Chemical Thermodynamics
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)
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System (рдирд┐рдХрд╛рдп): The part of the universe under thermodynamic study.
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Surroundings (рдкрд░рд┐рд╡реЗрд╢): Everything outside the system that can interact with it. $$\text{Universe} = \text{System} + \text{Surroundings}$$
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Types of Systems:
- Open System: Exchanges both matter and energy with surroundings (e.g., hot tea in an open beaker).
- Closed System: Exchanges energy but NOT matter (e.g., hot tea in a closed metal vessel).
- Isolated System: Exchanges NEITHER matter NOR energy (e.g., hot tea in a thermos flask).
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State Functions: Properties that depend only on the current state of the system, not on the path taken (e.g., $P, V, T, U, H, S, G$).
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Path Functions: Properties that depend on the path taken to achieve a state (e.g., Heat ($q$), Work ($w$)).
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Extensive Properties: Depend on the amount of matter present (e.g., Mass, Volume, Internal Energy, Enthalpy, Entropy).
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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 ($U$)
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Enthalpy Definition: $H = U + P V$
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Enthalpy Change at Constant Pressure: $$\Delta H = \Delta U + P \Delta V$$ $$\Delta H = q_p$$
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Relationship between $\Delta H$ and $\Delta U$ for Gaseous Reactions: $$\Delta H = \Delta U + \Delta n_g R T$$
Where:
- $\Delta n_g = (\text{Moles of gaseous products}) - (\text{Moles of gaseous reactants})$
- $R = 8.314 \text{ J K}^{-1} \text{mol}^{-1}$
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Exothermic Reaction (рдКрд╖реНрдорд╛рдХреНрд╖реЗрдкреА): Heat released, $\Delta H < 0$ (-ve)
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Endothermic Reaction (рдКрд╖реНрдорд╛рд╢реЛрд╖реА): Heat absorbed, $\Delta H > 0$ (+ve)
5. Heat Capacities (рдКрд╖реНрдорд╛ рдзрд╛рд░рд┐рддрд╛)
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Heat Capacity ($C$): Amount of heat required to raise the temperature of a system by $1^\circ\text{C}$ or $1\text{ K}$. $$C = \frac{q}{\Delta T}$$
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Specific Heat Capacity ($c$): Heat required per unit mass ($1\text{ g}$). $$c = \frac{q}{m \cdot \Delta T}$$
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Molar Heat Capacity ($C_m$): Heat required per mole ($1\text{ mol}$). $$C_m = \frac{q}{n \cdot \Delta T}$$
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Heat Capacity at Constant Volume ($C_v$): $$C_v = \left(\frac{\Delta U}{\Delta T}\right)_v$$
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Heat Capacity at Constant Pressure ($C_p$): $$C_p = \left(\frac{\Delta H}{\Delta T}\right)_p$$
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Mayer's Relation (for ideal gas): $$C_p - C_v = R$$
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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:
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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., $O_{2(g)}, C_{\text{graphite}}, Fe_{(s)}$).
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Enthalpy of Reaction from Enthalpy of Formation: $$\Delta_r H^\circ = \sum \Delta_f H^\circ (\text{Products}) - \sum \Delta_f H^\circ (\text{Reactants})$$
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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 ($S$)
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Entropy ($S$): Measure of randomness or degree of disorder in a system.
- State function, Extensive property.
- Units: $\text{J K}^{-1} \text{mol}^{-1}$
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Entropy Change Formula: $$\Delta S = \frac{q_{\text{rev}}}{T}$$
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Total Entropy Change ($\Delta S_{\text{total}}$): $$\Delta S_{\text{total}} = \Delta S_{\text{system}} + \Delta S_{\text{surroundings}}$$
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Second Law Statement:
- For a spontaneous (natural) process, total entropy of universe always increases: $$\Delta S_{\text{total}} > 0 \quad (\text{Spontaneous})$$ $$\Delta S_{\text{total}} = 0 \quad (\text{Equilibrium})$$ $$\Delta S_{\text{total}} < 0 \quad (\text{Non-spontaneous})$$
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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 $P$):
| $\Delta G$ Value | Nature 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 ($R$):
- $R = 8.314 \text{ J K}^{-1} \text{mol}^{-1}$
- $R = 0.0821 \text{ L atm K}^{-1} \text{mol}^{-1}$
- $R = 2 \text{ cal K}^{-1} \text{mol}^{-1}$