Definitions [12]
The remaining part of the universe without the system is called the surroundings.
A system, in thermodynamics, refers to that part of the universe in which observations are made.
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.
Define enthalpy.
Enthalpy of a system is sum of internal energy of a system and the energy equivalent to PV work.
H = U + PV
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)
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.
It is the enthalpy change when one mole of it dissolves in a specified amount of solvent
It is the enthalpy change associated with diluting a component in a solution at constant pressure and temperature.
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.
The total heat content of a system at constant pressure is known as enthalpу.
At constant pressure: ΔH = qp (heat exchanged at constant pressure).
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”.
Formulae [1]
\[\Delta_rH^\circ=\sum\Delta_fH_{(products)}^\circ-\sum\Delta_fH_{(reactants)}^\circ\]
Theorems and Laws [2]
State and explain Hess’s law of constant heat summation.
The law states that, “Overall, the enthalpy change for a reaction is equal to the sum of enthalpy changes of individual steps in the reaction”.
The enthalpy change for a chemical reaction is the same regardless of the pathway taken during the reaction. Hess’s law is a direct result of the principle that enthalpy is a state function. The enthalpy change of a reaction depends only upon the initial and final states, independent of the reaction path.
To determine the overall reaction equation, the reactants and products from the different steps are combined or subtracted as algebraic entities.
Consider the synthesis of NH3:
i. \[\ce{\phantom{...}2H2_{(g)} + N2_{(g)} -> N2H4_{(g)}, \Delta_rH^0_1 = +95.4 kJ}\]
ii. \[\ce{N2H4_{(g)} + H2_{(g)} -> 2NH3_{(g)}, \Delta_rH^0_2 = -187.6 kJ}\]
_______________________________________________
\[\ce{\phantom{.....}3H2_{(g)} + N2_{(g)} -> 2NH3_{(g)}}\], ΔrH0 = −92.2 kJ
The sum of the enthalpy changes for steps (i) and (ii) is equal to the enthalpy change for the overall reaction.
Statement: If a reaction takes place in several steps, its standard reaction enthalpy is equal to the sum of the standard enthalpies of all the intermediate steps into which the overall reaction can be divided, at the same temperature.
Note: Since enthalpy is a state function, the total enthalpy change is independent of the pathway — only the initial and final states matter.
Application:
\[\Delta_rH^\circ=\Delta_rH_1^\circ+\Delta_rH_2^\circ+\Delta_rH_3^\circ+\ldots\]
Key Points
| Type of System | Description |
|---|---|
| Open System | Can exchange both matter and energy with the surroundings. |
| Closed System | Can exchange only energy (not matter) with the surroundings. |
| Isolated System | Can neither exchange matter nor energy with the surroundings. |
The state of a system is described by its measurable macroscopic properties, such as temperature (T), pressure (P), volume (V), and amount of substance (n).
State Variables / State Functions:
- Properties whose values depend only on the current state of the system, not on how that state was reached.
- Examples: T, P, V, U (internal energy), H (enthalpy), S (entropy), G (Gibbs energy)
Non-State Functions (Path Functions):
- Their values depend on the path followed
- Examples: Work (W), Heat (q)
Note: Enthalpy (H = U + PV) and Gibbs energy (G = H − TS) are state functions. Work (W) and heat (q) are path functions.
- Enthalpy change when 1 mole of a compound is formed from its constituent elements in their standard states.
- Standard enthalpy of formation of elements in their most stable form = zero (e.g., graphite, not diamond, for carbon).
- Δf H∘ can be positive or negative.
Thermochemical Equations: Balanced equations that include the physical states and the enthalpy change. Example:
| Type | Symbol | Definition |
|---|---|---|
| Enthalpy of Fusion | ΔfusH | Enthalpy change when 1 mole solid → liquid at melting point |
| Enthalpy of Vaporisation | ΔvapH | Enthalpy change when 1 mole liquid → vapour at boiling point |
| Enthalpy of Sublimation | ΔsubH | Enthalpy change when 1 mole solid → vapour at constant T and P |
| Enthalpy of Ionisation | ΔionH | Enthalpy change accompanying the removal of an electron from 1 mole of gaseous atoms |
| Enthalpy of Atomisation | ΔatomH | Enthalpy change accompanying the dissociation of 1 mole of a gaseous substance into atoms |
Entropy (ΔS) is a thermodynamic property that measures the degree of randomness, disorder, or energy dispersal in a system. Higher entropy means greater disorder.
- For any process, the total entropy change is given by:
ΔStotal = ΔSsystem + ΔSsurroundings - A process is spontaneous if the total entropy of the universe increases, i.e., ΔStotal > 0
- If ΔStotal < 0, the process is non-spontaneous and cannot occur on its own.
- At equilibrium, there is no net change, so ΔSₜₒₜₐₗ = 0
- Processes such as melting, vaporisation, or mixing generally increase entropy and are therefore more likely to be spontaneous.
Entropy is influenced by:
- Physical state (gas > liquid > solid)
- Number of particles
- Temperature (higher T → higher disorder)
Gibbs free energy (ΔG) is a thermodynamic quantity that determines spontaneity at constant temperature and pressure.
It is defined as: ΔG = ΔH − TΔS,
where ΔH = enthalpy change, T = temperature, and ΔS = entropy change.
- A process is spontaneous when ΔG < 0 because free energy is released.
- If ΔG > 0, the process is non-spontaneous and requires external energy.
- At equilibrium, ΔG = 0 and no net change occurs in the system.
Temperature plays a key role when ΔH and ΔS have the same sign:
- ΔH < 0 and ΔS > 0 → always spontaneous
- ΔH > 0 and ΔS < 0 → never spontaneous
- ΔH < 0 and ΔS < 0 → spontaneous at low T
- ΔH > 0 and ΔS > 0 → spontaneous at high T
Gibbs free energy combines both enthalpy (heat changes) and entropy (disorder), making it a more practical criterion than entropy alone.
Relationship between ΔG° and equilibrium constant K:
Interpretation:
- If K > 1 → ΔG° < 0 → forward reaction favoured
- If K < 1 → ΔG° > 0 → reverse reaction favoured
- If K = 1 → ΔG° = 0 → equilibrium
At equilibrium: ΔG = 0 (not ΔG°)
Concepts [19]
- Thermodynamic Terms
- The State of the System
- The Internal Energy as a State Function - Work
- The Internal Energy as a State Function - Heat
- The Internal Energy as a State Function - the General Case
- Work
- Enthalpy (H)
- Calorimetric Measurement of ΔU and ΔH
- Standard Enthalpy of Reactions
- Enthalpy Changes During Phase Transformations
- Standard Enthalpy of Formation
- Thermochemical Equations
- Hess’ Law of Constant Heat Summation
- Is Decrease in Enthalpy a Criterion for Spontaneity
- Entropy and Spontaneity
- Gibbs Energy and Spontaneity
- Entropy and Second Law of Thermodynamics
- Absolute Entropy and Third Law of Thermodynamics
- Gibbs Energy Change and Equilibrium
