Rate of cooling of a body is proportional to the temperature difference between body and surroundings: dT/dt = -k(T - T_surroundings). Holds for small temperature differences.
-- NCERT, p. 10Heat Transfer
Lesson
Heat moves from a hotter body to a cooler one through three mechanisms — conduction, convection, and radiation. NEET questions on this topic test whether you can distinguish the mechanism, recall the governing law, and apply the Stefan-Boltzmann formula for radiation problems.
Conduction is heat transfer through a medium without bulk motion of matter. Metals are good conductors; wood, air, and rubber are poor conductors (insulators). The rate of heat flow through a uniform rod depends on thermal conductivity, cross-sectional area, temperature difference, and length. NCERT Class 11 Physics Chapter 10 (page 10) states the law governing steady-state conduction.
Convection is heat transfer by actual movement of fluid. Natural convection arises from density differences (hot fluid rises); forced convection uses an external agent like a fan or pump. Sea breezes and land breezes are standard NCERT examples. Convection cannot occur in solids.
Radiation is heat transfer through electromagnetic waves — no medium required. Every body above 0 K radiates. The Stefan-Boltzmann law gives the total power radiated: P = σεAT⁴, where σ = 5.67 × 10⁻⁸ W m⁻² K⁻⁴, ε is emissivity (1 for a black body), A is surface area, and T is absolute temperature in kelvin (NCERT Class 11 Physics Chapter 10, page 13). The net power radiated to surroundings at temperature T₀ is P_net = σεA(T⁴ − T₀⁴).
Watch-out: A common confusion is computing radiation power using Celsius instead of kelvin — the T⁴ dependence amplifies even a small offset. Always convert to kelvin first. Also note that emissivity ε = 1 for an ideal black body; real surfaces have ε < 1, and a good absorber is also a good emitter (Kirchhoff's law, NCERT Class 11 Physics Chapter 10, page 11).
Practice MCQs
Select an option to see the explanation. Wrong answers show why your choice was tempting — and name the exact trap it exploits.
Which mode of heat transfer does NOT require a material medium?
According to Kirchhoff's law of thermal radiation, at thermal equilibrium a good absorber of radiation is also a:
In which of the following is heat transferred primarily by convection?
A black body at temperature T radiates power P. If its absolute temperature is doubled to 2T, the radiated power becomes:
Two identical black bodies are at temperatures 300 K and 600 K. The ratio of the net rate of energy radiated by the hotter body to that of the cooler body is:
A body with surface area 0.10 m² and emissivity 0.60 is at 500 K. Taking σ = 5.67 × 10⁻⁸ W m⁻² K⁻⁴, the power radiated by this body is closest to:
A thermos flask reduces heat loss by minimising all three modes of transfer. The silvered inner walls primarily reduce heat loss by:
A solid sphere of radius R at temperature T is surrounded by an environment at temperature T₀. If the sphere's radius is halved (to R/2) while its temperature and emissivity remain unchanged, by what factor does the net rate of radiative heat loss change?
Quick recall before you leave
Worked Example
- 1
Given
A furnace wall (treated as a black body, ε = 1) has a small observation hole of area A = 4.0 × 10⁻⁴ m². The furnace interior is at T = 1.50 × 10³ K. The surrounding temperature is T₀ = 300 K. σ = 5.67 × 10⁻⁸ W m⁻² K⁻⁴.
- 2
Required
Find the net rate of radiative heat loss through the hole.
- 3
Concept
The hole acts as a black-body radiator (Kirchhoff's law — a small hole in a large cavity is an ideal black body). The net power radiated to the surroundings follows from the Stefan-Boltzmann law.
- 4
Formula
P_net = σεA(T⁴ − T₀⁴)
- 5
Substitution
P_net = (5.67 × 10⁻⁸)(1)(4.0 × 10⁻⁴)[(1.50 × 10³)⁴ − (300)⁴]
- 6
Calculation
T⁴ = (1.50 × 10³)⁴ = (1.50)⁴ × 10¹² = 5.0625 × 10¹² K⁴ T₀⁴ = (300)⁴ = (3.00)⁴ × 10⁸ = 81.00 × 10⁸ = 8.100 × 10⁹ K⁴ T⁴ − T₀⁴ = 5.0625 × 10¹² − 0.0081 × 10¹² = 5.0544 × 10¹² K⁴ σ × ε × A = 5.67 × 10⁻⁸ × 1 × 4.0 × 10⁻⁴ = 2.268 × 10⁻¹¹ W K⁻⁴ P_net = 2.268 × 10⁻¹¹ × 5.0544 × 10¹² = 2.268 × 5.0544 × 10¹ = 114.6 × 10¹ ≈ 115 W Note on exact quantities: ε = 1 (ideal black body, exact by definition) and the integer 4 in 4πR² or the exponent 4 in T⁴ are mathematical constants — they do not limit significant figures. The answer is reported to 3 significant figures, governed by the given area (4.0 × 10⁻⁴ has 2 sig figs) and temperature (1.50 × 10³ has 3 sig figs), so 2 sig figs controls: P_net ≈ 1.1 × 10² W.
- 7
Final answer
P_net ≈ 1.1 × 10² W (two significant figures, governed by the area measurement 4.0 × 10⁻⁴ m²).
- 8
Common trap
Using Celsius instead of kelvin: if you mistakenly use 1500 °C as T without converting, the answer balloons because (1773)⁴ ≫ (1500)⁴. Always confirm T is in kelvin before raising to the fourth power.
- 9
Similar NEET-style question
A spherical black body of radius 0.10 m is at 800 K in surroundings at 300 K. Find the net rate of radiative heat loss. (Hint: compute A = 4πr², then apply P_net = σA(T⁴ − T₀⁴).) ---
Before solving, remember these
Modes of heat transfer
Conduction: through direct contact (Fourier's law: dQ/dt = -k A dT/dx). Convection: bulk motion of fluid (natural or forced). Radiation: electromagnetic waves; no medium needed; Stefan-Boltzmann: P = σ ε A T⁴.
-- NCERT, p. 11Stefan-Boltzmann law
Power radiated by a black body: P = σ A T⁴, where σ = 5.67 × 10⁻⁸ W/m²/K⁴. For grey body: P = ε σ A T⁴ with emissivity ε ≤ 1. Net power emitted to surroundings at T_s: P = ε σ A (T⁴ - T_s⁴).
-- NCERT, p. 13Formulas
12 formulas — click to collapse
Bernoulli's equation
Conservation of energy along a streamline of incompressible non-viscous flow.
| Symbol | Quantity | SI Unit |
|---|---|---|
| P | pressure | Pa |
| rho | density | kg/m^3 |
| v | speed | m/s |
| g | gravity | m/s^2 |
| h | height | m |
Valid when
- Steady, non-viscous, incompressible flow
- Along a single streamline
- No work added/removed
Bulk modulus
Resistance of a material to uniform compression. Inverse: compressibility.
| Symbol | Quantity | SI Unit |
|---|---|---|
| K | bulk modulus | Pa |
| V | volume | m^3 |
| P | pressure | Pa |
Valid when
- Isotropic compression
- Within elastic regime
Capillary rise/depression
Height a liquid rises (or falls) in a capillary tube. cos(theta) > 0: rises (wetting); < 0: depresses.
| Symbol | Quantity | SI Unit |
|---|---|---|
| h | capillary height | m |
| T | surface tension | N/m |
| theta | contact angle | rad |
| rho | density | kg/m^3 |
| r | tube radius | m |
Valid when
- Narrow tube (capillary regime)
- Constant theta
Pressure in static fluid
Pressure at depth h below free surface of fluid of density rho.
| Symbol | Quantity | SI Unit |
|---|---|---|
| P | total pressure | Pa |
| P0 | atmospheric/surface pressure | Pa |
| rho | density | kg/m^3 |
| h | depth | m |
Valid when
- Static fluid (no flow)
- Constant g
- Constant rho (incompressible)
Latent heat
Heat absorbed/released during phase change at constant T. L_fusion or L_vaporisation.
| Symbol | Quantity | SI Unit |
|---|---|---|
| Q | heat | J |
| m | mass | kg |
| L | latent heat | J/kg |
Valid when
- Phase transition (constant T during)
- All mass m undergoes the transition
Specific heat / heat capacity
Heat required to raise mass m by temperature Delta_T. Specific heat c is material property.
| Symbol | Quantity | SI Unit |
|---|---|---|
| Q | heat | J |
| m | mass | kg |
| c | specific heat | J/kg/K |
| Delta_T | temp change | K |
Valid when
- No phase change during heating
- c approximately constant in temp range
Stefan-Boltzmann radiation law
Radiation power from a body. Black body epsilon=1; net to surroundings P = sigma*epsilon*A*(T^4 - T_s^4).
| Symbol | Quantity | SI Unit |
|---|---|---|
| sigma | Stefan-Boltzmann = 5.67e-8 | W/m^2/K^4 |
| epsilon | emissivity (0-1) | - |
| A | surface area | m^2 |
| T | absolute temp | K |
Valid when
- Body in radiative equilibrium
- T in kelvins
Stokes' law (viscous drag on sphere)
Drag force on a sphere of radius r moving with velocity v through viscous fluid (low Reynolds number).
| Symbol | Quantity | SI Unit |
|---|---|---|
| F | drag force | N |
| eta | viscosity | Pa*s |
| r | sphere radius | m |
| v | velocity | m/s |
Valid when
- Smooth, slow flow (low Reynolds number)
- Spherical body
- Newtonian fluid
Excess pressure inside drop/bubble
Excess internal pressure due to surface tension. Bubble has 2 surfaces, hence factor 4.
| Symbol | Quantity | SI Unit |
|---|---|---|
| Delta_P | excess pressure | Pa |
| T | surface tension | N/m |
| r | radius | m |
Valid when
- Spherical drop or bubble
- Constant T (one fluid pair)
Terminal velocity of sphere in viscous fluid
Constant velocity reached when net force is zero (gravity balanced by buoyancy + viscous drag).
| Symbol | Quantity | SI Unit |
|---|---|---|
| v_t | terminal velocity | m/s |
| r | sphere radius | m |
| rho_s | sphere density | kg/m^3 |
| rho_f | fluid density | kg/m^3 |
| eta | viscosity | Pa*s |
Valid when
- Steady state (net force zero)
- Stokes regime applicable
Thermal expansion (linear/area/volume)
Fractional change in length, area, volume per degree temperature change.
| Symbol | Quantity | SI Unit |
|---|---|---|
| alpha | linear coefficient | 1/K |
| beta | volume coefficient | 1/K |
| Delta_T | temperature change | K |
Valid when
- Isotropic material
- Modest temperature range (alpha ~ constant)
Young's modulus
Ratio of longitudinal stress to longitudinal strain in a stretched wire/rod within elastic limit.
| Symbol | Quantity | SI Unit |
|---|---|---|
| Y | Young's modulus | Pa |
| F | applied force | N |
| A | cross-section area | m^2 |
| L | original length | m |
| Delta_L | extension | m |
Valid when
- Within elastic limit (Hooke's law region)
- Uniform cross-section
- Force along length
Exam Traps & Common Mistakes
These are the exact patterns that cause wrong answers in NEET. Each trap includes when it triggers and how to avoid it.
5 items — click to collapse
Category: Similar Terms
Student uses 2T/r for soap bubble (drop formula). Bubble has 2 surfaces → 4T/r.
When it triggers
Question mentions soap bubble OR liquid drop OR air bubble in liquid.
How to avoid
Drop in air: 1 surface → 2T/r. Soap bubble in air: 2 surfaces → 4T/r. Air bubble in liquid: 1 surface → 2T/r.
Category: Similar Terms
Student uses Y formula when problem is about volumetric compression (use K) or vice versa.
When it triggers
Problem describes longitudinal stretching (use Y), volumetric pressure (use K), or shear (use G).
How to avoid
Y: longitudinal stress/strain. K: volumetric. G: shear. Match modulus to deformation type.
Root cause: concept gap
Correction
Drop in air: 1 surface → ΔP = 2T/r. Soap bubble: 2 surfaces (inner + outer) → ΔP = 4T/r. Air bubble inside liquid: 1 surface → 2T/r.
Root cause: formula misuse
Correction
v_t ∝ r² (because Stokes drag ∝ r v, gravity ∝ r³ - r³ = r³_diff). Doubling radius quadruples terminal velocity, not doubles.
Root cause: formula misuse
Correction
Y for longitudinal stretch (FL/A·ΔL); K for volumetric compression (-V·dP/dV); G for shear. Match modulus type to deformation type before computing.
Past Year Questions
15 questions from NEET 2020, 2021, 2022, 2023, 2024, 2025. Answers verified against NTA official keys. — click to collapse
If a soap bubble expands, the pressure inside the bubble
How NEET usually asks this
5 recurring patterns from past papers — click to collapse
Apply Bernoulli's equation to flow through pipes of varying cross-section / heights / Venturi-like geometries.
Common distractors
forgets height term
Drops rho*g*h term
equates pressures incorrectly
Picks wrong reference points
Two bodies of given material and dimensions; find ratio of heat needed for same temp change. Q ∝ m c.
Common distractors
ignores mass difference
Compares only specific heats, not masses
Energy to form a bubble of given radius from soap solution; or pressure inside vs outside. Bubble has 2 surfaces (factor 4T/r).
Common distractors
uses 2T r instead of 4T r for bubble
Treats soap bubble like a drop
Sphere falling in viscous liquid; find terminal velocity or shape of v(t) curve. v_t ∝ r^2.
Common distractors
expects linear acceleration
Default to constant acceleration without recognising drag-induced terminal v
Wire stretching: given Y, length, area, force or stress, find elongation or stress at limit. Y = FL/(A delta_L).
Common distractors
uses bulk modulus formula
Confuses Y with K
Sources
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