is in the formula
L_HvariableInstantaneous non-thermal emission (luminosity) — luminosity watt
L_SvariablePlasma heating rate (energy per time) — power watt
\frac{d}{dt}operatorComputes the rate of change with respect to time — time derivative
l_h\propto\frac{dl_s}{dt} · 2606.25636
$$p = \frac{\rho R T}{\mu}$$
Pressure relates to density, temperature, and molar mass.
What is in the formula
pvariablePressure of the gas — pressure pascal
ρvariableMass density of the gas — mass density kilogram per metre cubed
TvariableAbsolute temperature — temperature kelvin
μvariableMean molar mass of the gas mixture — molar mass kilogram per mole
RconstantUniversal gas constant relating energy scale to temperature — gas constant = 8.314462618 joule per mole kelvin
p=ρ\frac{rt}{μ} · 2607.02691
$$\frac{P_c v_c}{T_c} = \text{const}$$
Critical pressure, volume, and temperature have a constant ratio.
What is in the formula
P_cvariableCritical pressure — pressure pascal
v_cvariableCritical molar volume — molar volume cubic metre per mole
T_cvariableCritical temperature — temperature kelvin
\frac{p_cv_c}{t_c}={const} · 2512.19200
$$w = \frac{P}{\rho}$$
Relates pressure to energy density in cosmology.
What is in the formula
wvariableequation of state parameter — equation of state parameter
Pvariablepressure — pressure pascal
ρvariableenergy density — energy density joule per cubic metre
φ=p/\varepsilon · 2601.02980v1
w=-1 · 2601.06656v1
w=-1 · 2605.20060
w=\frac{p}{ρ} · 2605.13705v1
$$P(v) = \sqrt{\frac{2}{\pi}} \frac{v^2}{\sigma^3} \exp\left(-\frac{v^2}{2\sigma^2}\right)$$
Probability distribution of speeds in an ideal gas.
What is in the formula
P(v)variableProbability density of speed v — probability density second per metre
vvariableSpeed of a particle — speed metre per second
σvariableScale parameter related to temperature — speed scale metre per second
expoperatorExponential function — exponential function
√operatorSquare root — square root
p(v_{{kick}})=\sqrt{\frac{2}{π}}\frac{v_{{kick}}^2}{σ_{{kick}}^3}\exp(-\frac{v_{{kick}}^2}{2σ_{{kick}}^2}) · 2607.02653v1
f(v)=\frac{1}{n}\exp(-\frac{v^2}{2σ_v^2})\theta(v_{\rmesc}-v) · 2607.20620v1

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