skip to content
Skip to content
Home » Class 11 Chemistry Laws of Thermodynamics – Notes and Concepts

Class 11 Chemistry Laws of Thermodynamics – Notes and Concepts

There are 4 laws of thermodynamics:

  1. The Zeroth law of thermodynamics.
  2. The First law of thermodynamics.
  3. The Second law of thermodynamics.
  4. The Third law of thermodynamics

Zeroth law of thermodynamics

The zeroth law of thermodynamics states that if two thermodynamic systems are each in thermal equilibrium with a third one, then they are in thermal equilibrium with each other. The law is based on temperature measurement and is used to predict whether heat will transfer between objects or not. But overall, this law focuses on the idea that if the systems are in thermal equilibrium, no heat flow will take place. 

First law of thermodynamics

The First Law of Thermodynamics states that heat is a form of energy, and thermodynamic processes are therefore subject to the principle of conservation of energy. This indicates that heat energy cannot be created or destroyed. It can, however, be transferred from one location to another and converted to and from other forms of energy, and heat given to the system is used to change the internal energy, while the rest is used to do work by the system. 

ΔQ = ΔU + W
Where,
• ΔQ is the heat given or lost
• ΔU is the change in internal energy
• W is the work done

Second Law of Thermodynamics

The second law of thermodynamics states that the entropy in an isolated system always increases. Any isolated system spontaneously evolves toward thermal equilibrium, the state of maximum entropy. It is the second law of thermodynamics that provides the criterion for the feasibility of any process.  

Note: The entropy of the universe only increases and never decreases.

Ready to Score Better in Your SSLC Exams?

Prepare well for your SSLC exams with Xylem Online Tuition. Learn your subjects easily and get ready to score better.

Register Now

Explanation of Equation

Mathematically, the second law of thermodynamics is represented as
ΔSuniv > 0
Where ΔSuniv is the change in the entropy of the universe.

Entropy

Entropy is defined as the measure of the randomness of the system, or it is the measure of energy within an isolated system. The concept was introduced by physicist Rudolf Clausius in 1865. The entropy of the universe only increases and never decreases. It can be considered as a quantitative index that describes the quality of energy.

Now let us consider two factors that cause an increase in the entropy of a closed system. 

  1. In a closed system, while the mass remains constant, there is an exchange of heat with the surroundings. This change in the heat content creates a disturbance in the system; hence, the entropy of the system increases.
  2. Internal changes may occur in the movements of the molecules of the system. This leads to disturbances that further cause irreversibilities inside the system, resulting in the increase of entropy. 

Thermodynamics

This law was developed by the German chemist Walther Nernst between the years 1906 and 1912.  It states that the entropy of a perfect crystal at a temperature of zero Kelvin (absolute zero) is equal to zero.

Entropy is denoted as ’S’; it is a measure of the disorder in a closed system. It is directly related to the number of microstates accessible to the system, which means the greater the number of microstates the closed system can occupy, the greater its entropy. The microstate in which the energy of the system is at its minimum is called the ground state of the system.

Mathematical Explanation of the Third Law

As per statistical mechanics, the entropy of a system can be expressed via the following equation:
S − S0 = kB lnΩ
Where,
• S is the entropy of the system.
• S0 is the initial entropy.
• kB denotes the Boltzmann constant.
• Ω refers to the total number of microstates that are consistent with the system’s macroscopic configuration.
Now, for a perfect crystal that has exactly one unique ground state, Ω = 1. Therefore, the equation can be rewritten as follows:
S − S0 = kB ln(1) = 0 [because ln(1) = 0]
When the initial entropy of the system is selected as zero, the following value of ‘S’ can be obtained:
S − 0 = 0 ⇒ S = 0
Thus, the entropy of a perfect crystal at absolute zero is 0.

Enthalpy (H)

 It is the total heat content of a system. It is considered the sum of internal energy and pressure-volume energy of a system, where

 H = U + pV

The unit of enthalpy is kJ/mol. It is a state function with an extensive property. So whenever there is a change in enthalpy, it depends on the initial and final values and not on the path followed. 

Thus, if H1 is the enthalpy of a system in the initial state,
H2 is the enthalpy in the final state, then the change in enthalpy is
ΔH = H2 − H1.
ΔH is determined by using an apparatus called a calorimeter.

The standard enthalpy of reaction

It is the enthalpy change for a reaction when all the substances are in their standard states. In thermodynamics, the standard state refers to the existence of a substance in its pure form at 1 bar pressure and 298 K temperature. 

Enthalpy of phase transition

 It is the enthalpy change when one mole of a substance changes from one phase to another phase at a particular temperature. The important types of Enthalpies of phase transition are of 3 types: 

1) Molar Enthalpy of fusion (ΔfusH°)
It is the enthalpy change when one mole of a solid substance changes to the liquid state at its melting point.
2) Molar Enthalpy of vaporization (ΔvapH°)
It is the enthalpy change when one mole of a liquid substance changes to its vapour state at its boiling point.
3) Molar Enthalpy of sublimation (ΔsubH°)
It is the enthalpy change when one mole of a solid substance is directly converted to the gaseous state at a particular temperature below its melting point.

Note:  Enthalpies of fusion, vaporization, and sublimation are positive, since heat is absorbed during these processes; the magnitude of the enthalpy change depends on the strength of the intermolecular forces in the substance.

Relation between ΔH and ΔU

Consider a gaseous reaction taking place at constant pressure (P) and temperature (T).
Let H1, U1 and V1 be the initial enthalpy, internal energy and volume, respectively. Let these values change to H2, U2, and V2
Such that, H1 = U1 + pV1   (eq.1)
H2 = U2 + pV2   (eq.2)
(2) − (1) gives: H2 − H1 = (U2 + pV2) − (U1 + pV1)
Or, ΔH = (U2 − U1) + (pV2 − pV1)
Or, ΔH = ΔU + p (V2 − V1)
Or, ΔH = ΔU + pΔV   (eq.3)
From the ideal gas equation, pV = nRT [where R is the universal gas constant, R = 8.314 J K−1 mol−1]. If n1 and n2 are the total no. of moles of reactants and products, respectively,
then pV1 = n1RT and pV2 = n2RT
pV2 − pV1 = n2RT − n1RT. Or, p(V2 − V1) = (n2 − n1)RT.
Or, pΔV = ΔnRT
So equation (3) becomes ΔH = ΔU + ΔnRT
where Δn = np(g) − nR(g)
Hence, Δn = No. of moles of gaseous products − No. of moles of gaseous reactants
If Δn = 0, then ΔH = ΔU
If Δn > 0, then ΔH > ΔU and if Δn < 0, then ΔH < ΔU.

Endothermic and Exothermic processes

Exothermic and endothermic processes are thermodynamic changes that describe how heat and energy move between a chemical system and its surroundings. Let’s learn more about it:

• A process that releases thermal energy from the system into the surroundings. If HP < HR, ΔH is negative and heat is evolved during the process. Such a process is called an exothermic process.
• A process that absorbs thermal energy from the surroundings into the system. For a chemical reaction, if HP is the enthalpy of products and HR is that of reactants, then ΔH = HP − HR. If HP > HR, ΔH is positive and heat is absorbed during the process. This is called an endothermic process.

Hess’s Law of Constant Heat Summation

 The law states that the total enthalpy change for a physical or chemical process is the same whether the reaction takes place in a single step or in several steps. 

Standard enthalpy of combustion (ΔcHΘ)

The total heat released when exactly one mole of a substance burns completely in excess oxygen under standard conditions. It is always negative since heat always evolves during combustion.

Enthalpy of atomization (ΔaHΘ)

 It is the enthalpy change on breaking one mole of bonds completely to obtain atoms in the gas phase. In the case of diatomic molecules, the enthalpy of atomization is the same as the bond dissociation enthalpy. 

Bond Enthalpy (ΔbondHΘ)

 A chemical reaction that involves the breaking and making of chemical bonds. Energy is required to break a bond, and energy is released when a bond is formed. So enthalpy of bond dissociation is positive, and enthalpy of bond formation is negative.

Bond dissociation enthalpy

The amount of heat required to break one mole of covalent bonds to form products in the gas phase is called the bond dissociation enthalpy. For diatomic molecules, bond dissociation enthalpy and bond enthalpy are the same. 

Heat capacity ( C)

It is the amount of heat required to raise the temperature of a body to 1°C or 1K. If q amount of heat is required to raise the temperature of a body through ΔT, then heat capacity (C) = q / ΔT. Heat capacity in Thermodynamics is categorised into two:
  1. Specific heat capacity(c) is the heat capacity for one unit of mass (usually 1 kg or 1g) of a substance. It is measured in J/(kg .K)
  2. Molar heat capacity (Cm)  is the amount of heat required to raise the temperature of 1 mole of a substance.It is measured in J/(mol. K) 

Gibbs Energy

Gibbs Energy (G) is a thermodynamic quantity that helps us predict whether a chemical or physical process can occur spontaneously at constant temperature and pressure. It combines the concepts of enthalpy (ΔH) and entropy (ΔS) into a single term that indicates the “useful energy” available to do work.
The change in Gibbs free energy is given by the formula:
ΔG = ΔH − TΔS
Where:
• ΔG = change in Gibbs free energy
• ΔH = change in enthalpy (heat absorbed or released)
• ΔS = change in entropy (disorder)
• T = absolute temperature in Kelvin

FAQ's

What is the First Law of Thermodynamics?

The First Law states that heat is a form of energy and follows the principle of conservation of energy.

What is the formula for enthalpy?

Enthalpy is given by H = U + PV, where U is internal energy, P is pressure, and V is volume.

What is the difference between endothermic and exothermic processes?

An endothermic process absorbs heat from the surroundings, whereas an exothermic process releases heat to the surroundings.

What is Hess’s Law of Constant Heat Summation?What is Hess’s Law of Constant Heat Summation?

Hess’s Law states that the total enthalpy change is the same whether a reaction occurs in a single step or in several steps.

What is the Second Law of Thermodynamics?

The Second Law states that the entropy of an isolated system always increases, and the entropy of the universe never decreases.

What is the standard enthalpy of combustion?

It is the total heat released when exactly one mole of a substance burns completely in excess oxygen under standard conditions.

Define the enthalpy of a reaction.

The enthalpy of a reaction is defined as the heat energy change that occurs when reactants become products. ΔH is positive if heat is absorbed during the reaction; if heat is released, ΔH is negative.

During the endothermic reaction, what type of energy conversion will take place?

This is the conversion of kinetic energy to chemical energy. Heat is absorbed and converted into chemical energy during an endothermic reaction.

What is the main difference between an exothermic and an endothermic process?

The main difference between exothermic and endothermic reactions is that an endothermic reaction absorbs energy in the form of heat from its surroundings, whereas an exothermic reaction releases energy to the surroundings

What is bond dissociation enthalpy?

Bond dissociation enthalpy is the amount of heat required to break one mole of covalent bonds and form products in the gas phase.

Blog Page Contact