Physics Lab

Unit 7: Thermal Physics & Thermodynamics

Thermal Physics + Thermodynamics together contribute 8–12 % of the JEE-Main physics paper and is one of the highest-yield topics on JEE-Advanced because problems mix several sub-areas (e.g. calorimetry with conduction, or kinetic theory with a thermodynamic process). Expect:

  • JEE-Main: 2–3 single-correct MCQs + 1 numerical, usually one on kinetic theory (rms / Cp,Cv / mean-free-path), one on a thermodynamic process (W, Q, ΔU\Delta U), one on heat transfer (Fourier / Stefan / Newton's cooling) and frequently one calorimetry mixture.
  • JEE-Advanced: multi-concept problems — e.g. Carnot engine driving a refrigerator that melts ice; a gas inside a thermally-conducting cylinder; PV–T graphs requiring you to identify the process and compute η\eta or COP.

The chapter is "formula-heavy" but conceptually shallow if you internalise three skeletons: first law Q=ΔU+WQ = \Delta U + W, kinetic gas PV=13Nmv2ˉPV = \tfrac{1}{3} N m \bar{v^2}, and Fourier H=kAdT/dxH = -kA\,dT/dx. Everything else is a corollary.


Concept Map

THERMAL PHYSICS
│
├── Temperature & Expansion
│     ├── Linear (α)  →  ΔL = L₀ α ΔT
│     ├── Areal  (β = 2α)
│     └── Volume (γ = 3α)  + anomalous water
│
├── Calorimetry
│     ├── Q = mcΔT (sensible heat)
│     ├── Q = mL    (latent heat)
│     └── Principle of mixtures (Σ Q = 0)
│
├── Heat Transfer
│     ├── Conduction — Fourier  H = kA ΔT / L
│     │      • Thermal resistance R = L/(kA)
│     │      • Series/Parallel rules
│     ├── Convection — Newton's law of cooling
│     │      dT/dt = -k(T − T_s)
│     └── Radiation — Stefan-Boltzmann, Wien, Kirchhoff
│
KINETIC THEORY OF GASES
│
├── PV = ⅓ N m ⟨v²⟩    →  ⟨KE⟩ = (3/2) kT
├── v_rms : v_avg : v_mp  =  √3 : √(8/π) : √2
├── Equipartition  →  C_v = (f/2)R, C_p = C_v + R, γ = 1 + 2/f
└── Mean free path  λ = 1/(√2 n π d²)
│
THERMODYNAMICS
│
├── First law  Q = ΔU + W
├── Processes
│     ├── Isothermal     W = nRT ln(V₂/V₁)
│     ├── Adiabatic      PVᵞ = const, W = (P₁V₁ − P₂V₂)/(γ−1)
│     ├── Isobaric       W = PΔV
│     ├── Isochoric      W = 0
│     └── Polytropic     PVⁿ = const, W = (P₁V₁ − P₂V₂)/(n−1)
│
├── Cyclic processes — Net W = area on PV diagram
│
├── Engines  η = W/Q_h  ≤  1 − T_c/T_h  (Carnot bound)
├── Refrigerator  COP = Q_c/W
└── Second law (Kelvin–Planck ⇔ Clausius), Entropy ↑

Topic 1: Thermal Expansion

Sub-topic A: Linear, Areal & Volume Expansion

When a solid is heated, its dimensions change. For small temperature changes ΔT\Delta T, the relative change is linear:

ΔL=L0αΔT,ΔA=A0βΔT,ΔV=V0γΔT\Delta L = L_0 \, \alpha \, \Delta T, \quad \Delta A = A_0 \, \beta \, \Delta T, \quad \Delta V = V_0 \, \gamma \, \Delta T

where α\alpha, β\beta, γ\gamma are the coefficients of linear, superficial, and cubical expansion respectively.

Derivation of β=2α\beta = 2\alpha and γ=3α\gamma = 3\alpha for isotropic solids:

Take a square of side L0L_0. Its area is A0=L02A_0 = L_0^2. After heating,

A=L2=L02(1+αΔT)2L02(1+2αΔT)A = L^2 = L_0^2(1 + \alpha \Delta T)^2 \approx L_0^2 (1 + 2\alpha \Delta T)

(neglecting (αΔT)2(\alpha \Delta T)^2 since α105K1\alpha \sim 10^{-5}\,\text{K}^{-1}).

So ΔA/A0=2αΔTβ=2α\Delta A / A_0 = 2\alpha \Delta T \Rightarrow \beta = 2\alpha.

Similarly for a cube of volume V0=L03V_0 = L_0^3:

V=L03(1+αΔT)3L03(1+3αΔT)γ=3αV = L_0^3 (1 + \alpha \Delta T)^3 \approx L_0^3 (1 + 3\alpha \Delta T) \Rightarrow \gamma = 3\alpha

Hence the famous ratio:

α:β:γ=1:2:3\boxed{\alpha : \beta : \gamma = 1 : 2 : 3}

Sub-topic B: Apparent vs Real Expansion of Liquids

Liquids do not have shape — only γ\gamma matters. But if the container also expands,

γapparent=γrealγcontainer\gamma_{\text{apparent}} = \gamma_{\text{real}} - \gamma_{\text{container}}

This is why a flask appears to "lose" liquid when first heated (container expands faster) then overflows once the liquid catches up.

Sub-topic C: Anomalous Expansion of Water

Water has a density maximum at 4 °C. From 0 to 4 °C it contracts, then expands above 4 °C. This is why lakes freeze top-down — denser 4 °C water sinks, ice (less dense) floats and insulates, allowing aquatic life to survive.

Sub-topic D: Bimetallic Strip & Thermal Stress

A bimetallic strip is two metals (different α\alpha) bonded together. On heating, the metal with higher α\alpha expands more — the strip bends towards the metal with lower α\alpha. Used in thermostats.

Thermal stress in a clamped rod (cannot expand):

σ=YαΔT\sigma = Y \, \alpha \, \Delta T

derived from ΔL/L=αΔT\Delta L / L = \alpha \Delta T would be the expansion if free, but it's prevented; so an equivalent compressive strain αΔT\alpha \Delta T is imposed, giving stress YαΔTY \alpha \Delta T.

Worked Problem 1 (JEE-Main level)

A steel rod of length 1m1\,\text{m} and area 1cm21\,\text{cm}^2 is clamped between two rigid walls at 20C20\,^\circ \text{C}. Find the force on the walls when heated to 120C120\,^\circ \text{C}. Take Y=2×1011Y = 2\times 10^{11} Pa and α=1.2×105K1\alpha = 1.2 \times 10^{-5}\,\text{K}^{-1}.

Solution. σ=YαΔT=2×1011×1.2×105×100=2.4×108\sigma = Y \alpha \Delta T = 2\times 10^{11} \times 1.2\times 10^{-5}\times 100 = 2.4 \times 10^{8} Pa.

F=σA=2.4×108×104=2.4×104F = \sigma A = 2.4 \times 10^8 \times 10^{-4} = 2.4 \times 10^{4} N =24= 24 kN.

Worked Problem 2 (JEE-Advanced trap)

A circular hole of diameter 2cm2\,\text{cm} is drilled in a steel plate at 20C20\,^\circ\text{C}. To what diameter does the hole grow at 100C100\,^\circ\text{C}? (αsteel=1.2×105K1\alpha_{\text{steel}} = 1.2 \times 10^{-5}\,\text{K}^{-1}.)

Trap: Beginners think the hole shrinks. It doesn't — every linear dimension (including a void) scales by (1+αΔT)(1 + \alpha \Delta T).

d=2cm×(1+1.2×105×80)=2cm(1+9.6×104)2.00192cmd = 2\,\text{cm} \times (1 + 1.2\times 10^{-5}\times 80) = 2\,\text{cm}\,(1 + 9.6\times 10^{-4}) \approx 2.00192\,\text{cm}.


Topic 2: Calorimetry

Sub-topic A: Specific Heat and Latent Heat

Sensible heat (raises temperature):

Q=mcΔTQ = m c \Delta T

Latent heat (causes phase change at constant temperature):

Q=mLQ = m L

Standard JEE values to memorise:

QuantityValue
Specific heat of watercw=4186J/(kg⋅K)1cal/(g⋅K)c_w = 4186\,\text{J/(kg·K)} \approx 1\,\text{cal/(g·K)}
Specific heat of iceci=2100J/(kg⋅K)c_i = 2100\,\text{J/(kg·K)}
Latent heat of fusion (ice)Lf=3.34×105J/kg=80cal/gL_f = 3.34\times 10^5\,\text{J/kg} = 80\,\text{cal/g}
Latent heat of vaporisation (water)Lv=2.26×106J/kg=540cal/gL_v = 2.26 \times 10^6\,\text{J/kg} = 540\,\text{cal/g}

Sub-topic B: Principle of Mixtures

In an isolated system, Q=0\sum Q = 0 — heat lost by hot bodies equals heat gained by cold bodies, including any phase changes.

Worked Problem 3 (Ice-Steam)

1010 g of ice at 0C0\,^\circ\text{C} is added to 5050 g of water at 40C40\,^\circ\text{C} in a thermally-insulated calorimeter (mass effects ignored). Find the final temperature.

Solution. Heat available from cooling the water from 40 °C to 0 °C: Qavailable=50×1×40=2000Q_{\text{available}} = 50 \times 1 \times 40 = 2000 cal.

Heat to melt all ice: Qmelt=10×80=800Q_{\text{melt}} = 10 \times 80 = 800 cal.

Excess = 2000800=12002000 - 800 = 1200 cal — used to warm the 6060 g of water (now all liquid) from 00\,^\circC.

Tf=1200/(60×1)=20CT_f = 1200 / (60 \times 1) = 20\,^\circ\text{C}.

Worked Problem 4 (JEE-Advanced: partial phase change)

11 kg of steam at 100C100\,^\circ\text{C} is mixed with 11 kg of ice at 0C0\,^\circ\text{C}. Find the final state.

Solution. Maximum heat steam can release while condensing: Q1=1000×540=5.4×105Q_1 = 1000 \times 540 = 5.4\times 10^5 cal.

Heat to melt ice + warm to 100C100\,^\circ\text{C}: Q2=1000×80+1000×1×100=1.8×105Q_2 = 1000 \times 80 + 1000 \times 1 \times 100 = 1.8\times 10^5 cal.

Since Q1>Q2Q_1 > Q_2, steam over-supplies. Heat left after Q2Q_2 is used: 5.4×1051.8×105=3.6×1055.4\times 10^5 - 1.8\times 10^5 = 3.6\times 10^5 cal.

This 3.6×1053.6\times 10^5 cal further condenses steam at 100C100\,^\circ\text{C}: mass condensed =3.6×105/540=667= 3.6\times 10^5 / 540 = 667 g.

So 667667 g of steam condenses to water, and the final mixture at 100C100\,^\circ\text{C} contains: 667+1000=1667667 + 1000 = 1667 g of water + 1000667=3331000 - 667 = 333 g of steam.

Trap: Don't assume the system ends as a single phase — sometimes it equilibrates partway through a phase change.


Topic 3: Heat Transfer

Sub-topic A: Conduction — Fourier's Law

Heat current (rate) through a slab of cross-section AA, length LL, with hot face at T1T_1 and cold face at T2T_2 in steady state:

H=dQdt=kAdTdxH = \frac{dQ}{dt} = -kA\frac{dT}{dx}

For a rod with constant cross-section in steady state, HH is uniform, so dT/dxdT/dx is constant, and

H=kA(T1T2)LH = \frac{kA(T_1 - T_2)}{L}

Thermal resistance (analogous to electrical):

R=LkA,H=ΔTRR = \frac{L}{kA}, \qquad H = \frac{\Delta T}{R}

Derivation of T(x)T(x) profile (linear):

Steady state \Rightarrow HH independent of xx:

dTdx=HkA    (constant)    T(x)=T1(T1T2)Lx\frac{dT}{dx} = -\frac{H}{kA} \;\;\text{(constant)}\;\Rightarrow\; T(x) = T_1 - \frac{(T_1-T_2)}{L}x

So the temperature drops linearly along a uniform rod in steady state. (Not so if kk or AA varies with xx.)

Sub-topic B: Series and Parallel Thermal Resistance

Series (rods end-to-end, same heat current):

Req=R1+R2+R_{\text{eq}} = R_1 + R_2 + \ldots

For two rods of equal area:

L1+L2keqA=L1k1A+L2k2Akeq=L1+L2L1/k1+L2/k2\frac{L_1+L_2}{k_{\text{eq}}A} = \frac{L_1}{k_1 A} + \frac{L_2}{k_2 A} \Rightarrow k_{\text{eq}} = \frac{L_1+L_2}{L_1/k_1 + L_2/k_2}

Parallel (rods side-by-side, same ΔT\Delta T):

1Req=1R1+1R2+\frac{1}{R_{\text{eq}}} = \frac{1}{R_1}+\frac{1}{R_2}+\ldots

For two rods of equal length:

keq=k1A1+k2A2A1+A2k_{\text{eq}} = \frac{k_1 A_1 + k_2 A_2}{A_1+A_2}

Worked Problem 5 (Compound rod)

Two rods of equal length and area but conductivities kk and 3k3k are joined end-to-end. Hot end at 100100\,^\circC, cold end at 00\,^\circC. Find junction temperature.

Solution. Same HH through both:

kA(100T)L=3kA(T0)L\frac{k A (100 - T)}{L} = \frac{3k A (T - 0)}{L}

100T=3TT=25C\Rightarrow 100 - T = 3T \Rightarrow T = 25\,^\circ\text{C}.

Sub-topic C: Convection — Newton's Law of Cooling

For a body at temperature TT in surroundings at TsT_s, with TTsT - T_s small,

dTdt=k(TTs)\frac{dT}{dt} = -k(T - T_s)

Derivation (from Stefan's law):

Net radiative loss is P=eσA(T4Ts4)P = e\sigma A (T^4 - T_s^4). Writing T=Ts+θT = T_s + \theta with θTs\theta \ll T_s:

T4Ts44Ts3θT^4 - T_s^4 \approx 4T_s^3 \theta

So PθP \propto \theta. Energy balance mcdθ/dt=Pdθ/dt=kθmc \, d\theta/dt = -P \Rightarrow d\theta/dt = -k\theta where k=4eσATs3/(mc)k = 4e\sigma A T_s^3/(mc).

Solution: T(t)=Ts+(T0Ts)ektT(t) = T_s + (T_0 - T_s) e^{-kt}.

Sub-topic D: Radiation

Stefan-Boltzmann Law (total radiant exitance of a black body):

P=σAT4,σ=5.67×108W⋅m2K4\boxed{P = \sigma A T^4}, \qquad \sigma = 5.67\times 10^{-8}\,\text{W·m}^{-2}\text{K}^{-4}

For a body with emissivity e[0,1]e \in [0,1]: P=eσAT4P = e\sigma A T^4.

Net rate of radiation between body at TT and surroundings at TsT_s:

Pnet=eσA(T4Ts4)P_{\text{net}} = e\sigma A (T^4 - T_s^4)

Wien's Displacement Law: peak emission wavelength

λmaxT=b,b=2.898×103m⋅K\lambda_{\max} T = b, \quad b = 2.898 \times 10^{-3}\,\text{m·K}

(So the sun at 5800\sim 5800 K peaks at 500\sim 500 nm — visible.)

Kirchhoff's Law: at thermal equilibrium, emissivity = absorptivity at every wavelength. Good absorbers are good emitters — a black body is the perfect absorber and emitter.

Worked Problem 6 (Stefan)

A body at 327327\,^\circC is placed in surroundings at 2727\,^\circC. Power radiated is 8080 W. Find the power radiated when the body's temperature is 727727\,^\circC, surroundings unchanged.

Solution. T1=600T_1 = 600 K, T2=1000T_2 = 1000 K, Ts=300T_s = 300 K. Emissivity, area same:

P2P1=T24Ts4T14Ts4=10120.81×10101.296×10110.81×1010=991.9121.58.16\frac{P_2}{P_1} = \frac{T_2^4 - T_s^4}{T_1^4 - T_s^4} = \frac{10^{12} - 0.81\times 10^{10}}{1.296\times 10^{11} - 0.81\times 10^{10}}=\frac{991.9}{121.5}\approx 8.16

P28.16×80653P_2 \approx 8.16 \times 80 \approx 653 W.

Worked Problem 7 (Newton's cooling)

A liquid cools from 8080\,^\circC to 6060\,^\circC in 55 min in surroundings at 2020\,^\circC. Find time to cool from 6060\,^\circC to 4040\,^\circC.

Solution. Use approximate form T1T2t=k(T1+T22Ts)\frac{T_1-T_2}{t} = k\left(\frac{T_1+T_2}{2}-T_s\right).

For 80→60: 205=k(7020)k=4/50=0.08min1\frac{20}{5} = k(70-20)\Rightarrow k = 4/50 = 0.08\,\text{min}^{-1}.

For 60→40: 20t=0.08(5020)=2.4t8.33\frac{20}{t} = 0.08(50-20)=2.4\Rightarrow t \approx 8.33 min.


Topic 4: Kinetic Theory of Gases

Sub-topic A: Derivation of Gas Pressure

Consider NN molecules of mass mm in a cube of side LL. Molecules move randomly with mean square speed v2\overline{v^2}.

Take a molecule with velocity components (vx,vy,vz)(v_x, v_y, v_z). On hitting the wall normal to xx-axis it reverses vxvxv_x \to -v_x, Δp=2mvx\Delta p = 2 m v_x. It returns to the same wall after time Δt=2L/vx\Delta t = 2L/v_x.

Force from one molecule on this wall:

F1=ΔpΔt=2mvx2L/vx=mvx2LF_1 = \frac{\Delta p}{\Delta t} = \frac{2m v_x}{2L/v_x} = \frac{m v_x^2}{L}

Summing over NN molecules and averaging:

F=mLvx2=Nmvx2LF = \frac{m}{L} \sum v_x^2 = \frac{N m \overline{v_x^2}}{L}

By isotropy, vx2=vy2=vz2=v2/3\overline{v_x^2} = \overline{v_y^2} = \overline{v_z^2} = \overline{v^2}/3. Pressure:

P=FL2=Nmv23L3=13ρv2P = \frac{F}{L^2} = \frac{N m \overline{v^2}}{3 L^3} = \frac{1}{3}\rho \overline{v^2}

Hence the fundamental result:

PV=13Nmv2\boxed{PV = \tfrac{1}{3}N m \overline{v^2}}

Sub-topic B: Temperature & Average Kinetic Energy

Combining with PV=NkBTPV = N k_B T:

13Nmv2=NkBT12mv2=32kBT\tfrac{1}{3} N m \overline{v^2} = N k_B T \Rightarrow \tfrac{1}{2} m \overline{v^2} = \tfrac{3}{2} k_B T

So average translational KE per molecule is 32kBT\tfrac{3}{2} k_B T, independent of mass — the deep physical meaning of temperature.

Sub-topic C: Maxwell Speed Distribution — Three Speeds

Maxwell-Boltzmann:

f(v)=4πn(m2πkBT)3/2v2emv2/2kBTf(v) = 4\pi n \left( \frac{m}{2\pi k_B T} \right)^{3/2} v^2 e^{-mv^2/2k_B T}

You only need three derived speeds:

SpeedFormulaNumerical ratio
Most-probable vmpv_{mp}2kBT/m\sqrt{2 k_B T / m}2\sqrt{2}
Average vˉ\bar v8kBT/(πm)\sqrt{8 k_B T /(\pi m)}8/π1.596\sqrt{8/\pi} \approx 1.596
RMS vrmsv_{rms}3kBT/m\sqrt{3 k_B T / m}31.732\sqrt{3} \approx 1.732
vmp:vˉ:vrms=2:8/π:3\boxed{v_{mp} : \bar v : v_{rms} = \sqrt{2} : \sqrt{8/\pi} : \sqrt{3}}

Sub-topic D: Equipartition & Degrees of Freedom

Equipartition theorem: every quadratic degree of freedom contributes 12kBT\tfrac{1}{2}k_B T to the average energy.

Gas typeffU/n=(f/2)RTU/n = (f/2)RTCvC_vCpC_pγ\gamma
Monatomic (He, Ne)332RT\tfrac{3}{2}RT32R\tfrac{3}{2}R52R\tfrac{5}{2}R5/35/3
Diatomic, no vib (O₂, N₂ at 300 K)552RT\tfrac{5}{2}RT52R\tfrac{5}{2}R72R\tfrac{7}{2}R7/57/5
Diatomic, vib excited (high T)772RT\tfrac{7}{2}RT72R\tfrac{7}{2}R92R\tfrac{9}{2}R9/79/7
Polyatomic non-linear (H₂O, NH₃)63RT3RT3R3R4R4R4/34/3

Mayer's relation (proof for ideal gas):

Qp=nCpΔTQ_p = nC_p \Delta T, Qv=nCvΔTQ_v = nC_v \Delta T. At constant pressure W=nRΔTW = nR\Delta T, ΔU=nCvΔT\Delta U = nC_v \Delta T. First law nCpΔT=nCvΔT+nRΔT\Rightarrow nC_p\Delta T = nC_v\Delta T + nR\Delta T:

CpCv=R\boxed{C_p - C_v = R}

Also γ=Cp/Cv=1+2/f\gamma = C_p/C_v = 1 + 2/f.

Sub-topic E: Mean Free Path

Average distance between collisions:

λ=12nπd2\lambda = \frac{1}{\sqrt{2}\, n\, \pi d^2}

where n=N/Vn = N/V is number density and dd is the molecular diameter. The 2\sqrt{2} comes from relative velocity of two moving molecules.

Worked Problem 8 (mixing gases)

11 mol of He\text{He} (γ1=5/3\gamma_1 = 5/3) and 22 mol of O2\text{O}_2 (γ2=7/5\gamma_2 = 7/5) are mixed. Find γmix\gamma_{\text{mix}}.

Solution. Equivalent CvC_v:

Cv,mix=n1Cv,1+n2Cv,2n1+n2=132R+252R3=32+53R=136RC_{v,\text{mix}} = \frac{n_1 C_{v,1} + n_2 C_{v,2}}{n_1+n_2}=\frac{1\cdot\tfrac{3}{2}R + 2\cdot\tfrac{5}{2}R}{3}=\frac{\tfrac{3}{2}+5}{3}R=\frac{13}{6}R

Cp,mix=Cv,mix+R=19R/6C_{p,\text{mix}} = C_{v,\text{mix}} + R = 19R/6. So

γmix=19/613/6=19131.46\gamma_{\text{mix}} = \frac{19/6}{13/6} = \frac{19}{13} \approx 1.46

Worked Problem 9 (rms vs avg)

Find the temperature at which the rms speed of O2\text{O}_2 equals the rms speed of N2\text{N}_2 at 300300 K. (MO2=32M_{\text{O}_2}=32, MN2=28M_{\text{N}_2}=28.)

Solution. vrms=3RT/Mv_{rms} = \sqrt{3RT/M}. Equating:

TO232=30028TO2=300×3228342.9K.\frac{T_{\text{O}_2}}{32}=\frac{300}{28}\Rightarrow T_{\text{O}_2}=\frac{300\times 32}{28}\approx 342.9\,\text{K}.

Topic 5: First Law of Thermodynamics & Processes

Sub-topic A: First Law

Q=ΔU+W\boxed{Q = \Delta U + W}

with the IUPAC/physics convention: Q>0Q > 0 if heat is added to the system, W>0W > 0 if work is done by the system. (Won=WbyW_{\text{on}} = -W_{\text{by}}, careful!).

For an ideal gas, ΔU=nCvΔT\Delta U = nC_v \Delta Talways, regardless of the process — because UU depends only on TT.

Sub-topic B: The Four Basic Processes

For an ideal gas (n moles):

Isothermal (TT const). ΔU=0\Delta U = 0, so Q=WQ = W.

W=V1V2PdV=nRTln(V2/V1)W = \int_{V_1}^{V_2} P\, dV = nRT \ln(V_2/V_1)

Isobaric (PP const).

W=PΔV=nRΔT,Q=nCpΔT,ΔU=nCvΔTW = P\Delta V = nR\Delta T, \quad Q = nC_p \Delta T,\quad \Delta U = nC_v \Delta T

Isochoric (VV const).

W=0,Q=ΔU=nCvΔTW = 0,\quad Q = \Delta U = nC_v\Delta T

Adiabatic (Q=0Q = 0). ΔU=W\Delta U = -W and PVγ=constPV^\gamma = \text{const}.

Derivation of PVγ=constPV^\gamma = \text{const}: First law adiabatic nCvdT+PdV=0\Rightarrow nC_v dT + P\, dV = 0. Use PV=nRTnRdT=PdV+VdPPV = nRT \Rightarrow nR\, dT = P\, dV + V\, dP:

CvR(PdV+VdP)+PdV=0\frac{C_v}{R}(P\, dV + V\, dP) + P\, dV = 0 (Cv+R)PdV+CvVdP=0\Rightarrow (C_v + R)P\, dV + C_v V\, dP = 0 CpdV/V+CvdP/P=0\Rightarrow C_p\, dV/V + C_v\, dP/P = 0

Integrate: γlnV+lnP=constPVγ=const\gamma \ln V + \ln P = \text{const}\Rightarrow PV^\gamma = \text{const}.

Work done in adiabatic:

W=V1V2CVγdV=P1V1P2V2γ1=nR(T1T2)γ1W = \int_{V_1}^{V_2} \frac{C}{V^\gamma} dV = \frac{P_1 V_1 - P_2 V_2}{\gamma - 1} = \frac{nR(T_1 - T_2)}{\gamma - 1}

Sub-topic C: Master Table

ProcessWWΔU\Delta UQQCC (molar)
IsothermalnRTln(V2/V1)nRT\ln(V_2/V_1)00nRTln(V2/V1)nRT\ln(V_2/V_1)\infty
Isochoric00nCvΔTnC_v\Delta TnCvΔTnC_v\Delta TCvC_v
IsobaricnRΔTnR\Delta TnCvΔTnC_v\Delta TnCpΔTnC_p\Delta TCpC_p
AdiabaticnR(T1T2)γ1\dfrac{nR(T_1-T_2)}{\gamma-1}nCvΔTnC_v\Delta T0000
Polytropic (PVn=cPV^n=\text{c})nR(T1T2)n1\dfrac{nR(T_1-T_2)}{n-1}nCvΔTnC_v\Delta TnCΔTnC\Delta TCvRn1C_v - \dfrac{R}{n-1}

The polytropic molar heat capacity is a deep JEE-Advanced result, derivable from first law with W=nRΔT/(1n)W = nR\Delta T/(1-n) and ΔU=nCvΔT\Delta U = nC_v\Delta T.

Sub-topic D: Slopes on PV Diagram

  • Isobar: horizontal
  • Isochor: vertical
  • Isotherm: dP/dV=P/VdP/dV = -P/V
  • Adiabat: dP/dV=γP/VdP/dV = -\gamma P/Vsteeper than isotherm at any common point.

Worked Problem 10 (Adiabatic compression)

A monatomic ideal gas at 300300 K, 11 atm is compressed adiabatically to one-eighth its initial volume. Find the final temperature and pressure.

Solution. γ=5/3\gamma = 5/3. TVγ1=constTV^{\gamma-1} = \text{const}:

T2=T1(V1/V2)γ1=30082/3=3004=1200KT_2 = T_1 (V_1/V_2)^{\gamma-1} = 300\cdot 8^{2/3} = 300\cdot 4 = 1200\,\text{K}

P2=P1(V1/V2)γ=185/3=32P_2 = P_1 (V_1/V_2)^\gamma = 1\cdot 8^{5/3} = 32 atm.

Worked Problem 11 (Multi-process)

11 mole of ideal gas undergoes a cycle ABCA where AB is isobaric (P=2P0P=2P_0, V02V0V_0 \to 2V_0), BC is isochoric (PP0P \to P_0), CA is isothermal (VV0V \to V_0). Find net work over the cycle.

Solution. At A: (P,V)=(2P0,V0)TA=2P0V0/R(P,V) = (2P_0, V_0) \Rightarrow T_A = 2P_0 V_0/R. At B: (2P0,2V0)TB=4P0V0/R(2P_0, 2V_0)\Rightarrow T_B = 4P_0 V_0/R. At C: (P0,2V0)TC=2P0V0/R=TA(P_0, 2V_0) \Rightarrow T_C = 2P_0V_0/R = T_A. Good, CA is isothermal.

WAB=PΔV=2P0V0=2P0V0W_{AB} = P\Delta V = 2P_0 \cdot V_0 = 2P_0V_0. WBC=0W_{BC} = 0. WCA=nRTAln(V0/2V0)=2P0V0ln(1/2)=2P0V0ln2W_{CA} = nRT_A \ln(V_0/2V_0) = 2P_0V_0 \ln(1/2) = -2P_0V_0\ln 2.

Wnet=2P0V0(1ln2)2P0V0(10.693)0.614P0V0W_{\text{net}} = 2P_0V_0(1 - \ln 2) \approx 2P_0V_0 (1 - 0.693) \approx 0.614\,P_0V_0.


Topic 6: Cyclic Processes, Heat Engines & Carnot Cycle

Sub-topic A: Cyclic Processes — Net Work = Area

In a cycle, dU=0\oint dU = 0 since UU is a state function. Hence dQ=dW\oint dQ = \oint dW. The net work equals the enclosed area on a P-V diagram.

  • Clockwise loop \Rightarrow engine (net W>0W > 0, heat absorbed from hot reservoir);
  • Counter-clockwise \Rightarrow refrigerator (net W<0W < 0, heat dumped uphill).

Sub-topic B: Heat Engines & Efficiency

A heat engine takes QhQ_h from a hot reservoir, dumps QcQ_c to a cold reservoir, produces work W=QhQcW = Q_h - Q_c.

η=WQh=1QcQh\eta = \frac{W}{Q_h} = 1 - \frac{Q_c}{Q_h}

For a refrigerator:

COP=QcW=QcQhQc\text{COP} = \frac{Q_c}{W} = \frac{Q_c}{Q_h - Q_c}

For a heat pump:

COPHP=QhW=COPref+1\text{COP}_{\text{HP}} = \frac{Q_h}{W} = \text{COP}_{\text{ref}} + 1

Sub-topic C: Carnot Cycle — Full Derivation

Four reversible processes: A→B isothermal expansion at ThT_h, B→C adiabatic expansion (ThTcT_h\to T_c), C→D isothermal compression at TcT_c, D→A adiabatic compression (TcThT_c \to T_h).

Heat absorbed in A→B (isothermal):

Qh=nRThln(VB/VA)Q_h = nRT_h \ln(V_B/V_A)

Heat released in C→D (isothermal):

Qc=nRTcln(VC/VD)Q_c = nRT_c \ln(V_C/V_D)

Adiabatic legs give:

ThVBγ1=TcVCγ1,ThVAγ1=TcVDγ1T_h V_B^{\gamma-1} = T_c V_C^{\gamma-1},\qquad T_h V_A^{\gamma-1} = T_c V_D^{\gamma-1}

Dividing VB/VA=VC/VD\Rightarrow V_B/V_A = V_C/V_D. So ln\ln terms cancel and

ηCarnot=1TcTh\boxed{\eta_{\text{Carnot}} = 1 - \frac{T_c}{T_h}}

Sub-topic D: Carnot Theorem

(i) No engine working between two reservoirs can be more efficient than a reversible (Carnot) engine operating between them.

(ii) All reversible engines between the same two reservoirs have the same efficiency, independent of working substance.

Proof is a classic reductio ad absurdum: suppose another engine XX with ηX>ηC\eta_X > \eta_C. Use XX to drive a reversed Carnot engine — net effect would transfer heat from cold to hot reservoir with no work done, violating Clausius statement.

Sub-topic E: Second Law — Equivalent Statements

Kelvin–Planck: It is impossible to construct a device which extracts heat from a single reservoir and converts all of it into work in a cycle.

Clausius: It is impossible to construct a device which transfers heat from a colder body to a hotter body without any external work.

Equivalence: Violation of K-P \Rightarrow violation of Clausius (and vice versa), shown by chaining engines.

Sub-topic F: Entropy (Qualitative)

For a reversible process,

dS=dQrevTdS = \frac{dQ_{\text{rev}}}{T}

SS is a state function. For an isolated system ΔS0\Delta S \ge 0 (= 0 only if reversible). This is the second law in its most powerful form.

For an ideal gas reversibly between two states:

ΔS=nCvln(T2/T1)+nRln(V2/V1)\Delta S = nC_v \ln(T_2/T_1) + nR\ln(V_2/V_1)

Worked Problem 12 (Carnot)

A Carnot engine takes 10001000 J from a reservoir at 500500 K. The sink is at 300300 K. Find WW done and QcQ_c rejected.

Solution. η=1300/500=0.4\eta = 1 - 300/500 = 0.4. W=0.4×1000=400W = 0.4 \times 1000 = 400 J; Qc=600Q_c = 600 J.

Worked Problem 13 (Refrigerator + freezing water)

A refrigerator with COP = 55 removes heat from water at 00\,^\circC and dumps it into a room at 2727\,^\circC. How much water at 00\,^\circC is frozen per minute if the compressor draws 200200 W of electrical power?

Solution. Heat removed per second Qc=COPW=5200=1000Q_c = \text{COP}\cdot W = 5\cdot 200 = 1000 J/s. In 1 minute =60= 60 kJ.

Mass frozen m=Qc/Lf=60000J/(3.34×105J/kg)0.18m = Q_c / L_f = 60000\,\text{J} / (3.34\times 10^5\,\text{J/kg}) \approx 0.18 kg = 180180 g.

Worked Problem 14 (JEE-Advanced: irreversible expansion)

22 mol of ideal monatomic gas at T0=300T_0=300 K, V0=10V_0 = 10 L expands irreversibly against a constant external pressure Pext=P0/2P_{\text{ext}} = P_0/2 where P0P_0 is initial pressure. Find the final temperature given the process is adiabatic.

Solution. Adiabatic Q=0\Rightarrow Q = 0, so ΔU=Wby gas\Delta U = -W_{\text{by gas}}. But for an irreversible expansion against constant PextP_{\text{ext}}, W=PextΔVW = P_{\text{ext}} \Delta V, not the reversible formula.

P0=nRT0/V0=2(8.314)(300)/(10×103)=4.99×105P_0 = nRT_0/V_0 = 2(8.314)(300)/(10\times10^{-3}) = 4.99\times 10^5 Pa. Pext=P0/2=2.49×105P_{\text{ext}} = P_0/2 = 2.49\times 10^5 Pa.

Final state must have Pf=PextP_f = P_{\text{ext}} (mechanical equilibrium): Vf=nRTf/PfV_f = nRT_f/P_f.

ΔU=nCv(TfT0)=Pext(VfV0)\Delta U = n C_v (T_f - T_0) = -P_{\text{ext}}(V_f - V_0):

nCv(TfT0)=Pext[nRTfPfV0]=nRTf+PextV0nC_v(T_f - T_0) = -P_{\text{ext}}\left[\frac{nRT_f}{P_f} - V_0\right] = -nRT_f + P_{\text{ext}}V_0 nCvTf+nRTf=nCvT0+PextV0\Rightarrow n C_v T_f + nR T_f = n C_v T_0 + P_{\text{ext}}V_0 n(Cv+R)Tf=nCvT0+PextV0\Rightarrow n(C_v+R) T_f = nC_v T_0 + P_{\text{ext}}V_0 Tf=nCvT0+PextV0nCpT_f = \frac{n C_v T_0 + P_{\text{ext}} V_0}{n C_p}

With Cv=32R=12.47C_v = \tfrac{3}{2}R = 12.47, Cp=52R=20.78C_p = \tfrac{5}{2}R = 20.78:

Numerator =2(12.47)(300)+(2.49×105)(10×103)=7482+2495=9977= 2(12.47)(300) + (2.49\times 10^5)(10\times 10^{-3}) = 7482 + 2495 = 9977 J. Denominator =2(20.78)=41.56= 2(20.78) = 41.56. Tf240T_f \approx 240 K.

(So the irreversible expansion is less cool than the reversible Tf=T0(Pf/P0)(γ1)/γ=300(0.5)0.4=227T_f = T_0(P_f/P_0)^{(\gamma-1)/\gamma}= 300\cdot (0.5)^{0.4}=227 K. A textbook JEE-Advanced trap.)


Problem-Solving Heuristics

  1. Choose the right CC. Heat at constant VV uses CvC_v, at constant PP uses CpC_p. For a polytropic, derive C=CvR/(n1)C = C_v - R/(n-1).
  2. Sign of WW. Always state clearly whether the convention is Wby gasW_{\text{by gas}} (most physics texts, the one used here) or Won gasW_{\text{on gas}} (chemistry).
  3. ΔU\Delta U depends only on ΔT\Delta T for an ideal gas. Use the easiest path (often isochoric) to compute ΔU\Delta U.
  4. In cycles, jump straight to areas. Compute QQ for each leg only if asked; net work is the enclosed area.
  5. Adiabat vs isotherm crossings. Adiabat is steeper by a factor of γ\gamma — this distinguishes which is which on a P-V diagram.
  6. Conduction in steady state \Rightarrow same H everywhere. Use the series-resistance picture; for parallel rods use parallel-resistance.
  7. Stefan involves T4T^4. If T2TT \to 2T, power ×16\times 16 — these factor-of-many MCQs come up.
  8. Wien gives "the colour". λmax1/T\lambda_{\max} \propto 1/T — hotter is bluer.
  9. For irreversible expansion vs reversible expansion, compute WW from W=PextΔVW = P_{\text{ext}} \Delta V if pressure is constant external, not PdV\int P\,dV.
  10. Carnot bound η1Tc/Th\eta \le 1 - T_c/T_h — any larger answer is wrong by the second law.
  11. Mean free path drops with PP at fixed TT: λ1/nT/P\lambda \propto 1/n \propto T/P.
  12. Don't confuse TrmsT_{\text{rms}} with TT itself. vrmsTv_{rms}\propto \sqrt T, not TT.

Common Traps & Mistakes

  • Hole expands too. Anything you draw on a uniformly heated body — solid disk, hole, ring of dots — scales by the same (1+αΔT)(1+\alpha\Delta T).
  • Latent heat reservoirs. Don't assume mixing ends in a single phase; check whether the heat budget exceeds latent heat.
  • Polytropic mol. heat. The formula C=Cv+R/(1n)C = C_v + R/(1-n) has a sign that flips depending on which way you write it; double-check whose convention.
  • Adiabatic process formulas apply only to reversible (quasi-static) adiabats. For sudden compression against constant external pressure, use first law directly.
  • Stefan vs Newton's cooling. Newton's law is the small-ΔT\Delta T linearisation of Stefan. They are not independent laws.
  • Wien vs Stefan. Wien tells where the peak is; Stefan tells the total radiated power. Don't confuse them.
  • Equipartition only at sufficiently high TT. At low temperatures rotational/vibrational modes "freeze out" — that's why H2\text{H}_2 behaves like a monatomic gas below 100\sim 100 K.
  • Qh=Qc+WQ_h = Q_c + W only for an engine in steady cycle. For a single process it does not hold.
  • Sign of work in compression. If gas is compressed, ΔV<0\Delta V < 0, so Wby<0W_{\text{by}} < 0. Plug signs algebraically, don't try to remember separate "expansion" and "compression" formulas.
  • Cyclic ΔU=0\Delta U = 0 but not ΔS=0\Delta S = 0 for the universe — only for the gas.

Quick Revision Card

  • Linear expansion: ΔL=L0αΔT\Delta L = L_0 \alpha \Delta T; α:β:γ=1:2:3\alpha:\beta:\gamma = 1:2:3.
  • Thermal stress: σ=YαΔT\sigma = Y\alpha\Delta T.
  • Calorimetry: Q=mcΔTQ = mc\Delta T, phase change Q=mLQ = mL.
  • Fourier: H=kAΔT/LH = kA\Delta T/L; R=L/(kA)R = L/(kA); series RR's add, parallel RR's combine.
  • Newton's cooling: dT/dt=k(TTs)dT/dt = -k(T-T_s), exponential decay.
  • Stefan: P=eσAT4P = e\sigma A T^4; Wien: λmaxT=b\lambda_{\max}T = b; Kirchhoff: e=ae = a.
  • Kinetic: KE=32kBT\langle\text{KE}\rangle = \tfrac{3}{2}k_BT; vrms=3RT/Mv_{rms} = \sqrt{3RT/M}.
  • Cv=(f/2)RC_v = (f/2)R, Cp=Cv+RC_p = C_v + R, γ=1+2/f\gamma = 1 + 2/f.
  • Mean free path λ=1/(2nπd2)\lambda = 1/(\sqrt 2 n\pi d^2).
  • First law: Q=ΔU+WQ = \Delta U + W, ΔU=nCvΔT\Delta U = nC_v\Delta T.
  • Isothermal W=nRTln(V2/V1)W = nRT\ln(V_2/V_1); adiabatic PVγ=PV^\gamma = const, W=(P1V1P2V2)/(γ1)W = (P_1V_1-P_2V_2)/(\gamma-1).
  • Cycle: net WW = enclosed area; η=W/Qh=1Qc/Qh1Tc/Th\eta = W/Q_h = 1 - Q_c/Q_h \le 1 - T_c/T_h.
  • COP refrigerator =Qc/W= Q_c/W; COP heat pump =Qh/W=COPref+1= Q_h/W = \text{COP}_{\text{ref}} + 1.

Formula Sheet

ConceptFormula
Linear expansionΔL=L0αΔT\Delta L = L_0 \alpha \Delta T
Areal / volume expansionβ=2α, γ=3α\beta = 2\alpha,\ \gamma = 3\alpha
Thermal stress (clamped)σ=YαΔT\sigma = Y \alpha \Delta T
CalorimetryQ=mcΔT, Q=mLQ = mc\Delta T,\ Q=mL
Fourier conductionH=kA(T1T2)/LH = kA(T_1-T_2)/L
Thermal resistanceR=L/(kA)R = L/(kA)
Newton's coolingdT/dt=k(TTs)dT/dt = -k(T-T_s)
Stefan-BoltzmannPnet=eσA(T4Ts4)P_{\text{net}} = e\sigma A(T^4 - T_s^4)
WienλmaxT=2.898×103m⋅K\lambda_{\max}T = 2.898\times 10^{-3}\,\text{m·K}
Kinetic pressureP=13ρv2P = \tfrac{1}{3}\rho \overline{v^2}
Energy per molecule12mv2=32kBT\tfrac{1}{2}m\overline{v^2}=\tfrac{3}{2}k_BT
RMS speedvrms=3RT/Mv_{rms} = \sqrt{3RT/M}
Average speedvˉ=8RT/(πM)\bar v = \sqrt{8RT/(\pi M)}
Most-probable speedvmp=2RT/Mv_{mp} = \sqrt{2RT/M}
Degrees of freedomCv=(f/2)R, Cp=Cv+R, γ=1+2/fC_v = (f/2)R,\ C_p = C_v + R,\ \gamma = 1+2/f
Mean free pathλ=1/(2nπd2)\lambda = 1/(\sqrt{2}\, n\pi d^2)
First lawQ=ΔU+WQ = \Delta U + W
Isothermal workW=nRTln(V2/V1)W = nRT\ln(V_2/V_1)
Adiabatic relationPVγ=PV^\gamma = const,\ TVγ1=TV^{\gamma-1}= const
Adiabatic workW=(P1V1P2V2)/(γ1)W = (P_1V_1 - P_2V_2)/(\gamma - 1)
Polytropic (PVnPV^n=c)W=(P1V1P2V2)/(n1), C=CvR/(n1)W = (P_1V_1-P_2V_2)/(n-1),\ C = C_v - R/(n-1)
Engine efficiencyη=1Qc/Qh\eta = 1 - Q_c/Q_h
Carnot boundηC=1Tc/Th\eta_C = 1 - T_c/T_h
Refrigerator COPCOP=Qc/W=Tc/(ThTc)\text{COP} = Q_c/W = T_c/(T_h - T_c) (Carnot)
Heat pump COPCOPHP=Th/(ThTc)\text{COP}_{\text{HP}} = T_h/(T_h-T_c) (Carnot)
Entropy (reversible)ΔS=dQ/T\Delta S = \int dQ/T
Ideal-gas ΔS\Delta SnCvln(T2/T1)+nRln(V2/V1)nC_v \ln(T_2/T_1)+ nR\ln(V_2/V_1)

Sub-topics

6 pages

Practice quiz

Quiz
Unit 7: Thermal Physics & Thermodynamics — JEE Quiz
15 questions · pick the best answer
Q1

A steel rod of length 1 m and cross-section 1 cm² is clamped between two rigid supports at 20 °C. The thermal force on the supports when heated to 120 °C is (Y = 2×10¹¹ Pa, α = 1.2×10⁻⁵ K⁻¹):

Q2

A circular hole of radius 1.000 cm is drilled in a brass plate at 27 °C. Its radius at 127 °C is (αbrass=2_brass = 2×10⁻⁵ /K):

Q3

10 g of ice at 0 °C is added to 30 g of water at 50 °C in an insulated calorimeter. Final temperature?

Q4

Two rods of equal length and area but conductivities k and 3k are joined end to end. Hot end at 100 °C, cold end at 0 °C. The junction temperature is:

Q5

A body at 327 °C is placed in surroundings at 27 °C and radiates 80 W. Its rate of radiation when heated to 727 °C is approximately:

Q6

A liquid cools from 80 °C to 60 °C in 5 min in surroundings at 20 °C. Time taken to cool from 60 °C to 40 °C (use Newton's law of cooling, mean-temperature form):

Q7

The temperature at which rms speed of O₂ equals rms speed of N₂ at 300 K is:

Q8

Mixture of 1 mole He (γ=5/3) and 2 moles O₂ (γ=7/5). The effective γ of the mixture is:

Q9

1 mole monatomic gas at 300 K, 1 atm is compressed adiabatically to V/8. Final temperature is:

Q10

1 mole ideal gas at 300 K, 1 atm expands isothermally to triple its volume. Heat absorbed (R = 8.314 J/mol·K):

Q11

A Carnot engine takes 1000 J at 500 K and rejects heat at 300 K. Work output is:

Q12

A refrigerator with COP 5 dumps 6 kJ per cycle to the room. The work done per cycle is:

Q13

A monatomic gas undergoes the process T = T₀ + αV² (α positive). Its molar heat capacity is:

Q14

An ideal monatomic gas is taken through a cycle ABCA: A→B isobaric expansion at P=2P₀ from V₀ to 2V₀; B→C isochoric drop to P₀; C→A isothermal compression. Net work done over one cycle:

Q15

Two identical rods, one of thermal conductivity 2k and the other k, are joined in series. The equivalent thermal conductivity is: