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Tamil Nadu Board of Secondary EducationHSC Science Class 11

Revision: Thermodynamics Chemistry HSC Science Class 11 Tamil Nadu Board of Secondary Education

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Definitions [30]

Definition: Thermodynamic System

A part of the universe chosen for analysis, separated by boundaries, where energy and matter exchanges are observed, is called a thermodynamic system.

OR

An assembly of an extremely large number of particles (atoms or molecules) in solid, liquid, gaseous, or a combination of two or more phases is called a thermodynamic system.

Definition: Surrounding

Everything outside the system which has direct effect on the system is called its surrounding.

Definition: Isolated System

A system that exchanges neither energy nor matter with its surroundings is called an isolated system.

Definition: Closed System

A system that exchanges only energy (not matter) with its surroundings is called a closed system.

Definition: Thermodynamics

The branch of science which deals with exchange of heat energy between bodies and conversion of heat energy into mechanical energy and vice versa is called thermodynamics.

Definition: Open System

A system that exchanges both energy and matter with its surroundings is called an open system.

Define the following term:

Adiabatic process

A thermodynamic process during which there is no transfer of heat (energy) from the system to the surroundings or from the surroundings to the system is called an adiabatic process.

Define the following term:

Isochoric process

It is defined as one in which the volume of the system remains constant during its change from the initial to the final stage of the process.

Define the following term:

Isobaric process

It is defined as one in which the pressure of the system remains constant during its change from the initial to the final state.

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: 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: 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: Intensive Variables

The thermodynamic state variables that do not depend on the size of the system (e.g., pressure, temperature) are called intensive variables.

Definition: Thermodynamic State Variables

The specific values of macroscopic variables that completely describe every equilibrium state of a thermodynamic system are called thermodynamic state variables.

Definition: Extensive Variables

The thermodynamic state variables that depend on the size of the system (e.g., internal energy, volume) are called extensive variables.

Definition: Enthalpy of Hydration

It is the enthalpy change during the hydration of 1 mole of anhydrous salt by the addition of a specific number of moles of water.

Definition: Enthalpy

The total heat content of a system at constant pressure is known as enthalpу.

ΔH = ΔU + PΔV

At constant pressure: ΔH = qp​ (heat exchanged at constant pressure).

Definition: Enthalpy of Combustion:

It is defined as the change in heat enthalpy when one mole of a substance is completely burnt in oxygen.

ΔΗ = Σ (Heat of Combustion of reactant)- Σ (Heat of Combustion of product)

Definition: Enthalpy of Solution

It is the enthalpy change when one mole of it dissolves in a specified amount of solvent

Definition: Enthalpy of Dilution

It is the enthalpy change associated with diluting a component in a solution at constant pressure and temperature.

Define enthalpy.

Enthalpy of a system is sum of internal energy of a system and the energy equivalent to PV work.

H = U + PV

Define enthalpy of combustion.

The heat of combustion of a substance is defined as “The change in enthalpy of a system when one mole of the substance is completely burnt in excess of air or oxygen”. It is denoted by ∆HC.

Definition: Enthalpy of Neutralisation:

It is defined as the heat evolved or decrease in enthalpy when 1 gm equivalent of an acid is neutralised by 1 gm equivalent of a base in solution.

Define enthalpy of neutralization.

The enthalpy of neutralization is defined as the change in enthalpy of the system when one gram equivalent of an acid is neutralized by one gram equivalent of a base or vice versa in dilute solution.

\[\ce{H^+_{(aq)} + OH^-_{(aq)} -> H2O_{(l)}}\] = 57.32 kJ

Define molar heat capacity.

The heat capacity for 1 mole of a substance, is called molar heat capacity (cm). It is defined as “The amount of heat absorbed by one mole of the substance to raise its temperature by 1 kelvin”.

Definition: Entropy

A useful state variable that measures the change in heat divided by the temperature of the system, where the combined entropy of the system and its environment remains constant if the process approaches reversibility, is called entropy.

Define is Gibb’s free energy.

Gibbs free energy is defined as the part of the total energy of a system that can be converted (or) available for conversion into work.

G = H − TS

where G = Gibb’s free energy

H = enthalpy

T = temperature

S = entropy

Formulae [3]

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 × \[\frac{(P_T-P_1)}{(P_2-P_1)}\]

Write the mathematical equation of the first law of thermodynamics for an isochoric process.

By substituting equation W = −pex . ΔV in the equation ΔU = q + W, we get

ΔU = q − pex . ΔV  ...(1)

If the reaction is carried out in a closed container so that the volume of the system is constant, then Δ = 0. In such a case, no work is involved.

The equation (1) becomes ΔU = qv

Equation (1) suggests that the change in internal energy of the system is due to heat transfer. The subscript v indicates a constant volume process. As U is a state function, qv is also a state function. We see that an increase in the internal energy of a system is numerically equal to the heat absorbed by the system in a constant volume (isochoric) process.

Formula: Entropy

ΔS = \[\frac {ΔQ}{T}\]

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.

Write the mathematical equation of the first law of thermodynamics for an isochoric process.

By substituting equation W = −pex . ΔV in the equation ΔU = q + W, we get

ΔU = q − pex . ΔV  ...(1)

If the reaction is carried out in a closed container so that the volume of the system is constant, then Δ = 0. In such a case, no work is involved.

The equation (1) becomes ΔU = qv

Equation (1) suggests that the change in internal energy of the system is due to heat transfer. The subscript v indicates a constant volume process. As U is a state function, qv is also a state function. We see that an increase in the internal energy of a system is numerically equal to the heat absorbed by the system in a constant volume (isochoric) process.

Law: First Law of Thermodynamics

Statement:
The net heat energy supplied to a system is equal to the sum of the change in internal energy of the system and the work done by the system. It is based on the law of conservation of energy.

Formula:

Q = ΔU + W

where Q = heat added, ΔU = change in internal energy, W = work done by the system.

Write statement of second law of thermodynamics.

The second law of thermodynamics states that the total entropy of a system and its surroundings increases in a spontaneous process.

Mathematically,

ΔStotal = `Delta S_"system" + Delta S_"surroundings" gt 0`

For an equilibrium:

ΔStotal = 0

State the third law of thermodynamics.

The third law of thermodynamics states that the entropy of a pure crystalline substance at absolute zero is zero. Otherwise, it can be stated that it is impossible to lower the temperature of an object to absolute zero in a finite number of steps. Mathematically,

`lim_(T->0)` S = 0 for a perfectly ordered crystalline state.

Key Points

Key Points: First Law of Thermodynamics

First Law: Energy of system + surroundings remains constant → ΔU = q + W

ΔU: change in internal energy, q: heat, W: work done on system

Sign convention:

  • Work by system (−)
  • on system (+)
  • Heat absorbed (+)
  • released (−)

ΔU > 0: energy enters system; ΔU < 0: energy leaves system

  • Isothermal: ΔU = 0 → q = −W
  • Adiabatic: q = 0 → ΔU = W
  • Isochoric: W = 0 → ΔU = q
  • Isobaric: ΔU = q + W
Key Points: Entropy and Second Law of Thermodynamics

Entropy (S): A thermodynamic property that measures the degree of randomness or disorder of a system.

\[\Delta S=\frac{q_{rev}}{T}\]

Second Law: The entropy of the universe always tends to increase during any spontaneous process.

Δ Suniverse > 0 (for spontaneous processes)

Total entropy change:

Δ Stotal = ΔSsystem + ΔSsurroundings
 
Condition Process
ΔStotal = +ve Spontaneous
ΔStotal = −ve Non-spontaneous
ΔStotal = 0 Equilibrium

Entropy of mixing:

\[\Delta S_{mix}=-R\sum x_i\ln x_i\]

(ΔS for mixing is always positive, since ΔS is always fractional/positive)

Key Points: Third Law of Thermodynamics and Absolute Entropy

Third Law: The entropy of a perfectly ordered crystalline substance at absolute zero (0 K) is zero.

Absolute Entropy (Standard Molar Entropy, S°): The entropy value of a substance at 298 K and 1 bar pressure, relative to 0 K.

  • Unlike the enthalpy of formation, the absolute entropy of elements is not zero at standard conditions.
  • Standard entropy of reaction: \[\Delta_{r}S^{\circ}=\sum S_{products}^{\circ}-\sum S_{reactants}^{\circ}\]
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