2.4.2States of Matter (Quantitative)

Combined gas law and ideal gas equation PV = nRT

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WHY do we even need this?

We already know three separate experimental laws:

Law Holds what constant Relation Meaning
Boyle n,Tn, T PV=constPV = \text{const} squeeze → pressure up
Charles n,Pn, P V/T=constV/T = \text{const} heat → expands
Avogadro P,TP, T V/n=constV/n = \text{const} more gas → more volume

Carrying three laws is clumsy. The WHAT we want is one master equation from which all three fall out as special cases. That master equation is PV=nRTPV = nRT.


HOW to derive it from first principles

Why can we multiply proportionalities? If a quantity depends on several variables and we know how it responds to each one separately (others held fixed), the joint dependence is the product. So combine:

VnTPV \propto \frac{nT}{P}

Introduce a proportionality constant RR (the universal gas constant — same for every ideal gas, that's the whole point):

V=RnTPPV=nRTV = R\,\frac{nT}{P} \quad\Longrightarrow\quad \boxed{PV = nRT}

Why two values of RR? Same constant, different units. If PP is in atm and VV in litres, use 0.08210.0821; if SI (Pa, m³, J), use 8.3148.314. Always keep TT in kelvin — never Celsius.


Getting the Combined Gas Law (WHY it's just PV=nRTPV=nRT in disguise)

For a fixed amount of gas, nn and RR never change. So rearrange:

PVT=nR=constant\frac{PV}{T} = nR = \text{constant}

Therefore between any two states of the same sealed sample:

Why is this so useful? You never need to know nn or RR — they cancel. Perfect for "gas goes from condition 1 to condition 2" problems.

Figure — Combined gas law and ideal gas equation PV = nRT

Useful spin-offs (derive, don't memorise)

Density form. Moles n=mMn = \dfrac{m}{M} where mm = mass, MM = molar mass. Substitute:

PV=mMRT    PM=mVRT=ρRTPV = \frac{m}{M}RT \;\Longrightarrow\; PM = \frac{m}{V}RT = \rho RT

ρ=PMRT\boxed{\rho = \frac{PM}{RT}}

Why this matters: density of a gas rises with pressure and molar mass, falls with temperature — exactly what your intuition expects.

Molar volume at STP. At STP (T=273.15T=273.15 K, P=1P=1 atm), for n=1n=1: V=nRTP=1×0.0821×273.15122.4 LV = \frac{nRT}{P} = \frac{1 \times 0.0821 \times 273.15}{1} \approx 22.4\ \text{L}


Worked Examples


Common Mistakes


Active Recall

Recall Quick self-test (hide answers!)
  • Derive PV=nRTPV=nRT from Boyle, Charles, Avogadro. → multiply proportionalities VnT/PV\propto nT/P, add constant RR.
  • Why does nn vanish in the combined gas law? → it's constant for a sealed sample.
  • Value & units of RR? → 0.08210.0821 L·atm·K⁻¹·mol⁻¹ or 8.3148.314 J·K⁻¹·mol⁻¹.
  • Derive ρ=PM/RT\rho = PM/RT. → sub n=m/Mn=m/M then ρ=m/V\rho=m/V.
Recall Feynman: explain to a 12-year-old

Imagine a balloon full of bouncing balls. Pressure is how hard the balls hit the walls, volume is how big the balloon is, temperature is how fast the balls move, and moles is how many balls there are. The equation PV=nRTPV=nRT just says: if you add more balls or make them faster, they push harder or need more room. Squish the balloon smaller and each hit lands more often, so pressure climbs. One tidy rule connects all four.


Connections


Ideal gas equation
PV=nRTPV = nRT
The four quantities in PV=nRTPV=nRT
Pressure, Volume, moles (n), Temperature (in Kelvin)
Value of R in L·atm units
0.0821 L atm K1mol10.0821\ \text{L atm K}^{-1}\text{mol}^{-1}
Value of R in SI units
8.314 J K1mol18.314\ \text{J K}^{-1}\text{mol}^{-1}
Combined gas law
P1V1T1=P2V2T2\dfrac{P_1V_1}{T_1} = \dfrac{P_2V_2}{T_2}
Why does n cancel in the combined gas law
n and R are constant for a fixed (sealed) sample
Density form of ideal gas law
ρ=PMRT\rho = \dfrac{PM}{RT}
Molar volume of ideal gas at STP
22.4 L\approx 22.4\ \text{L}
Boyle's law from PV=nRT (fix n,T)
PV=PV= constant
Charles's law from PV=nRT (fix n,P)
V/T=V/T= constant
Must temperature be in Celsius or Kelvin
Kelvin (absolute), always
Convert Celsius to Kelvin
T(K)=T(°C)+273.15T(K) = T(°C) + 273.15

Concept Map

multiply

multiply

multiply

add constant

fix n and R

sub n = m/M

n=1 at STP

requires

Boyle: V prop 1/P

Charles: V prop T

Avogadro: V prop n

V prop nT/P

Constant R

PV = nRT

Combined Gas Law P1V1/T1 = P2V2/T2

Density rho = PM/RT

Molar volume 22.4 L at STP

T in kelvin

Hinglish (regional understanding)

Intuition Hinglish mein samjho

Dekho, gas ke andar chhote-chhote particles idhar-udhar bounce kar rahe hain. Unke behaviour ko samajhne ke liye chaar cheezein important hain: Pressure (PP), Volume (VV), amount yaani moles (nn), aur Temperature (TT, hamesha Kelvin mein). Ye chaaron ek single formula se jude hain — PV=nRTPV = nRT. Yahi ideal gas equation hai, aur isse hi Boyle, Charles aur Avogadro teenon laws nikal aate hain. Basically ek hi "master rule" hai jismein sab kuch aa jaata hai.

Derivation simple hai: Boyle kehta hai V1/PV \propto 1/P, Charles kehta hai VTV \propto T, aur Avogadro kehta hai VnV \propto n. Teenon ko multiply karo to VnT/PV \propto nT/P, aur proportionality constant RR daal do — bas ban gaya PV=nRTPV = nRT. RR ek universal constant hai, matlab har ideal gas ke liye same. Units ka dhyan rakho: atm-litre mein R=0.0821R = 0.0821, aur SI (Pa, m³) mein R=8.314R = 8.314.

Jab gas ek sealed container mein ho aur uski condition change ho (pehle state 1, phir state 2), tab nn aur RR constant rehte hain, to woh cancel ho jaate hain aur milta hai combined gas law: P1V1T1=P2V2T2\frac{P_1V_1}{T_1} = \frac{P_2V_2}{T_2}. Exam mein "gas ko compress kiya aur heat kiya, naya pressure batao" type questions mein yahi lagana hai — bina nn jaane bhi answer aa jaata hai.

Do sabse badi galtiyaan avoid karo: (1) Temperature ko Celsius mein mat daalo, hamesha Kelvin (°C+273°C + 273). (2) RR ki value aur units match karo — agar pressure atm mein hai to 0.08210.0821, warna galat answer. Bonus: density form ρ=PM/RT\rho = PM/RT yaad rakho, isse molar mass nikalna easy ho jaata hai.

Go deeper — visual, from zero

Test yourself — States of Matter (Quantitative)

Connections