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Revision: Class 11 >> Thermal Properties of Matter NEET (UG) Thermal Properties of Matter

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Definitions [41]

Define latent heat capacity.

Latent heat capacity of a substance is defined as the amount of heat energy required to change the state of a unit mass of the material.

Definition: Temperature

The temperature of a body determines its hotness, while heat energy is its heat content.

Define molar specific heat capacity.

Molar specific heat capacity is defined as heat energy required to increase the temperature of one mole of a substance by IK or 1°C.

C = `1/μ ((Δ"Q")/(Δ"T"))`

Define thermal conductivity.

The quantity of heat transferred through a unit length of a material in a direction normal to Unit surface area due to a unit temperature difference under steady-state conditions is known as the thermal conductivity of a material.

Define specific heat capacity.

Specific heat capacity of a substance is defined as the amount of heat energy required to raise the temperature of 1 kg of a substance by 1 Kelvin or 1°C.

Define one mole.

One mole of any substance is the amount of that substance which contains the Avogadro number (NA) of particles (such as atoms or molecules).

Definition: Heat

"Heat is energy in transit. When two bodies at different temperatures are brought in contact, they exchange heat."

Definition: Temperature

"Temperature is a physical quantity that defines the thermodynamic state of a system."

Definition: Thermal Equilibrium

When two bodies at different temperatures are brought into contact through a diathermic wall, heat flows from the hotter body to the cooler one. This continues until both reach the same temperature, at which point heat flow stops. This state is called thermal equilibrium.

Definition: Adiabatic Wall

An adiabatic wall is an ideal partition that completely prevents heat transfer between two systems. In diagrams, it is shown as a thick, cross-hatched (slanting lines) region.

Definition: Diathermic Wall

diathermic wall is a partition that freely allows heat to flow between two systems. It is shown as a thin dark line in diagrams. A thin copper sheet is a good example.

Definition: Thermometry

Thermometry is the branch of physics dealing with temperature measurement. It relies on the principle that certain physical properties of materials change continuously and predictably with temperature.

Definition: Ideal Gas Equation

“The relation between three properties of a gas, i.e., pressure, volume and temperature, is called the ideal gas equation.”

Definition: Kelvin Scale

The SI absolute temperature scale starting at absolute zero. Written as K (no degree symbol °).

Definition: Ideal Gas

A hypothetical gas whose molecules have no volume and exert no intermolecular forces; obeys PV = μRT exactly.

Definition: Triple Point

The unique temperature & pressure at which solid, liquid, and gas phases of a substance coexist in equilibrium.

Definition: Universal Gas Constant (R)

A constant in the ideal gas equation; R = 8.31 J mol⁻¹ K⁻¹.

Definition: Kelvin

One kelvin = 1/273.16 of the difference between absolute zero and the triple point of water.

Definition: Extrapolation

Extending a graph line beyond the measured data to predict values.

Definition: Absolute Zero

The lowest theoretically possible temperature (0 K = −273.15 °C), where ideal gas molecules have zero kinetic energy.

Answer the following question.

What is thermal stress?

  1. Consider a metallic rod of length l0 fixed between two rigid supports at T °C.
  2. If the temperature of rod is increased by ΔT, length of the rod would become, l = l0 (1 + αΔT) Where, α is the coefficient of linear expansion of the material of the rod.
  3. But the supports prevent the expansion of the rod. As a result, rod exerts stress on the supports. Such stress is termed as thermal stress.
Definition: Thermal Expansion

The increase in the dimensions (length, area, or volume) of a body due to an increase in its temperature is called thermal expansion. Conversely, a decrease in temperature causes contraction.

Define the following term:

Coefficient of cubical expansion

The coefficient of volume expansion is equal to the change in volume of a rod of volume 1m3 when its temperature rises by 1°c.

Define the following term:

Coefficient of superficial expansion

The coefficient of superficial expansion is equal to the change in the area of a rod of area 1m2 when its temperature rises by 1°c.

State the relation between the three types of expansion.

If the Coefficient of Linear expansion is denoted by α
Coefficient of superficial expansion is denoted by β
And Coefficient of volume expansion is denoted by γ
Then the relation between α, β and γ is stated as
β = 2 α and γ = 3 α

α : β : γ : : 1 : 2 : 3

Definition: Specific Heat Capacity

The specific heat capacity of a substance is the amount of heat energy required to raise the temperature of unit mass of that substance through 1°C (or 1 K).

OR

Heat capacity of a body when expressed for the unit mass is called the specific heat capacity of the substance of that body.

OR

The amount of heat energy required to raise the temperature of a unit mass of an object by 1 °C is called the specific heat of that object.

Define heat capacity.

The heat capacity of a body is the quantity of heat required to raise its temperature by 1°C. It depends upon the mass and the nature of the body.

Definition: Calorimetry

Calorimetry is the science of measuring heat exchange during physical or chemical processes. The word comes from the Latin calor (heat) + Greek metron (measure).

Definition: Calorimeter

A calorimeter is a cylindrical vessel which is used to measure the amount of heat gained (or lost) by a body when it is mixed with another body or substance.

Define Triple point.

The triple point of water is that point where water in a solid, liquid and gas state co-exists in equilibrium and this occurs only at a unique temperature and a pressure.

Define Sublimation.

Sublimation is the process in which a solid changes directly into a gas on heating, without passing through the liquid state.

Definition: Change of State

A transition from one state to another is called a change of state (or phase change).

Or

The process of change from one state to another at a constant temperature is called the change of phase.

Definition: Latent Heat

The heat energy absorbed (or liberated) in change of phase is not externally manifested by any rise or fall in temperature, it is called the latent heat.

OR

Latent heat is the quantity of heat energy required to change the state of unit mass of a substance from one phase to another, at constant temperature and constant pressure.

Definition: Latent Heat of Vaporization

The quantity of heat required to convert unit mass of a substance from its liquid state to vapour state, at its boiling point without any change in its temperature is called its latent heat of vapourization (Lv).

Definition: Latent Heat of Fusion

The quantity of heat required to convert unit mass of a substance from its solid state to the liquid state, at its melting point, without any change in its temperature, is called its latent heat of fusion (Lf).

OR

The heat energy absorbed at constant temperature during the transformation of solid into liquid is called the latent heat of fusion. The amount of heat energy absorbed at constant temperature by unit mass of a solid to convert into liquid phase is called the specific latent heat of fusion.

Answer the following question.

Define coefficient of thermal conductivity.

The coefficient of thermal conductivity of a material is defined as the quantity of heat that flows in one second between the opposite faces of a cube of side 1 m, the faces being kept at a temperature difference of 1°C (or 1 K).

Definition: Bad Conductors of Heat

Substances that do not conduct heat easily are called bad conductors of heat.

Definition: Good Conductors of Heat

Solid substances that conduct heat easily are called good conductors of heat.

Definition: Conduction

Conduction is the process by which heat flows from the hot end to the cold end of a solid body without any net bodily movement of the particles of the body.

Definition: Convection

Convection is the process by which heat is transmitted through a substance from one point to another due to the actual bodily movement of the heated particles of the substance.

Definition: Radiation

The transfer of heat energy from one place to another via emission of EM energy (in a straight line with the speed of light) without heating the intervening medium is called radiation.

Formulae [8]

Formula: Average Kinetic Energy and Temperature

\[E_k=\frac{3}{2}k_BT\]

Where:

  • Ek = Average kinetic energy of the molecules (in joules)
  • kB = Boltzmann constant = 1.380649 × 10−23 J/K
  • T = Absolute temperature (in kelvin)
Formula: Heat Exchange

Q = mcΔT

Where:

  • Q = Heat absorbed or released (in joules)
  • m = Mass of the substance (in kg)
  • c = Specific heat capacity (J/kg·K)
  • ΔT = Change in temperature (Tfinal−Tinitial)
Conversion Formulas

Master Conversion Formula:

\[\frac{T_F-32}{180}=\frac{T_C}{100}\] = \[\frac {T_K−273.15}{100}\]

Conversion Formula
Celsius → Fahrenheit TF = \[\frac{9}{5}\] × TC + 32
Fahrenheit → Celsius TC = \[\frac{5}{9}\] × (TF - 32)
Celsius → Kelvin TK = TC + 273.15)
Kelvin → Celsius TC = TK - 273.15)
Thermometric Property T = 100 × \[\frac{(P_T-P_1)}{(P_2-P_1)}\]
Formula: Combined Gas Law

\[\frac{P_1V_1}{T_1}=\frac{P_2V_2}{T_2}\]

Conversion Formulas

Master Conversion Formula:

\[\frac {T_C}{100}\] = \[\frac {(T_{F}-32)}{180}\] = \[\frac {(T_{K}-273.15)}{100}\]

Celsius → Kelvin: TK = TC + 273.15
Kelvin → Celsius: TC = TK − 273.15
Celsius → Fahrenheit: TF = \[\frac {9}{5}\] × TC + 32
Fahrenheit → Celsius: TC = \[\frac {5}{9}\] × (TF − 32)
Formula: Specific Heat Capacity

Specific heat capacity c = \[\frac{\text{Heat capacity of body } C'}{\text{Mass of the body } m}\]

or

Specific heat capacity c = \[\frac{Q}{m\times\Delta t}\]

Formula: Latent Heat

Q = m × L

where,

Q = Heat energy absorbed or released during phase change
m = Mass of the substance undergoing phase change
L = Specific Latent Heat (characteristic of the substance & process)

SI Units = J kg⁻¹

Mathematical Formulation

Proportionality Form

\[\frac{dT}{dt}\propto(T-T_0)\]

Introducing the constant of proportionality C:

\[\frac{dT}{dt}=C\left(T-T_0\right)\]

T = Temperature of the body at time t
T0 = Temperature of the surroundings (constant)
C = Constant of proportionality
\[\frac {dT}{dt}\] = Rate of fall of temperature (rate of cooling)

Theorems and Laws [5]

Law: The Zeroth Law of Thermodynamics

If system A is in thermal equilibrium with system C, and system B is also in thermal equilibrium with system C, then systems A and B are in thermal equilibrium with each other.

Law: Gay-Lussac's Law — Pressure & Temperature

Statement:

The pressure of a fixed mass of gas is directly proportional to its absolute temperature if volume is kept constant.

Mathematically, P ∝ T ⇒ \[\frac {P}{T}\] = constant

This means: heating a gas in a sealed (rigid) container increases its pressure.

Graph: P vs T (Isochore)

Gay-Lussac's Law P vs T graph showing straight line
P vs T graph at constant volume — a straight line through the origin (Kelvin scale).

Law: Boyle's Law — Pressure & Volume

Statement:

For a fixed mass of gas at constant temperature, the pressure is inversely proportional to the volume.

Mathematically, P ∝ \[\frac {1}{V}\] ⇒ PV = constant

Graph: P vs V (Isotherm)

Boyle's Law PV Graph showing hyperbolic isotherms

This means: squeezing a gas into a smaller space increases its pressure. Doubling the pressure halves the volume.

Law: Charles' Law — Volume & Temperature

Statement:

The volume of a fixed mass of gas is directly proportional to its absolute temperature if the pressure is kept constant.

Mathematically, V ∝ T ⇒ \[\frac {V}{T}\] = constant

Graph: V vs T (Isobar)

A straight line through the origin when using Kelvin. All lines converge at 0 K (absolute zero).

Law: Newton's Law of Cooling

"The rate of loss of heat (dT/dt) of a body is directly proportional to the difference in temperatures (T−T₀) of the body and the surroundings, provided the difference in temperatures is small."

A hot body loses heat to its surroundings in the form of heat radiation. The rate of loss of heat depends on the difference in temperature of the body and its surroundings.

Key Points

Key Points: Ideal Gas Equation
  • An ideal gas has point-mass molecules, no intermolecular forces, and perfectly elastic collisions.
  • Boyle's Law (constant T): PV = constant — pressure and volume are inversely proportional.
  • Charles' Law (constant P): V/T = constant — volume and temperature are directly proportional.
  • Gay-Lussac's Law (constant V): P/T = constant — pressure and temperature are directly proportional.
  • The Ideal Gas Equation, PV = nRT, combines all three laws into a single universal relationship.
  • The Universal Gas Constant R = 8.314 J mol⁻¹ K⁻¹ is the same for all ideal gases.
  • Real gases approximate ideal behaviour at low pressure and high temperature.
  • Always use absolute temperature (Kelvin) in gas law calculations. T(K) = T(°C) + 273.15
Key Points: Absolute Zero and Absolute Temperature
  • Gases expand linearly with temperature, making them useful for thermometers. This consistent behaviour suggests the existence of a lowest temperature limit.
  • Absolute zero (−273.15 °C or 0 K) is the temperature where an ideal gas would have zero pressure. It is the lowest possible temperature.
  • The Kelvin scale begins at absolute zero and uses the triple point of water (273.16 K) as a reference point. It is the SI temperature scale.
  • The ideal gas equation (PV = μRT) combines all gas laws into a single relationship among pressure, volume, and temperature. It works best for gases at low pressure and high temperature.
Key Points: Specific Heat Capacity
  • Heat energy absorbed (Q) depends on: mass (m), rise in temperature (Δt), and specific heat capacity (c), i.e., Q ∝ m × Δt × c.
  • Heat capacity (C') and specific heat capacity (c) are related by: C′ = m × c.
Key Points: Calorimetry
  • Calorimeter: An insulated device used to measure heat transfer during a process.
  • Principle of Calorimetry: Heat lost = Heat gained (energy is conserved).
  • Method of Mixtures: Heat a sample, place it in the calorimeter, and measure the temperature change to calculate the heat.
  • Formula: Used to calculate the specific heat of a substance from measured temperatures and masses.
  • Good Practice: Transfer the sample quickly and stir well for accurate results.
  • Why Water is Used: Water has high specific heat, so it absorbs a lot of heat without a large temperature change.
Key Points: Practical Applications of State
  • A change of state occurs when heat exchange causes a substance to transition between solid, liquid, and gas phases.
  • Temperature remains constant during a phase change because heat energy changes molecular arrangement (potential energy), not molecular speed (kinetic energy).
  • The heating curve has flat plateaus at the melting point (0 °C) and boiling point (100 °C) for water, with rising slopes in between.
Key Points: Latent Heat
  • Formula: Q = mL. Specific latent heat L has SI unit J kg⁻¹.
  • Temperature stays constant during any phase change. Heat energy goes into breaking or forming intermolecular bonds, not into raising kinetic energy.
  • Latent Heat of Fusion (water): Lf = 3.33 × 10⁵ J kg⁻¹ = 80 cal/g. Heat needed to melt 1 kg of ice at 0°C.
  • Latent Heat of Vaporisation (water): Lv = 22.6 × 10⁵ J kg⁻¹ = 540 cal/g. Heat is needed to convert 1 kg of water to steam at 100°C.
  • Lv ≫ Lf because vaporisation requires complete molecular separation and work against atmospheric pressure during expansion.
  • All latent heat values depend on atmospheric pressure. Standard values quoted at 1 atm. Increasing pressure raises the boiling point (pressure cooker effect).
Key Points: Heat Transfer
  • Heat can be transferred in three ways — conduction, convection, and radiation.
  • Conduction transfers heat through solids; molecules vibrate but do not move from their positions.
  • Convection transfers heat through liquids and gases; molecules physically move from place to place.
  • Both conduction and convection require a material medium; radiation does not.
  • Radiation travels through electromagnetic waves at a speed of 3×10⁸ ms⁻¹.
  • Conduction is the slowest process, convection is rapid, and radiation is the fastest mode of heat transfer.
  • The energy received from the Sun is an example of heat transfer by radiation.
Key Points: Conduction
  • The transfer of heat from the hot part to the cold part of an object is called conduction of heat.
  • Conduction takes place through solid substances only — it requires a medium.
  • Heat travels by molecular collisions: fast-vibrating molecules pass energy to slower neighbours.
  • Copper conducts heat faster than aluminium, which conducts faster than steel.
  • Conduction of heat through a substance depends on the property of that substance.
  • Good conductors: silver, copper, aluminium, brass — all metals.
  • Bad conductors: wood, cloth, air, paper — most non-metals.
  • Good conductors of heat are also good conductors of electricity, and bad conductors of heat are also bad conductors of electricity.
Key Points: Convection
  • Convection occurs only in fluids (liquids and gases) — not in solids.
  • In conduction, molecules vibrate but stay in place.
  • In convection, molecules physically move from one place to another.
  • Heating reduces density → hot fluid rises; cool fluid sinks → a convection current is set up.
  • Convection currents transfer heat to the entire mass of the fluid.
  • Potassium permanganate makes convection currents visible as magenta-coloured streams.
Key Points: Radiation
  • When water is heated from the top, its density decreases, and it stays at the top. Since hot water cannot sink, convection does not occur and the bottom remains cool.
  • Radiation is the transfer of heat without a medium — through electromagnetic waves.
  • Heat from the Sun reaches us through radiation across the vacuum of space.
  • All objects above 0 K emit thermal radiation (electromagnetic waves).
  • Radiation is a two-step process: thermal energy → EM waves → thermal energy.
  • Black or dark surfaces absorb more heat radiation; absorption also depends on the intrinsic properties of the substance.
  • An infrared camera uses the radiation emitted by objects to see at night — useful for military surveillance.
  • Copper is an excellent conductor; plastic is a bad conductor (insulator).
  • Heat readily conducts through metals (copper and steel) but not through non-metals (wood and plastic).
Key Points: Newton’s Law of Cooling
  • A hot body loses heat to its surroundings in the form of heat radiation.
  • The rate of cooling is directly proportional to the temperature difference between the body and its surroundings.
  • The cooling curve (T vs t) shows rapid initial cooling that gradually slows down.
  • Plotting \[\frac {dT}{dt}\] vs (T−T₀) gives a straight line through the origin, confirming Newton's law.
  • Mathematically: dT/dt = C(T − T₀), where C is the constant of proportionality.
  • The rate of cooling is proportional to — not independent of — the temperature difference. A 4× drop in temperature difference produces a 4× drop in cooling rate.
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