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

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Definitions [56]

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 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.

OR

The degree of hotness or coldness of an object (and not the amount of its thermal energy) is called temperature.

Definition: Heat

The form of energy transferred between two or more systems and its surroundings by virtue of temperature difference is called heat.

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 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 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."

OR

The form of energy which is exchanged among various bodies or a system on account of temperature difference is called heat.

  • Units: joule (J), calorie (cal), BTU (British Thermal Unit)

Definition: Temperature

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

OR

The degree of hotness or coldness of a body, whose natural flow is from higher temperature to lower temperature, is called temperature.

  • SI unit: kelvin (K) | Scalar quantity

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: 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: 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: Ice Point

The temperature at which pure water freezes at 1 atm pressure is called the ice point.

Definition: Steam Point / Boiling Point

The temperature at which pure water boils and vapourises into steam at 1 atm pressure is called the steam point or boiling point.

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.”

OR

The relation between the three properties of a gas - pressure (P), volume (V), and temperature (T) - expressed as PV = nRT, is called the ideal gas equation.

Definition: Absolute Zero

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

OR

The lowest attainable temperature, obtained by plotting the relation between pressure of the gas vs its temperature, where all lines for different gases cut the temperature axis at the same point (−273.15°C), is called the absolute zero of temperature.

Definition: Kelvin

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

Definition: Universal Gas Constant (R)

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

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.

OR

The temperature where the solid, liquid, and gas state of a material co-exist in equilibrium, and this occurs only at a unique temperature and pressure, is called the triple point.

Definition: Absolute Temperature

The temperature scale where −273.15°C corresponds to 0 K, i.e., the temperature at which the pressure of a gas would become zero, is called the absolute temperature (0 K).

Definition: Kelvin Scale

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

Definition: Extrapolation

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

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.

OR

The increase in the dimensions of a body due to an increase in its temperature is called thermal expansion.

OR

When matter changes its shape, area and volume in response to a change in temperature (i.e., an object expands and becomes larger due to a change in its temperature), this is called thermal expansion.

Definition: Coefficient of Superficial Expansion (β)

The change in area per unit original surface area of a two-dimensional body (at 0°C) per unit rise in temperature is called the coefficient of superficial expansion.

Definition: Volume Expansion

When a solid is heated and its volume increases, the expansion is called volume expansion.

ΔV = V0γΔT

where γ is called the coefficient of volume expansion.

Definition: Coefficient of Linear Expansion (α)

The increase in length per unit original length of a rod (at 0°C) per unit rise in temperature is called the coefficient of linear expansion.

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: Coefficient of Cubical Expansion (γ)

The increase in volume of a body per unit original volume (at 0°C) per unit rise in temperature is called the coefficient of cubical expansion.

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: Linear Expansion

When a solid is heated and its length increases, the increase in length proportional to the original length and temperature change is called linear expansion.

ΔL = L0αΔT
Final length: L = L0(1 + αΔT)

where α is called the coefficient of linear expansion.

Definition: Areal (Superficial) Expansion

When the area of an object changes with increase in temperature, it is called areal expansion (or superficial expansion).

ΔA = A0βΔT

where β is called the coefficient of areal expansion.

Definition: Molar Heat Capacity

The amount of heat required to raise the temperature of one mole of a substance through a unit degree Celsius or Kelvin is called molar heat capacity.

Definition: Heat Capacity

The quantity of heat needed to raise the temperature of the whole body by 1°C (or 1 K) is called heat capacity.

OR

The amount of heat ΔQΔQ supplied to a substance to change its temperature from T to T + ΔT, per unit mass per unit degree change in temperature, is called specific heat:

s = \[\frac {S}{m}\] = \[\frac {1}{m}\]\[\frac {ΔQ}{ΔT}\]
  • Unit: J kg⁻¹ K⁻¹

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.

OR

The amount of heat per unit mass absorbed or given out by a substance to change its temperature by one unit (one degree), i.e., 1°C or 1 K, is called specific heat capacity.

OR

The quantity of heat required to raise the temperature of a unit mass of a gas by one degree, whose exact value depends upon the mode of heating the gas and can range from zero to infinity or even be negative, is called the specific heat capacity of a gas.

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).

OR

An experimental technique for the quantitative measurement of heat exchange is called calorimetry.

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.

Definition: Change of State

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

OR

A transition from one state of matter (solid, liquid, or gas) to another is called change of state.

Define Sublimation.

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

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.

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.

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

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.

OR

The quantity of heat absorbed or given out by unit mass of a substance during change of state of the substance at a constant temperature is called the latent heat of the substance.

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: 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.

OR

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 is called conduction.

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: 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.

OR

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

OR

The mode of heat transfer by actual motion of matter (bulk transport of fluid) from the source of heat, which occurs only in fluids, is called convection.

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.

OR

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.

Definition: Emissivity

The ratio that measures how effectively a surface emits thermal radiation compared to a perfect black body, where for a perfect radiator e = 1, is called emissivity.

Definition: Thermal Conductivity

Thermal conductivity of a solid is a measure of the ability of the solid to conduct heat through it. Thus, good conductors of heat have higher thermal conductivity than bad conductors.

OR

The measure of how well a material conducts heat — the greater the value of K, the more rapidly it conducts heat — is called thermal conductivity.

  • SI Unit: Js⁻¹ m⁻¹ K⁻¹ or W m⁻¹ K⁻¹

Definition: Temperature Gradient

Under steady state condition, the temperature at points within the rod decreases uniformly with distance from the hot end to the cold end. The fall of temperature with distance between the ends of the rod in the direction of flow of heat is called the temperature gradient.

OR

The rate of change of temperature with distance in the direction of flow of heat is called temperature gradient.

Formulae [11]

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)
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)
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: Heat Transfer

\[Q=mc\Delta T\]

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: Molar Heat Capacity

C = M × c = Q/(nΔT)

Unit: J/mol · K

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)

Formula: Temperature Gradient

\[\frac {(T_1-T_2)}{x}\]

where,

  • T₁ = Temperature of hot end
  • T₂ = Temperature of cold end
  • x = Length of the rod

Theorems and Laws [8]

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

When volume is constant, the ratio of pressure to temperature of a gas remains constant.

\[\frac {P}{T}\] = constant
Law: Boyle's Law

When temperature is constant, the product of pressure and volume of a gas remains constant.

pV = constant
Law: Charle's Law

When pressure is constant, the ratio of volume to temperature of a gas remains constant.

\[\frac {V}{T}\] = constant
Law: Principle of Calorimetry

Statement: When different parts of an isolated system are at different temperatures, heat transfers from the part at higher temperature to the part at lower temperature. The heat lost by the hot object is equal to the heat gained by the cold object, provided no heat is allowed to escape to the surroundings.

Heat lost by hot body = Heat gained by cold body
m1c1Δθ1 = m2c2Δθ2

(For liquid in calorimeter: m1c1Δθ + mcccΔθ)

Key Points:

  • A system is said to be isolated if no exchange of heat occurs between the system and its surroundings.
  • Calorimetry literally means measurement of heat.
  • Energy supplied by heater = VIt (voltage × current × time).
  • This principle is based on the Law of Conservation of Energy.
Law: Fourier's Law of Heat Conduction

Statement: In steady-state heat flow by conduction in a bar with ends maintained at different temperatures TC and TD, the heat flow is proportional to the temperature difference and the area of cross-section A, and inversely proportional to the length L.

H = K\[\frac {A(T_C−T_D)}{L}\]

Also written as:

\[\frac {Q}{t}\] = \[\frac {kA(T_{hot}−T_{cold})}{d}\]

Where K is the thermal conductivity of the material.

Key Points:

  • Gases are poor conductors; liquids have intermediate conductivities; solids are generally good conductors.
  • The greater the value of K, the more rapidly the material conducts heat.
Law: Stefan–Boltzmann Law

Statement: All bodies emit radiant energy depending on their temperature. The heat emitted (H) by a body is given by:

H = σeAT4

Where:

  • σ = Stefan-Boltzmann constant
  • e = Emissivity (for perfect radiator, e = 1)
  • A = Area of the body
  • T = Temperature (in Kelvin)

Key Points:

  • Black bodies absorb and emit more radiant energy than bodies of lighter colors.
  • Thermal radiation is partially reflected and partially absorbed when it falls on other bodies.
Law: Newton's Law of Cooling

Statement: The rate of loss of heat \[\frac {dT}{dt}\] of the body is directly proportional to the difference of temperature (T − T0) of the body and the surroundings, provided the difference in temperatures is small.

Mathematical Form:

\[\frac {dT}{dt}\] ∝ (T − T0)

Graphical Representation:

  • Graph of rate of cooling \[\left(\frac{dT}{dt}\right)\] vs (T − T0) → straight line through origin.

  • Graph of Temperature T vs time t → exponential decay curve (temperature drops steeply at first, then gradually).

Key Points

Key Points: Ideal Gas Equation
  • An ideal gas has point-mass molecules, no intermolecular forces, and perfectly elastic collisions.
  • 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: Thermal Expansion
  • Solids have three types of expansion - Linear (1D), Superficial (2D), and Cubical (3D) - with β = 2α and γ = 3α.
  • Change in dimensions: ΔL = L0αΔT, ΔA = A0βΔT, ΔV = V0γΔT.
  • Liquids have only volume expansion; real expansion = apparent expansion + vessel expansion, i.e., γr = γa + γv.
  • Gases have only real expansion as the container expansion is negligible.
  • Final quantity after heating: L = L0(1 + αΔT), A = A0(1 + βΔT), V = V0(1 + γΔT).
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
  • A calorimeter is an insulated device used to measure heat transfer; measurement of specific heat of a substance is carried out using it.
  • Principle of Calorimetry: Heat lost by hot body = Heat gained by cold body, which represents the law of conservation of heat energy.
  • In the method of mixtures, a heated sample is placed in the calorimeter and the temperature change is measured to calculate specific heat using the formula Q = msΔt.
  • Specific heat of a substance depends on the nature of the substance; water is preferred in calorimetry due to its high specific heat, allowing it to absorb large amounts of heat with minimal temperature change.
  • For accurate results, the sample must be transferred quickly into the calorimeter and stirred well to ensure uniform heat distribution.
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.
Key Points: Thermal Conductivity
  • Thermal conductivity is the measure of a solid's ability to conduct heat. Good conductors have higher thermal conductivity.
  • When a metal rod is heated at one end, heat flows from the hot end to the cold end by conduction.
  • Variable state — the temperature of every section keeps increasing with time.
  • Steady state — temperature at each section is constant but different across sections.
  • Temperature gradient = (T₁ − T₂) / x — the fall of temperature per unit length in the direction of heat flow.
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