Chemical Thermodynamics

ЁЯПл MP BoardClass 11Chemistry

ЁЯУР Formula & Cheat Sheet (English)

MP Board Class 11 Chemistry: Chemical Thermodynamics

Quick Revision Notes & Formula Sheet


1. Basic Terms & Definitions (рдореВрд▓ рдЕрд╡рдзрд╛рд░рдгрд╛рдПрдВ)

  • System (рдирд┐рдХрд╛рдп): The part of the universe under thermodynamic study.

  • Surroundings (рдкрд░рд┐рд╡реЗрд╢): Everything outside the system that can interact with it. $$\text{Universe} = \text{System} + \text{Surroundings}$$

  • Types of Systems:

    1. Open System: Exchanges both matter and energy with surroundings (e.g., hot tea in an open beaker).
    2. Closed System: Exchanges energy but NOT matter (e.g., hot tea in a closed metal vessel).
    3. Isolated System: Exchanges NEITHER matter NOR energy (e.g., hot tea in a thermos flask).
  • State Functions: Properties that depend only on the current state of the system, not on the path taken (e.g., $P, V, T, U, H, S, G$).

  • Path Functions: Properties that depend on the path taken to achieve a state (e.g., Heat ($q$), Work ($w$)).

  • Extensive Properties: Depend on the amount of matter present (e.g., Mass, Volume, Internal Energy, Enthalpy, Entropy).

  • Intensive Properties: Independent of the amount of matter present (e.g., Temperature, Pressure, Density, Specific Heat, Molar Volume).


2. First Law of Thermodynamics (рдКрд╖реНрдорд╛рдЧрддрд┐рдХреА рдХрд╛ рдкреНрд░рдердо рдирд┐рдпрдо)

Energy can neither be created nor destroyed; it can only be converted from one form to another (Law of Conservation of Energy).

$$\Delta U = q + w$$

Where:

  • $\Delta U$ = Change in internal energy (рдЖрдВрддрд░рд┐рдХ рдКрд░реНрдЬрд╛ рдореЗрдВ рдкрд░рд┐рд╡рд░реНрддрди)
  • $q$ = Heat supplied to system
  • $w$ = Work done on system

IUPAC Sign Conventions:

  • $q > 0$ (+ve): Heat absorbed by the system.
  • $q < 0$ (-ve): Heat released by the system.
  • $w > 0$ (+ve): Work done on the system (Compression / рд╕рдВрдкреАрдбрди).
  • $w < 0$ (-ve): Work done by the system (Expansion / рдкреНрд░рд╕рд╛рд░).

3. Work Done Formulas (рдХрд╛рд░реНрдп рдХреЗ рд╕реВрддреНрд░)

General Pressure-Volume Work:

$$w = - P_{\text{ext}} \cdot \Delta V = - P_{\text{ext}} (V_2 - V_1)$$

1. Reversible Isothermal Process ($T = \text{constant}$):

$$w_{\text{rev}} = - 2.303 \cdot n R T \cdot \log_{10}\left(\frac{V_2}{V_1}\right)$$ OR $$w_{\text{rev}} = - 2.303 \cdot n R T \cdot \log_{10}\left(\frac{P_1}{P_2}\right)$$

2. Irreversible Isothermal Process:

$$w_{\text{irrev}} = - P_{\text{ext}} (V_2 - V_1)$$

3. Free Expansion (Expansion in vacuum, $P_{\text{ext}} = 0$):

$$w = 0$$

4. Isochoric Process ($\Delta V = 0$):

$$w = 0 \implies \Delta U = q_v$$

5. Adiabatic Process ($q = 0$):

$$\Delta U = w_{\text{ad}}$$


4. Enthalpy ($H$) & Internal Energy ($U$)

  • Enthalpy Definition: $H = U + P V$

  • Enthalpy Change at Constant Pressure: $$\Delta H = \Delta U + P \Delta V$$ $$\Delta H = q_p$$

  • Relationship between $\Delta H$ and $\Delta U$ for Gaseous Reactions: $$\Delta H = \Delta U + \Delta n_g R T$$

    Where:

    • $\Delta n_g = (\text{Moles of gaseous products}) - (\text{Moles of gaseous reactants})$
    • $R = 8.314 \text{ J K}^{-1} \text{mol}^{-1}$
  • Exothermic Reaction (рдКрд╖реНрдорд╛рдХреНрд╖реЗрдкреА): Heat released, $\Delta H < 0$ (-ve)

  • Endothermic Reaction (рдКрд╖реНрдорд╛рд╢реЛрд╖реА): Heat absorbed, $\Delta H > 0$ (+ve)


5. Heat Capacities (рдКрд╖реНрдорд╛ рдзрд╛рд░рд┐рддрд╛)

  • Heat Capacity ($C$): Amount of heat required to raise the temperature of a system by $1^\circ\text{C}$ or $1\text{ K}$. $$C = \frac{q}{\Delta T}$$

  • Specific Heat Capacity ($c$): Heat required per unit mass ($1\text{ g}$). $$c = \frac{q}{m \cdot \Delta T}$$

  • Molar Heat Capacity ($C_m$): Heat required per mole ($1\text{ mol}$). $$C_m = \frac{q}{n \cdot \Delta T}$$

  • Heat Capacity at Constant Volume ($C_v$): $$C_v = \left(\frac{\Delta U}{\Delta T}\right)_v$$

  • Heat Capacity at Constant Pressure ($C_p$): $$C_p = \left(\frac{\Delta H}{\Delta T}\right)_p$$

  • Mayer's Relation (for ideal gas): $$C_p - C_v = R$$

  • Poisson's Ratio ($\gamma$): $$\gamma = \frac{C_p}{C_v}$$ (Monoatomic = 1.66, Diatomic = 1.40, Triatomic = 1.33)


6. Thermochemistry (рдКрд╖реНрдорд╛ рд░рд╕рд╛рдпрди)

Hess's Law of Constant Heat Summation:

The total enthalpy change in a chemical reaction is the same regardless of whether the reaction takes place in one step or in several steps.

$$\Delta H = \Delta H_1 + \Delta H_2 + \Delta H_3 + \dots$$

Important Enthalpies of Reaction:

  1. Standard Enthalpy of Formation ($\Delta_f H^\circ$): Enthalpy change when 1 mole of a substance is formed from its elements in their standard state.

    • Note: $\Delta_f H^\circ$ of pure elements in standard state = $0$ (e.g., $O_{2(g)}, C_{\text{graphite}}, Fe_{(s)}$).
  2. Enthalpy of Reaction from Enthalpy of Formation: $$\Delta_r H^\circ = \sum \Delta_f H^\circ (\text{Products}) - \sum \Delta_f H^\circ (\text{Reactants})$$

  3. Enthalpy of Reaction from Bond Enthalpies: $$\Delta_r H^\circ = \sum \text{Bond Enthalpy (Reactants)} - \sum \text{Bond Enthalpy (Products)}$$


7. Second Law of Thermodynamics & Entropy ($S$)

  • Entropy ($S$): Measure of randomness or degree of disorder in a system.

    • State function, Extensive property.
    • Units: $\text{J K}^{-1} \text{mol}^{-1}$
  • Entropy Change Formula: $$\Delta S = \frac{q_{\text{rev}}}{T}$$

  • Total Entropy Change ($\Delta S_{\text{total}}$): $$\Delta S_{\text{total}} = \Delta S_{\text{system}} + \Delta S_{\text{surroundings}}$$

  • Second Law Statement:

    • For a spontaneous (natural) process, total entropy of universe always increases: $$\Delta S_{\text{total}} > 0 \quad (\text{Spontaneous})$$ $$\Delta S_{\text{total}} = 0 \quad (\text{Equilibrium})$$ $$\Delta S_{\text{total}} < 0 \quad (\text{Non-spontaneous})$$
  • Order of Entropy: $\text{Gas} > \text{Liquid} > \text{Solid}$


8. Gibbs Free Energy ($G$) & Spontaneity

  • Gibbs Energy Definition: $G = H - T S$
  • Gibbs-Helmholtz Equation: $$\Delta G = \Delta H - T \Delta S$$

Criteria for Spontaneity (at Constant $T$ and $P$):

$\Delta G$ ValueNature of Process
$\Delta G < 0$ (-ve)Spontaneous (рд╕реНрд╡рддрдГ рдкреНрд░рд╡рд░реНрддрд┐рдд)
$\Delta G = 0$Equilibrium (рд╕рд╛рдореНрдпрд╛рд╡рд╕реНрдерд╛)
$\Delta G > 0$ (+ve)Non-spontaneous (рд╕реНрд╡рддрдГ рдЕрдкреНрд░рд╡рд░реНрддрд┐рдд)

Temperature Dependence on Spontaneity:

$\Delta H$$\Delta S$$\Delta G = \Delta H - T\Delta S$Spontaneity Condition
-+Always -Spontaneous at all temperatures
+-Always +Non-spontaneous at all temperatures
--- (at low $T$)Spontaneous at low temperatures
++- (at high $T$)Spontaneous at high temperatures

9. Gibbs Energy & Equilibrium Constant

Relationship between Standard Gibbs Free Energy Change ($\Delta G^\circ$) and Equilibrium Constant ($K$):

$$\Delta G^\circ = - R T \ln K$$ $$\Delta G^\circ = - 2.303 \cdot R T \cdot \log_{10} K$$

Where:

  • $R = 8.314 \text{ J K}^{-1} \text{mol}^{-1}$
  • $T$ = Temperature in Kelvin
  • $K$ = Equilibrium Constant ($K_c$ or $K_p$)

10. Third Law of Thermodynamics (рддреГрддреАрдп рдирд┐рдпрдо)

  • Statement: The entropy of a perfectly crystalline substance approaches zero as the absolute temperature approaches zero ($0\text{ K}$).

$$\lim_{T \to 0} S = 0$$

  • Application: Helps in calculating absolute values of entropy ($S$) of pure substances at any temperature.

ЁЯТб Quick Memory Trick & Important Units

  • 1 Calorie = $4.184 \text{ Joules}$
  • 1 L-atm = $101.3 \text{ Joules}$
  • Universal Gas Constant ($R$):
    • $R = 8.314 \text{ J K}^{-1} \text{mol}^{-1}$
    • $R = 0.0821 \text{ L atm K}^{-1} \text{mol}^{-1}$
    • $R = 2 \text{ cal K}^{-1} \text{mol}^{-1}$