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Lesson Directive // ThermodynamicsREF_CORE

The Ideal Gas Model

PPVV==nnRRTT

Hover over a variable in the formula above, or see glossary below:

PP
Pressure
Pascals (Pa)
VV
Volume
Cubic metres (m³)
nn
Amount of Substance
Moles (mol)
RR
Ideal Gas Constant
J/(mol·K)
TT
Temperature
Kelvin (K)

An ideal gas is a theoretical model where gas molecules are perfectly elastic point particles that do not interact with each other. Real gases approximate this model well under low pressure and high temperature conditions.

INSIGHT: Pressure is caused by gas molecules bouncing off container walls millions of times per second.

The Four Laws Combined

PV = nRT combines Boyle's Law (P ∝ 1/V at constant T), Charles's Law (V ∝ T at constant P), and Avogadro's Law (V ∝ n) into a single unified equation for predicting gas behaviour.

INSIGHT: If you know any four of the five quantities, you can solve for the fifth.

Entropy & the Second Law

The Second Law of Thermodynamics states that the total entropy of an isolated system always increases. Heat flows spontaneously from hot to cold — never the reverse — because the disordered state is statistically overwhelmingly more probable.

INSIGHT: Entropy always increases. Ordered systems naturally tend toward disorder.
Detailed Theory & ReferencesEXT_DOC

The Ideal Gas Law and Thermodynamics

The Ideal Gas Law is the equation of state for a hypothetical ideal gas, a useful approximation for many real gases under standard conditions:

PV=nRTPV = nRT

State Variables

SymbolQuantitySI Unit
PPPressurePascal (Pa)
VVVolumeCubic metre (m³)
nnAmount of substanceMole (mol)
RRIdeal gas constant8.314 J/(mol·K)
TTTemperatureKelvin (K)

The Four Laws it Unifies

  • Boyle's Law (1662): At constant temperature and amount, PV=constPV = \text{const}, so P1/VP \propto 1/V.
  • Charles's Law (1787): At constant pressure and amount, V/T=constV/T = \text{const}, so VTV \propto T.
  • Gay-Lussac's Law (1809): At constant volume and amount, P/T=constP/T = \text{const}, so PTP \propto T.
  • Avogadro's Law (1811): At constant pressure and temperature, V/n=constV/n = \text{const}, so VnV \propto n.

The Laws of Thermodynamics

  1. Zeroth Law: If system A is in thermal equilibrium with B, and B with C, then A is in equilibrium with C. (This defines temperature.)
  2. First Law (Conservation of Energy): The change in internal energy equals heat added minus work done: ΔU=QW\Delta U = Q - W.
  3. Second Law: The total entropy of an isolated system never decreases. Heat flows spontaneously from high to low temperature.
  4. Third Law: As temperature approaches absolute zero, the entropy of a perfect crystal approaches a constant minimum.

Entropy

Entropy SS is a measure of the number of microscopic configurations Ω\Omega consistent with a macroscopic state: S=kBlnΩS = k_B \ln \Omega where kB=1.38×1023k_B = 1.38 \times 10^{-23} J/K is the Boltzmann constant.

References

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