Thermal Properties of Matter

NEET Ug . NEET Physics . Physics . Thermal Properties of Matter

Chapter 11: Thermal Properties of Matter

Ch 11

NEET Physics

NEET Ug

Introduction

Thermal Properties of Matter

  • Temperature measures hotness or coldness of a body.
  • During phase changes (e.g., boiling, freezing), temperature remains constant despite heat flow.
  • Heat is energy transfer due to temperature difference.
  • Thermal properties explain phenomena like why ice feels cold.

Solved Examples

  • Ex 1: Why does temperature remain constant during boiling?
    • Heat energy is used for phase change, not temperature rise.

Practice Set

  • Q1: What does temperature measure?
    • A) Energy content B) Hotness or coldness C) Heat flow D) Mass
  • Q2: During freezing, temperature of water
    • A) Increases B) Decreases C) Remains constant D) Fluctuates
  • Q3: Ice feels cold because
    • A) It has low temperature B) It absorbs heat from hand C) It emits heat D) It has high heat content

Answer Key

  • Q1: B - Temperature indicates hotness or coldness.
  • Q2: C - Temperature remains constant during phase change.
  • Q3: B - Ice absorbs heat from hand, causing cold sensation.

Memory Aids

  • Phase change = constant temperature despite heat flow.
  • Temperature = measure of hotness/coldness, not energy.
  • Heat = energy transfer due to temperature difference.

Temperature and Heat

Key Concepts

  • Temperature: Relative measure of hotness or coldness.
  • Heat: Energy transferred due to temperature difference.
  • Heating effects: temperature rise, expansion, or state change.
  • Units: Temperature (Kelvin, °C), Heat (Joule, J).

Solved Examples

  • Ex 1: Define heat.
    • Heat is energy transfer between systems due to temperature difference.
  • Ex 2: What happens when an object is heated?
    • Temperature may rise, object may expand or change state.

Practice Set

  • Q1: Heat is transferred because of
    • A) Pressure difference B) Temperature difference C) Volume difference D) Mass difference
  • Q2: Which is a relative measure?
    • A) Heat B) Temperature C) Energy D) Work
  • Q3: When an object is heated, which may NOT occur?
    • A) Temperature rise B) Expansion C) Change of state D) Decrease in temperature

Answer Key

  • Q1: B - Heat flows due to temperature difference.
  • Q2: B - Temperature is a relative measure of hotness/coldness.
  • Q3: D - Heating does not cause temperature decrease.

Memory Aids

  • Heat = energy transfer due to \(\Delta T\).
  • Temperature = relative hotness, not absolute energy.
  • Heating effects: rise in temperature, expansion, or phase change.

Measurement of Temperature

Thermometer and Temperature Measurement

  • A thermometer measures temperature using physical properties that vary with temperature.
  • Commonly, volume change of liquids like mercury or alcohol is used due to linear variation with temperature.
  • Glass thermometers contain such liquids to indicate temperature changes.

Temperature Scales and Fixed Points

  • Two fixed reference points define temperature scales: ice point (freezing) and steam point (boiling) of water.
  • Ice point: 0°C (Celsius), 32°F (Fahrenheit).
  • Steam point: 100°C (Celsius), 212°F (Fahrenheit).
  • Common scales: Celsius and Fahrenheit.

Relation Between Celsius and Fahrenheit

  • Linear relation: \( \frac{t_F - 32}{180} = \frac{t_C}{100} \)
  • Or equivalently: \( t_F = \frac{9}{5} t_C + 32 \)
Diagram 1 – NEET Physics Thermal Properties of Matter

Solved Examples

Ex 1

  • Convert 25°C to Fahrenheit.
  • Use formula: \( t_F = \frac{9}{5} \times 25 + 32 = 45 + 32 = 77^{\circ}F \)

Ex 2

  • Convert 95°F to Celsius.
  • Use formula: \( t_C = \frac{5}{9} (95 - 32) = \frac{5}{9} \times 63 = 35^{\circ}C \)

Practice Set

Q1

What is the boiling point of water in Fahrenheit?

  • A) 100°F
  • B) 212°F
  • C) 180°F
  • D) 32°F

Q2

Convert 0°C to Fahrenheit.

  • A) 0°F
  • B) 32°F
  • C) 100°F
  • D) 212°F

Q3

If temperature is 68°F, what is it in Celsius?

  • A) 20°C
  • B) 25°C
  • C) 30°C
  • D) 15°C

Answer Key

  • Q1: B) 212°F — Boiling point of water is 212°F on Fahrenheit scale.
  • Q2: B) 32°F — Freezing point of water is 0°C = 32°F.
  • Q3: A) 20°C — Using \( t_C = \frac{5}{9} (68 - 32) = 20^{\circ}C \).

Memory Aids

  • Use \( t_F = \frac{9}{5} t_C + 32 \) to convert Celsius to Fahrenheit.
  • Use \( t_C = \frac{5}{9} (t_F - 32) \) to convert Fahrenheit to Celsius.
  • Remember fixed points: 0°C = 32°F (freezing), 100°C = 212°F (boiling).

Ideal Gas Equation and Absolute Temperature

Gas Behaviour and Temperature Scales

  • All gases at low density show similar expansion behaviour.
  • Variables: Pressure (P), Volume (V), Temperature (T).
  • Temperature in Kelvin: \( T = t + 273.15 \), where \( t \) is in °C.
  • Boyle's Law (at constant T): \( PV = \text{constant} \).
  • Charles' Law (at constant P): \( \frac{V}{T} = \text{constant} \).
  • Pressure vs Temperature at constant volume is linear; extrapolates to zero pressure at -273.15°C (absolute zero).
  • Absolute zero is the lowest possible temperature; basis of Kelvin scale (0 K = -273.15°C).
  • Ideal Gas Equation: \( PV = \mu RT \), where \( \mu \) = moles, \( R = 8.31\,\mathrm{J\,mol^{-1}K^{-1}} \).
Diagram 2 – NEET Physics Thermal Properties of Matter

Pressure-Temperature Relation for Gases

  • Pressure increases linearly with temperature at constant volume.
  • Extrapolation of pressure lines for different gases meet at absolute zero (-273.15°C).
  • Graph shows pressure vs temperature for gases A, B, C starting near 0 K.
  • Pressure is nearly zero at absolute zero; increases with temperature.
Diagram 3 – NEET Physics Thermal Properties of Matter

Temperature Scales and Conversion

  • Kelvin scale starts at absolute zero (0 K = -273.15°C).
  • Celsius scale: 0°C (freezing), 100°C (boiling) of water.
  • Fahrenheit scale: 32°F (freezing), 212°F (boiling) of water.
  • Unit size same for Kelvin and Celsius scales.
  • Conversion formula: \( T = t_C + 273.15 \).
  • General relation for any scale: \[ \frac{\text{Reading} - \text{Lower fixed point}}{\text{Upper fixed point} - \text{Lower fixed point}} = \text{constant} \]
  • Example: \[ \frac{t_C - 0}{100} = \frac{t_F - 32}{180} = \frac{t_R - 0}{80} = \frac{t_K - 273.15}{100} \]
Diagram 4 – NEET Physics Thermal Properties of Matter

Solved Examples

Ex 1

  • Given: \( P = 2\,\mathrm{atm} \), \( V = 5\,\mathrm{L} \), \( T = 300\,\mathrm{K} \), find \( n \) using \( PV = nRT \).
  • Use \( R = 0.0821\,\mathrm{L\,atm\,mol^{-1}K^{-1}} \).
  • Calculation: \( n = \frac{PV}{RT} = \frac{2 \times 5}{0.0821 \times 300} \approx 0.406\,\mathrm{mol} \).

Ex 2

  • Convert 25°C to Kelvin.
  • Calculation: \( T = 25 + 273.15 = 298.15\,\mathrm{K} \).

Practice Set

Q1

  • At constant temperature, if volume of a gas is halved, pressure will be:
    • A) Halved
    • B) Doubled
    • C) Unchanged
    • D) Quartered

Q2

  • What is the temperature in Celsius corresponding to 0 K?
    • A) -273.15°C
    • B) 0°C
    • C) 273.15°C
    • D) -100°C

Q3

  • A gas occupies 4 L at 27°C and 1 atm. What volume will it occupy at 127°C and 1 atm?
    • A) 5 L
    • B) 6 L
    • C) 7 L
    • D) 8 L

Answer Key

  • Q1: B) Doubled — Boyle's law: \( PV = \text{constant} \), halving volume doubles pressure.
  • Q2: A) -273.15°C — 0 K equals absolute zero in Celsius.
  • Q3: D) 8 L — Using Charles' law: \( \frac{V_1}{T_1} = \frac{V_2}{T_2} \), convert temperatures to K and solve.

Memory Aids

  • Boyle's Law: \( P \propto \frac{1}{V} \) at constant T.
  • Charles' Law: \( V \propto T \) at constant P.
  • Ideal Gas Equation: \( PV = nRT \).
  • Kelvin = Celsius + 273.15.
  • Absolute zero = -273.15°C = 0 K.

Thermal Expansion

Concepts

  • Thermal expansion: Increase in dimensions due to temperature rise.
  • Occurs in solids (length, area, volume), liquids and gases (volume only).
  • Gas state depends on volume, pressure, temperature; expansion can be at constant volume or pressure.
  • Different substances and states have different expansion properties.
Diagram 5 – NEET Physics Thermal Properties of Matter

Solved Examples

  • Ex 1: Calculate length after heating: Use \( L_T = L_0 (1 + \alpha \Delta T) \).
  • Ex 2: Find volume increase: Use \( V_T = V_0 (1 + \gamma \Delta T) \).

Practice Set

  • Q1: Thermal expansion occurs in which states? A) Solids only B) Liquids only C) Gases only D) All states
  • Q2: Which expansion is possible only in solids? A) Linear B) Volume C) Area D) Both A and C
  • Q3: If a gas is heated at constant volume, which property changes? A) Pressure B) Volume C) Temperature D) Mass

Answer Key

  • Q1: D; All states expand on heating.
  • Q2: D; Solids show linear and area expansion.
  • Q3: A; Pressure changes at constant volume.

Memory Aids

  • Thermal expansion = size increase with temperature.
  • Solids: length, area, volume expand; Liquids/gases: volume only.
  • Gas expansion depends on pressure/volume constraints.

Thermal Expansion in Solids

Types

  • Linear expansion: Increase in length \( \Delta l \).
  • Area expansion: Increase in surface area \( \Delta A \).
  • Volume expansion: Increase in volume \( \Delta V \).
Diagram 6 – NEET Physics Thermal Properties of Matter

Solved Examples

  • Ex 1: Calculate new length: \( L_T = L_0 (1 + \alpha \Delta T) \).
  • Ex 2: Calculate new area: \( A_T = A_0 (1 + \beta \Delta T) \).
  • Ex 3: Calculate new volume: \( V_T = V_0 (1 + \gamma \Delta T) \).

Practice Set

  • Q1: Coefficient of linear expansion is increase in length per unit length per degree. True or False? A) True B) False C) Sometimes D) None
  • Q2: Relation between coefficients: \( \alpha = \frac{\beta}{2} = \frac{\gamma}{3} \). What is \( \beta \) if \( \alpha = 2 \times 10^{-5} \)? A) \(4 \times 10^{-5}\) B) \(1 \times 10^{-5}\) C) \(6 \times 10^{-5}\) D) \(2 \times 10^{-5}\)
  • Q3: Volume expansion coefficient \( \gamma \) unit is? A) m B) \( ^\circ C^{-1} \) C) m/s D) kg

Answer Key

  • Q1: A; Definition of linear expansion coefficient.
  • Q2: A; \( \beta = 2\alpha = 4 \times 10^{-5} \).
  • Q3: B; Units are per degree Celsius or Kelvin.

Memory Aids

  • \( \alpha \) for length, \( \beta = 2\alpha \) for area, \( \gamma = 3\alpha \) for volume.
  • Units: inverse temperature (\( ^\circ C^{-1} \) or K⁻¹).
  • Volume expansion > area expansion > linear expansion.

Anomalous Expansion of Water

Key Points

  • Water expands on heating above 4°C.
  • Between 0°C and 4°C, water contracts on heating (negative volume expansion).
  • Maximum density at 4°C.
  • Explains ice floating and freezing from top.
Diagram 7 – NEET Physics Thermal Properties of Matter

Solved Examples

  • Ex 1: Explain why ice floats using density variation with temperature.
  • Ex 2: Describe volume change of water from 0°C to 10°C.

Practice Set

  • Q1: Water has maximum density at? A) 0°C B) 4°C C) 10°C D) 100°C
  • Q2: Between 0°C and 4°C, water volume? A) Increases B) Decreases C) Constant D) None
  • Q3: Anomalous expansion means? A) Normal expansion B) Negative expansion C) No expansion D) Random expansion

Answer Key

  • Q1: B; Maximum density at 4°C.
  • Q2: B; Volume decreases on heating from 0°C to 4°C.
  • Q3: B; Negative volume expansion in 0–4°C range.

Memory Aids

  • Water densest at 4°C.
  • Volume decreases 0–4°C, increases above 4°C.
  • Ice floats due to lower density than water.

Coefficient of Volume Expansion for Ideal Gas

Concepts

  • Ideal gas law: \( PV = \mu RT \).
  • At constant pressure: \( P \Delta V = \mu R \Delta T \).
  • Volume change: \( \frac{\Delta V}{V} = \frac{\Delta T}{T} \).
  • Coefficient of volume expansion \( \gamma \propto \frac{1}{T} \).

Solved Examples

  • Ex 1: Calculate volume change for ideal gas heated from 300 K to 330 K at constant pressure.

Practice Set

  • Q1: For ideal gas, volume expansion coefficient \( \gamma \) is proportional to? A) T B) 1/T C) P D) V
  • Q2: If temperature doubles, volume change ratio is? A) 1 B) 2 C) 0.5 D) 0
  • Q3: At constant pressure, volume change \( \Delta V \) is proportional to? A) \( \Delta T \) B) \( \Delta P \) C) \( \Delta V \) D) None

Answer Key

  • Q1: B; \( \gamma \propto 1/T \).
  • Q2: B; Volume doubles if temperature doubles.
  • Q3: A; Volume change proportional to temperature change.

Memory Aids

  • Ideal gas volume expansion ~ temperature increase.
  • \( \gamma = \frac{1}{T} \) approx. for ideal gases.

Thermal Stress

Concepts

  • Thermal stress arises when expansion is prevented.
  • Thermal strain: \( \frac{\Delta L}{L} = \alpha \Delta T \).
  • Thermal stress: \( \sigma = Y \alpha \Delta T \) (Y = Young's modulus).
  • Force developed: \( F = Y A \alpha \Delta T \) (A = cross-sectional area).

Solved Examples

  • Ex 1: Calculate thermal stress if rod fixed at ends heated by \( \Delta T \).
  • Ex 2: Find force developed in rod with given area and Young's modulus.

Practice Set

  • Q1: Thermal stress occurs when expansion is? A) Allowed B) Prevented C) Ignored D) None
  • Q2: Thermal strain formula is? A) \( \alpha \Delta T \) B) \( Y \alpha \Delta T \) C) \( \frac{\Delta L}{L} \) D) Both A and C
  • Q3: Force due to thermal stress is? A) \( Y A \alpha \Delta T \) B) \( \alpha \Delta T \) C) \( Y \alpha \) D) \( A \Delta T \)

Answer Key

  • Q1: B; Stress arises if expansion is prevented.
  • Q2: D; Thermal strain = \( \frac{\Delta L}{L} = \alpha \Delta T \).
  • Q3: A; Force = Young's modulus × area × expansion.

Memory Aids

  • Stress = Young's modulus × strain.
  • Strain from thermal expansion = \( \alpha \Delta T \).
  • Force depends on cross-sectional area.

Density and Temperature

Concepts

  • Volume increases with temperature; mass constant ⇒ density decreases.
  • Density change: \( \rho' = \frac{\rho}{1 + \gamma \Delta \theta} \approx \rho (1 - \gamma \Delta \theta) \) if \( \gamma \Delta \theta << 1 \).
  • For floating solid: immersed fraction \( f = \frac{\rho_s}{\rho_l} \).
  • With temperature increase: \( f' = f \frac{1 + \gamma_l \Delta \theta}{1 + \gamma_s \Delta \theta} \).
  • If \( \gamma_l > \gamma_s \), immersed fraction increases.
  • Length of pendulum increases with temperature, increasing time period.
  • Time period change: \( T' = T (1 + \alpha \Delta \theta)^{1/2} \approx T (1 + \frac{1}{2} \alpha \Delta \theta) \).
  • Time lost in interval \( t \): \( \Delta t = \frac{\Delta T}{T} \times t \).

Solved Examples

  • Ex 1: Calculate density change for given \( \gamma \) and temperature rise.
  • Ex 2: Find time lost by pendulum clock heated by \( \Delta \theta \).

Practice Set

  • Q1: Density decreases with temperature because? A) Mass decreases B) Volume increases C) Both D) None
  • Q2: Immersed fraction increases if? A) \( \gamma_l > \gamma_s \) B) \( \gamma_s > \gamma_l \) C) Equal D) None
  • Q3: Time period of pendulum increases with temperature by? A) \( \alpha \Delta \theta \) B) \( \frac{1}{2} \alpha \Delta \theta \) C) \( 2 \alpha \Delta \theta \) D) None

Answer Key

  • Q1: B; Volume increase lowers density.
  • Q2: A; Liquid expands more, increasing immersed fraction.
  • Q3: B; Time period increases approx. by half the linear expansion factor.

Memory Aids

  • Density inversely proportional to volume.
  • Immersed fraction depends on relative expansion coefficients.
  • Pendulum time period increases with length expansion.

Specific Heat Capacity

Definition and Formula

  • Heat capacity (S) = \( \frac{\Delta Q}{\Delta T} = ms \)
  • \( \Delta Q \): heat supplied to change temperature from \( T \) to \( T + \Delta T \)
  • \( m \): mass of the substance (kg)
  • \( s \): specific heat capacity (J/kg·K)

Specific Heat Capacity

  • Amount of heat per unit mass to raise temperature by 1 K
  • Formula: \( s = \frac{1}{m} \frac{\Delta Q}{\Delta T} = \frac{S}{m} \)
  • Depends on substance nature and temperature

Molar Specific Heat Capacity

  • Heat capacity per mole of substance (in gram moles)
  • Formula: \( C = \frac{S}{\mu} = \frac{1}{\mu} \frac{\Delta Q}{\Delta T} \)
  • \( \mu \): number of moles
  • Two types:
    • At constant pressure: \( C_p \)
    • At constant volume: \( C_V \)

Solved Examples

  • Ex 1: Calculate heat capacity if \( \Delta Q = 500\,J \), \( \Delta T = 10\,K \), and mass \( m = 2\,kg \).
    • Heat capacity \( S = \frac{\Delta Q}{\Delta T} = \frac{500}{10} = 50\,J/K \)
    • Specific heat \( s = \frac{S}{m} = \frac{50}{2} = 25\,J/kg\cdot K \)
  • Ex 2: Find molar specific heat if \( S = 100\,J/K \) and \( \mu = 4\,mol \).
    • \( C = \frac{S}{\mu} = \frac{100}{4} = 25\,J/mol\cdot K \)

Practice Set

  • Q1: Heat capacity \( S \) is defined as:
    • A) \( \frac{\Delta T}{\Delta Q} \)
    • B) \( \frac{\Delta Q}{\Delta T} \)
    • C) \( m \times s \)
    • D) \( \frac{1}{m} \frac{\Delta Q}{\Delta T} \)
  • Q2: Specific heat capacity \( s \) depends on:
    • A) Mass only
    • B) Nature of substance and temperature
    • C) Volume only
    • D) Pressure only
  • Q3: Molar specific heat capacity at constant volume is denoted by:
    • A) \( C_p \)
    • B) \( C_V \)
    • C) \( s \)
    • D) \( S \)

Answer Key

  • Q1: B) \( \frac{\Delta Q}{\Delta T} \) is the definition of heat capacity.
  • Q2: B) It depends on the nature of substance and temperature.
  • Q3: B) \( C_V \) denotes molar specific heat at constant volume.

Memory Aids

  • Heat capacity \( S = ms \)
  • Specific heat \( s = \frac{S}{m} \)
  • Molar heat \( C = \frac{S}{\mu} \)
  • Remember: \( C_p > C_V \) for gases

Calorimetry

Concept and Principle

  • Calorimetry measures specific heat or latent heat of substances.
  • A calorimeter is the device used for heat measurement.
  • Heat lost by a hot body = Heat gained by a cold body (no heat loss to surroundings).
  • Based on the law of conservation of energy.
  • Formula: Heat Lost = Heat Gained

Solved Examples

  • Ex 1: A 100 g hot metal at 100°C is dropped into 200 g water at 20°C. Final temperature is 25°C. Find specific heat of metal.
    • Heat lost by metal = Heat gained by water
    • mmetalcmetal(Tinitial - Tfinal) = mwatercwater(Tfinal - Tinitial)
    • Calculate cmetal using known values.

Practice Set

  • Q1: What is the principle behind calorimetry?
    • A) Conservation of momentum
    • B) Conservation of energy
    • C) Newton's third law
    • D) Pascal's law
  • Q2: A 50 g metal at 150°C is placed in 100 g water at 25°C. Final temperature is 30°C. If specific heat of water is 4.2 J/g°C, what is the heat lost by metal?
    • A) 2100 J
    • B) 3150 J
    • C) 1050 J
    • D) 4200 J
  • Q3: In a calorimeter, 200 g of water at 20°C is mixed with 100 g of ice at 0°C. What is the final temperature? (Latent heat of fusion of ice = 336 J/g, specific heat of water = 4.2 J/g°C)
    • A) 0°C
    • B) 10°C
    • C) 15°C
    • D) 20°C

Answer Key

  • Q1: B) Conservation of energy — Calorimetry is based on heat lost equals heat gained.
  • Q2: C) 1050 J — Heat gained by water = m c ΔT = 100 × 4.2 × (30-25) = 2100 J; heat lost by metal equals heat gained, so 1050 J is half, check carefully: Actually, heat gained by water = 100 × 4.2 × 5 = 2100 J, so heat lost by metal = 2100 J (Option A). Correction: Option A is correct.
  • Q3: A) 0°C — Ice melts absorbing heat; water temperature drops to 0°C before any temperature rise.

Memory Aids

  • Heat lost = Heat gained (no heat loss to surroundings).
  • Calorimeter measures heat exchange.
  • Use m c ΔT for sensible heat; m L for latent heat.

Change of State

Key Concepts

  • Matter exists in three states: solid, liquid, gas.
  • Change of state: transition between these states.
  • Melting: solid to liquid.
  • Fusion: liquid to solid.
  • Melting point: temperature where solid and liquid coexist in equilibrium; depends on pressure; normal melting point at 1 atm.
  • Vaporisation: liquid to vapor.
  • Boiling point: temperature where liquid and vapor coexist; depends on pressure; normal boiling point at 1 atm.
  • Sublimation: solid to vapor without liquid phase.
  • Latent heat (L): heat required to change state of unit mass at constant temperature; formula: L = Q/m.
  • SI unit of latent heat: J/kg; practical unit: cal/g.
  • Latent heat of fusion: heat to convert solid to liquid; e.g., ice = 80 cal/g.
  • Latent heat of vaporisation: heat to convert liquid to vapor; e.g., water = 540 cal/g.
  • Triple point: temperature and pressure where solid, liquid, and vapor coexist; for water: 0.016C and 6.11d7 102 Pa.

Solved Examples

  • Ex 1: Calculate heat to melt 2 kg ice at 06C. Given latent heat of fusion = 3.33 d7 105 J/kg.
    • Q = mL = 2 d7 3.33 d7 105 = 6.66 d7 105 J
  • Ex 2: Heat required to vaporise 1.5 kg water at 1006C. Latent heat of vaporisation = 22.6 d7 105 J/kg.
    • Q = mL = 1.5 d7 22.6 d7 105 = 3.39 d7 106 J

Practice Set

  • Q1: What is the process of solid changing directly to vapor called?
    • A) Melting
    • B) Sublimation
    • C) Vaporisation
    • D) Fusion
  • Q2: The latent heat of fusion of ice is approximately:
    • A) 80 cal/g
    • B) 540 cal/g
    • C) 100 cal/g
    • D) 2260 cal/g
  • Q3: How much heat is required to convert 500 g of ice at 06C to water at 06C? (Latent heat of fusion = 3.33 d7 105 J/kg)
    • A) 1.665 d7 105 J
    • B) 6.66 d7 104 J
    • C) 3.33 d7 105 J
    • D) 8.33 d7 104 J

Answer Key

  • Q1: B) Sublimation - solid changes directly to vapor without liquid phase.
  • Q2: A) 80 cal/g - standard latent heat of fusion for ice.
  • Q3: A) 1.665 d7 105 J - Q = mL = 0.5 d7 3.33 d7 105.

Memory Aids

  • Melting = solid to liquid; Fusion = liquid to solid.
  • Latent heat formula: L = Q/m.
  • Ice fusion latent heat ~ 80 cal/g; water vaporisation ~ 540 cal/g.
  • Triple point water: 0.016C, 6.11 d7 102 Pa.
Diagram 8 – NEET Physics Thermal Properties of Matter

Heat Transfer

Modes of Heat Transfer

  • Heat transfer occurs due to temperature difference between systems.
  • Three modes: Conduction, Convection, Radiation.

Solved Examples

  • Ex 1: Heat flows from 1006C to 06C through a rod of area 0.01 m8 and thickness 0.5 m with thermal conductivity 200 W/mK. Calculate heat flow in 10 s.
    • Use \( Q = \frac{K A (T_1 - T_2) t}{d} \)
    • \( Q = \frac{200 \times 0.01 \times (100 - 0) \times 10}{0.5} = 4000 \) J

Practice Set

  • Q1: Heat transfer by conduction depends on
    • A) Temperature difference only
    • B) Area, temperature difference, time, and thickness
    • C) Thickness only
    • D) Time only
  • Q2: Which mode of heat transfer involves actual motion of particles?
    • A) Conduction
    • B) Convection
    • C) Radiation
    • D) None
  • Q3: Heat flow \( Q \) through a slab is directly proportional to
    • A) Thickness \( d \)
    • B) Cross-sectional area \( A \)
    • C) Time \( t \)
    • D) Both B and C

Answer Key

  • Q1: B - Heat conduction depends on area, temperature difference, time, and inversely on thickness.
  • Q2: B - Convection involves actual motion of heated particles.
  • Q3: D - Heat flow is directly proportional to area and time.

Memory Aids

  • Conduction: Heat flows through solids without particle movement.
  • Convection: Heat transfer by fluid motion.
  • Radiation: Heat transfer without medium.
  • Formula: \( Q = \frac{K A (T_1 - T_2) t}{d} \)
Diagram 9 – NEET Physics Thermal Properties of Matter

Convection

Key Points

  • Heat transfer by actual motion of heated particles in liquids and gases.
  • Causes natural phenomena: trade winds, monsoons, land and sea breezes.

Solved Examples

  • Ex 1: Identify the mode of heat transfer responsible for monsoons.
    • Answer: Convection

Practice Set

  • Q1: Heat transfer in fluids due to particle movement is called
    • A) Conduction
    • B) Convection
    • C) Radiation
    • D) Evaporation
  • Q2: Which of the following is an application of convection?
    • A) Heat conduction in metals
    • B) Formation of trade winds
    • C) Heat from the sun
    • D) Reflection of heat
  • Q3: Convection occurs in
    • A) Solids only
    • B) Liquids and gases
    • C) Vacuum
    • D) All states of matter

Answer Key

  • Q1: B - Convection involves heat transfer by fluid particle motion.
  • Q2: B - Trade winds form due to convection currents.
  • Q3: B - Convection occurs in liquids and gases.

Memory Aids

  • Convection = fluid motion heat transfer.
  • Think: Winds and ocean currents.

Radiation

Key Points

  • Heat transfer without heating the intervening medium.
  • Thermal radiation \( Q \) is partly absorbed (\( Q_a \)), reflected (\( Q_r \)), and transmitted (\( Q_t \)).
  • Relation: \( Q = Q_a + Q_r + Q_t \) and \( a + r + t = 1 \) where \( a, r, t \) are absorptance, reflectance, and transmittance.
  • Coefficients \( a, r, t \) are dimensionless ratios.

Solved Examples

  • Ex 1: If a body absorbs 70% of radiation and reflects 20%, find transmittance.
    • \( a + r + t = 1 \Rightarrow t = 1 - (a + r) = 1 - (0.7 + 0.2) = 0.1 \)

Practice Set

  • Q1: For a body, if absorptance \( a = 0.5 \) and reflectance \( r = 0.3 \), transmittance \( t \) is
    • A) 0.2
    • B) 0.8
    • C) 0.5
    • D) 0.3
  • Q2: A perfectly black body has
    • A) \( a = 1, r = 0, t = 0 \)
    • B) \( a = 0, r = 1, t = 0 \)
    • C) \( a = 0, r = 0, t = 1 \)
    • D) \( a = 0.5, r = 0.5, t = 0 \)
  • Q3: Which of the following is true for a good reflector?
    • A) High absorptance
    • B) High transmittance
    • C) Low absorptance
    • D) None

Answer Key

  • Q1: A - \( t = 1 - (0.5 + 0.3) = 0.2 \)
  • Q2: A - Perfect black body absorbs all radiation.
  • Q3: C - Good reflector has low absorptance.

Memory Aids

  • \( a + r + t = 1 \)
  • Black body: \( a=1, r=0, t=0 \)
  • Good reflector = bad absorber.
Diagram 10 – NEET Physics Thermal Properties of Matter

Wien's Displacement Law

Key Points

  • Wavelength of maximum radiation intensity \( \lambda_m \) and temperature \( T \) satisfy \( \lambda_m T = b \).
  • Constant \( b = 2.89 \times 10^{-3} \) mK.
  • As temperature increases, \( \lambda_m \) shifts to shorter wavelengths.
  • Used to find temperature of stars from their radiation.

Solved Examples

  • Ex 1: Find \( \lambda_m \) for a body at 5800 K.
    • \( \lambda_m = \frac{b}{T} = \frac{2.89 \times 10^{-3}}{5800} = 4.98 \times 10^{-7} \) m (498 nm)

Practice Set

  • Q1: Wien's constant \( b \) has value
    • A) \( 2.89 \times 10^{-3} \) mK
    • B) \( 5.67 \times 10^{-8} \) W/m8K8
    • C) \( 3.0 \times 10^{8} \) m/s
    • D) \( 1.38 \times 10^{-23} \) J/K
  • Q2: If \( \lambda_m = 500 \) nm, temperature \( T \) is
    • A) 5780 K
    • B) 2890 K
    • C) 1000 K
    • D) 2000 K
  • Q3: As temperature increases, \( \lambda_m \) shifts
    • A) To longer wavelengths
    • B) To shorter wavelengths
    • C) Remains constant
    • D) Randomly

Answer Key

  • Q1: A - Wien's constant is \( 2.89 \times 10^{-3} \) mK.
  • Q2: A - \( T = \frac{b}{\lambda_m} = \frac{2.89 \times 10^{-3}}{500 \times 10^{-9}} = 5780 \) K.
  • Q3: B - Peak wavelength shifts to shorter wavelengths with higher temperature.

Memory Aids

  • \( \lambda_m T = b \)
  • Hotter body emits shorter wavelength radiation.
Diagram 11 – NEET Physics Thermal Properties of Matter

Stefan-Boltzmann Law

Key Points

  • Emissive power \( E \) of a perfect black body: \( E = \sigma T^4 \).
  • Stefan's constant \( \sigma = 5.67 \times 10^{-8} \) W/m8K8.
  • For ordinary body: \( E = e \sigma T^4 \), where \( e \) is emissivity.
  • Net energy radiated when surrounded by temperature \( T_0 \): \( E = e A \sigma (T^4 - T_0^4) t \).

Solved Examples

  • Ex 1: Calculate radiant energy emitted by a black body at 500 K with area 2 m8 in 10 s.
    • \( E = \sigma T^4 = 5.67 \times 10^{-8} \times 500^4 = 354.4 \) W/m8
    • Energy \( Q = E A t = 354.4 \times 2 \times 10 = 7088 \) J

Practice Set

  • Q1: Stefan's constant \( \sigma \) has value
    • A) \( 5.67 \times 10^{-8} \) W/m8K8
    • B) \( 2.89 \times 10^{-3} \) mK
    • C) \( 3.0 \times 10^{8} \) m/s
    • D) \( 1.38 \times 10^{-23} \) J/K
  • Q2: Radiant energy emitted by a body is proportional to
    • A) \( T \)
    • B) \( T^2 \)
    • C) \( T^3 \)
    • D) \( T^4 \)
  • Q3: If emissivity \( e = 0.8 \), area \( A = 1 \) m8, temperature \( T = 400 \) K, time \( t = 5 \) s, calculate radiant energy.
    • A) 1.16 J
    • B) 2.91 J
    • C) 3.72 J
    • D) 4.56 J

Answer Key

  • Q1: A - Stefan's constant is \( 5.67 \times 10^{-8} \) W/m8K8.
  • Q2: D - Radiant energy is proportional to \( T^4 \).
  • Q3: B - \( Q = e A \sigma T^4 t = 0.8 \times 1 \times 5.67 \times 10^{-8} \times 400^4 \times 5 = 2.91 \) J.

Memory Aids

  • \( E = \sigma T^4 \)
  • Emissivity \( e \) scales radiant energy.

Thermal Conduction: Ohm's Law Analogy

Key Points

  • Heat flow rate: \( H = \frac{dQ}{dt} = \frac{K A (T_1 - T_2)}{L} \).
  • Thermal resistance: \( R_{th} = \frac{L}{K A} \).
  • Analogy: \( H = \frac{\Delta T}{R_{th}} \) similar to \( I = \frac{V}{R} \) in electricity.
  • Results from Ohm's law apply to thermal conduction.

Solved Examples

  • Ex 1: Calculate thermal resistance of a rod of length 0.5 m, area 0.01 m8, and thermal conductivity 200 W/mK.
    • \( R_{th} = \frac{L}{K A} = \frac{0.5}{200 \times 0.01} = 0.25 \) K/W

Practice Set

  • Q1: Thermal resistance \( R_{th} \) is
    • A) \( \frac{K A}{L} \)
    • B) \( \frac{L}{K A} \)
    • C) \( K A L \)
    • D) \( \frac{L K}{A} \)
  • Q2: Heat flow rate \( H \) is
    • A) \( \frac{\Delta T}{R_{th}} \)
    • B) \( R_{th} \Delta T \)
    • C) \( K A L \)
    • D) \( \frac{L}{K A} \)
  • Q3: For a rod with \( R_{th} = 0.5 \) K/W and temperature difference 100 K, heat flow rate is
    • A) 50 W
    • B) 200 W
    • C) 100 W
    • D) 0.5 W

Answer Key

  • Q1: B - Thermal resistance \( R_{th} = \frac{L}{K A} \).
  • Q2: A - Heat flow rate \( H = \frac{\Delta T}{R_{th}} \).
  • Q3: C - \( H = \frac{100}{0.5} = 200 \) W.

Memory Aids

  • Thermal resistance analogous to electrical resistance.
  • Heat flow \( H = \frac{\Delta T}{R_{th}} \).
Diagram 12 – NEET Physics Thermal Properties of Matter

Thermal Conduction in Composite Slabs

Key Points

  • Series arrangement: Slabs stacked one after another.
    • Heat flow: \( Q = \frac{A (T_1 - T_2) t}{\frac{x_1}{K_1} + \frac{x_2}{K_2} + \frac{x_3}{K_3}} \)
    • Equivalent conductivity: \( \frac{1}{K} = \left( \frac{x_1}{K_1} + \frac{x_2}{K_2} + \frac{x_3}{K_3} \right) \frac{1}{x_1 + x_2 + x_3} \)
  • Parallel arrangement: Slabs side by side.
    • Heat flow: \( Q = (K_1 A_1 + K_2 A_2 + K_3 A_3) \frac{(T_1 - T_2)}{x} t \)
    • Equivalent conductivity: \( K = \frac{K_1 A_1 + K_2 A_2 + K_3 A_3}{A_1 + A_2 + A_3} \)

Solved Examples

  • Ex 1: Calculate equivalent conductivity for series slabs with \( x_1 = x_2 = x_3 = 1 \) m, \( K_1 = 2 \), \( K_2 = 4 \), \( K_3 = 6 \) W/mK.
    • \( \frac{1}{K} = \frac{1}{2} + \frac{1}{4} + \frac{1}{6} = 0.5 + 0.25 + 0.1667 = 0.9167 \)
    • \( K = 1.09 \) W/mK

Practice Set

  • Q1: In series slabs, total thermal resistance is
    • A) Sum of individual resistances
    • B) Product of individual resistances
    • C) Average of individual resistances
    • D) None
  • Q2: Equivalent conductivity for parallel slabs is
    • A) Weighted average by thickness
    • B) Weighted average by area
    • C) Harmonic mean
    • D) Geometric mean
  • Q3: Heat flow through parallel slabs depends on
    • A) Total area and conductivity
    • B) Thickness only
    • C) Temperature difference only
    • D) None

Answer Key

  • Q1: A - Thermal resistances add in series.
  • Q2: B - Equivalent conductivity is area-weighted average.
  • Q3: A - Heat flow depends on total area and conductivity.

Memory Aids

  • Series: Resistances add.
  • Parallel: Conductivities weighted by area.
Diagram 13 – NEET Physics Thermal Properties of Matter

Ice Layer Growth Time

Key Points

  • Time to grow ice layer from thickness \( x_1 \) to \( x_2 \):
    • \( t = \frac{\rho L}{2 K T} (x_2^2 - x_1^2) \)
    • \( \rho \): density, \( L \): latent heat, \( K \): thermal conductivity, \( T \): atmospheric temperature.
  • Time intervals for thickness changes 0 to \( x \), \( x \) to \( 2x \), etc. are in ratio 1:3:5.

Solved Examples

  • Ex 1: If time to grow ice from 0 to \( x \) is 1 hour, time from \( x \) to \( 2x \) is
    • 3 hours (ratio 1:3)

Practice Set

  • Q1: Time to grow ice layer is proportional to
    • A) Thickness \( x \)
    • B) Square of thickness \( x^2 \)
    • C) Cube of thickness \( x^3 \)
    • D) None
  • Q2: Ratio of time intervals for ice growth from 0 to \( x \), \( x \) to \( 2x \), \( 2x \) to \( 3x \) is
    • A) 1:2:3
    • B) 1:3:5
    • C) 1:4:9
    • D) 1:1:1
  • Q3: In the formula \( t = \frac{\rho L}{2 K T} (x_2^2 - x_1^2) \), \( T \) is
    • A) Temperature of ice
    • B) Temperature of water
    • C) Temperature of atmosphere
    • D) None

Answer Key

  • Q1: B - Time is proportional to square of thickness difference.
  • Q2: B - Time intervals ratio is 1:3:5.
  • Q3: C - \( T \) is atmospheric temperature.

Memory Aids

  • Ice growth time \( \propto x^2 \).
  • Time intervals ratio odd numbers: 1, 3, 5...

Newton's Law of Cooling

Key Concepts

  • Rate of cooling \( \left(-\frac{dQ}{dt}\right) \) is proportional to temperature difference \( (T_2 - T_1) \) if difference < 40°C.
  • Mathematically: \( \frac{dQ}{dt} = k (T_2 - T_1) \), where \( k \) depends on surface area and nature.
  • Temperature decreases exponentially: \( T = T_0 + (T_i - T_0) e^{-kt} \), \( T_i \) = initial temp, \( T_0 \) = surrounding temp.
  • Plotting \( \ln(T - T_0) \) vs time \( t \) gives a straight line with slope \( -k \) and intercept \( \ln(T_i - T_0) \).
  • Shortcut formula: \( \frac{T_1 - T_2}{t} = k \left( \frac{T_1 + T_2}{2} - T_0 \right) \) to avoid calculating \( e^{-kt} \).
Diagram 14 – NEET Physics Thermal Properties of Matter

Solved Examples

  • Ex 1: Initial temp \( T_i = 80^\circ C \), surrounding temp \( T_0 = 30^\circ C \), \( k = 0.1 \ \text{s}^{-1} \). Find temp after 10 s.
    • Use \( T = T_0 + (T_i - T_0) e^{-kt} \)
    • \( T = 30 + (80 - 30) e^{-0.1 \times 10} = 30 + 50 e^{-1} \approx 30 + 50 \times 0.3679 = 48.4^\circ C \)
  • Ex 2: Given \( T_1 = 70^\circ C \), \( T_2 = 50^\circ C \), \( T_0 = 30^\circ C \), time \( t = 5 \) min. Find \( k \).
    • Use shortcut: \( \frac{T_1 - T_2}{t} = k \left( \frac{T_1 + T_2}{2} - T_0 \right) \)
    • \( \frac{70 - 50}{5} = k (60 - 30) \Rightarrow 4 = 30k \Rightarrow k = \frac{4}{30} = 0.1333 \ \text{min}^{-1} \)

Practice Set

  • Q1: If the initial temperature of a body is 90°C and surrounding temperature is 30°C, which formula gives temperature at time \( t \)?
    • A) \( T = T_i e^{-kt} \)
    • B) \( T = T_0 + (T_i - T_0) e^{-kt} \)
    • C) \( T = T_0 e^{-kt} \)
    • D) \( T = (T_i - T_0) e^{kt} \)
  • Q2: For a cooling body, the plot of \( \ln(T - T_0) \) vs time \( t \) is:
    • A) A horizontal line
    • B) A straight line with positive slope
    • C) A straight line with negative slope
    • D) A parabola
  • Q3: A body cools from 80°C to 60°C in 5 minutes in surroundings of 30°C. Using shortcut formula, find \( k \).
    • A) 0.1 min⁻¹
    • B) 0.133 min⁻¹
    • C) 0.2 min⁻¹
    • D) 0.05 min⁻¹

Answer Key

  • Q1: B - Formula includes surrounding temperature and exponential decay.
  • Q2: C - \( \ln(T - T_0) \) decreases linearly with time, slope = \( -k \).
  • Q3: B - Using \( \frac{T_1 - T_2}{t} = k \left( \frac{T_1 + T_2}{2} - T_0 \right) \), \( k = 0.133 \) min⁻¹.

Memory Aids

  • Cooling rate ∝ temperature difference (small difference < 40°C).
  • Temperature decays exponentially: \( T = T_0 + (T_i - T_0) e^{-kt} \).
  • Plot \( \ln(T - T_0) \) vs \( t \) → straight line with slope \( -k \).
  • Shortcut: \( \frac{T_1 - T_2}{t} = k \left( \frac{T_1 + T_2}{2} - T_0 \right) \) avoids exponentials.
Diagram 15 – NEET Physics Thermal Properties of Matter

NEET Physics — ALL CHAPTERS

1

Basic Mathematics

2

Units and Measurement

3

Motion in a Straight Line

4

Motion in a Plane

5

Laws of Motion

6

Work, Energy and Power

7

System of Particles and Rotational Motion

8

Gravitation

9

Mechanical Properties of Solids

10

Mechanical Properties of Fluids

11

Thermal Properties of Matter

12

Thermodynamics

13

Kinetic Theory

14

Oscillations

15

Waves

16

Electric Charges and Fields

17

Electrostatic Potential and Capacitance

18

Current Electricity

19

Moving Charges and Magnetism

20

Magnetism and Matter

21

Electromagnetic Induction

22

Alternating Current

23

Electromagnetic Waves

24

Ray Optics and Optical Instruments

25

Wave Optics

26

Dual Nature of Radiation and Matter

27

Atoms

28

Nuclei

29

Semiconductor Electronics: Materials, Devices and Simple Circuits