ChemistryPC

States of Matter

Build conceptual understanding of States of Matter. Focus on definitions, mechanisms, and core principles.

1-2 Qs/year45 minPhase 3 · FOUNDATION

Concept Core

Matter exists in three principal states — solid, liquid, and gas — governed by the balance between kinetic energy and intermolecular forces. Intermolecular interactions increase in strength: dispersion (London) forces < dipole-dipole < hydrogen bonding. Stronger interactions lead to higher boiling points and lower vapour pressures.

Gas laws describe ideal gas behavior:

  • Boyle's law: PV = constant (at constant T and n)
  • Charles's law: V/T = constant (at constant P and n)
  • Gay-Lussac's law: P/T = constant (at constant V and n)
  • Avogadro's law: V ∝ n (at constant T and P)

These combine into the ideal gas equation: PV = nRT, where R = 0.0821 L·atm/(mol·K) = 8.314 J/(mol·K).

Dalton's law of partial pressures: PtotalP_{total} = p₁ + p₂ + ...; partial pressure pip_{i} = xix_{i} × PtotalP_{total} (xix_{i} = mole fraction).

Graham's law of diffusion: r₁/r₂ = √(M₂/M₁) — rate inversely proportional to square root of molar mass.

Solved Example 1: Volume of 2 mol ideal gas at 27°C and 2 atm. V = nRT/P = (2 × 0.0821 × 300)/2 Dimensional analysis: mol × L·atm/(mol·K) × K / atm = L ✓ V = 24.63 L

Solved Example 2: Rate of diffusion of gas A is twice that of gas B (MBM_{B} = 64 g/mol). Find MAM_{A}. rArB\frac{r_{A}}{r_{B}} = √(MBMA\frac{M_{B}}{M_{A}}) → 2 = √(64/MAM_{A}) → 4 = 64/MAM_{A}MAM_{A} = 16 g/mol (likely CH₄)

Solved Example 3: Total pressure of 2 mol N₂ + 3 mol O₂ in 10 L at 300 K. ntotaln_{total} = 5 mol; P = nRT/V = (5 × 0.0821 × 300)/10 = 12.315 atm pNp_{N}₂ = (25\frac{2}{5}) × 12.315 = 4.926 atm; pOp_{O}₂ = (35\frac{3}{5}) × 12.315 = 7.389 atm ✓

Kinetic molecular theory postulates random motion, elastic collisions, negligible intermolecular forces, and KE ∝ T. From PV = (13\frac{1}{3})mnc², combined with PV = nRT: Derivation of vrmsv_{rms}: PV = (13\frac{1}{3})Nmc² and PV = nRT, so (13\frac{1}{3})Nmc² = nRT.
Since N = nNₐ and m = M/Nₐ: (13\frac{1}{3})(nNₐ)(M/Nₐ)c² = nRT → c² = 3RT/M → vrmsv_{rms} = √(3RT/M).

Molecular speeds: vrmsv_{rms} = √(3RT/M), vavgv_{avg} = √(8RT/πM), vmpv_{mp} = √(2RT/M). Order: vrmsv_{rms} > vavgv_{avg} > vmpv_{mp} (ratio 1.224 : 1.128 : 1 relative to vmpv_{mp}).

Real gases deviate from ideal behavior at high pressure and low temperature. The van der Waals equation accounts for this: (P + a/V²)(V − b) = RT (per mole), where 'a' corrects for intermolecular attraction and 'b' for molecular volume.

The compressibility factor Z = PV/(nRT): Z = 1 (ideal), Z < 1 (attractive forces dominate, gas more compressible than ideal), Z > 1 (repulsive forces dominate, gas less compressible). Exception: H₂ and He show Z > 1 at all pressures because their 'a' is very small.

Boyle temperature TBT_{B} = a/(Rb) — the temperature at which a real gas behaves ideally over a wide pressure range.

Critical constants: TcT_{c} = 8a/(27Rb), PcP_{c} = a/(27b²), VcV_{c} = 3b; relationship: PcVcTc\frac{P_{cV_c}}{T_{c}} = 3R/8.

Liquefaction requires high pressure and low temperature (below TcT_{c}). The Joule-Thomson effect cools gases on expansion below the inversion temperature. Andrews isotherms for CO₂ (TcT_{c} = 31.1°C) illustrate gas-liquid-supercritical behavior.

Liquid state properties: Vapour pressure increases with temperature (more molecules escape); surface tension decreases with temperature (weaker cohesive forces); viscosity decreases with temperature for liquids (more kinetic energy overcomes intermolecular forces).

The key testable concept is ideal gas equation numericals, Graham's law calculations, and the relationship between molecular speeds (vrmsv_{rms} > vavgv_{avg} > vmpv_{mp}).

Key Testable Concept

The key testable concept is **ideal gas equation numericals, Graham's law calculations, and the relationship between molecular speeds (v_rms > v_avg > v_mp)**.

Comparison Tables

A) Gas Laws

LawStatementFormulaConstant ConditionsGraph Shape
Boyle'sVolume inversely proportional to pressurePV = const or P₁V₁ = P₂V₂T, n constantPV vs P: horizontal line; P vs V: hyperbola
Charles'sVolume directly proportional to temperatureV/T = const or V₁/T₁ = V₂/T₂P, n constantV vs T(K): straight line through origin
Gay-Lussac'sPressure directly proportional to temperatureP/T = const or P₁/T₁ = P₂/T₂V, n constantP vs T(K): straight line through origin
Avogadro'sVolume proportional to molesV ∝ n or V₁/n₁ = V₂/n₂T, P constantV vs n: straight line through origin
CombinedCombines Boyle, Charles, Gay-LussacP₁V₁/T₁ = P₂V₂/T₂n constant
Ideal gasGeneral equationPV = nRTNone (all variable)

B) Molecular Speeds

SpeedFormulaRatio (relative to vmpv_{mp})Physical Meaning
Most probable (vmpv_{mp})√(2RT/M)1.000Speed possessed by maximum number of molecules
Average (vavgv_{avg})√(8RT/πM)1.128Arithmetic mean of all molecular speeds
Root mean square (vrmsv_{rms})√(3RT/M)1.224Square root of mean of squares of speeds
Ordervmpv_{mp} < vavgv_{avg} < vrmsv_{rms}1 : 1.128 : 1.224Always in this order at any temperature

C) Ideal vs Real Gas

PropertyIdeal GasReal GasCondition for Ideal Behavior
Intermolecular forcesNonePresent (attractive + repulsive)Low pressure, high temperature
Molecular volumeNegligibleFinite (correction 'b')Very low pressure
Obeys gas lawsPerfectlyDeviates at high P, low TT >> TcT_{c}, P → 0
EquationPV = nRT(P + an²/V²)(V − nb) = nRT
Compressibility factor ZAlways 1Z < 1 or Z > 1Z → 1 at low P, high T
LiquefactionCannot be liquefiedCan be liquefied below TcT_{c}

D) Liquid State Properties

PropertyDefinitionTemperature EffectExample
Vapour pressurePressure exerted by vapour in equilibrium with liquidIncreases with TWater: 17.5 mmHg (20°C) → 760 mmHg (100°C)
Surface tensionForce per unit length at liquid surfaceDecreases with TWater has high surface tension (H-bonding)
ViscosityResistance to flowDecreases with T (liquids)Glycerol > water > diethyl ether
Boiling pointT where vapour pressure = external pressureDecreases at lower external PWater: 100°C at 1 atm, ~70°C on Everest

Study Materials

Available in the NoteTube app — start studying for free.

100 Flashcards

SM-2 spaced repetition flashcards with hints and explanations

20 Study Notes

Structured notes across 10 scientifically grounded formats

Continue studying in NoteTube

Frequently Asked Questions

Common questions about studying States of Matter for NEET 2026.

States of Matter — NEET 2026 Chemistry | NoteTube