Thermodynamics

Chemistry
NEET UG
Version 1Updated 22 Mar 2026

Thermodynamics, derived from Greek words 'therme' (heat) and 'dynamis' (power), is a branch of physical chemistry that deals with the quantitative relationships between heat and other forms of energy. It provides a framework to understand energy transformations in physical and chemical processes, predicting the feasibility and direction of reactions without considering their rates. At its core, th…

Quick Summary

Thermodynamics is the study of energy transformations, particularly involving heat and work. It defines a 'system' (the part of the universe under study) and 'surroundings' (everything else), separated by a boundary.

Systems can be open (exchange matter and energy), closed (exchange energy only), or isolated (no exchange). Key properties are either extensive (depend on amount, like volume) or intensive (independent of amount, like temperature).

State functions (e.g., internal energy, enthalpy, entropy, Gibbs free energy) depend only on the initial and final states, while path functions (heat, work) depend on the process path. The First Law states energy conservation: ΔU=Q+W\Delta U = Q + W.

The Second Law introduces entropy (disorder) and predicts spontaneity: ΔStotal>0\Delta S_{total} > 0 for spontaneous processes. Gibbs free energy (ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S) is the practical criterion for spontaneity at constant T and P.

The Third Law defines zero entropy at absolute zero for perfect crystals. Understanding these laws and concepts is fundamental for predicting chemical and physical changes.

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Key Concepts

First Law of Thermodynamics (Energy Conservation)

The First Law states that energy cannot be created or destroyed, only converted from one form to another. For…

Spontaneity and Gibbs Free Energy

Spontaneity refers to whether a process will occur on its own without continuous external intervention. The…

Relationship between ΔH\Delta H and ΔU\Delta U

Enthalpy (H) is defined as H=U+PVH = U + PV. For a chemical reaction or physical change occurring at constant…

  • First LawΔU=Q+W\Delta U = Q + W (Energy Conservation) \n- Work (Constant P): W=PextΔVW = -P_{ext}\Delta V \n- Work (Reversible Isothermal): Wrev=nRTln(V2/V1)W_{rev} = -nRT \ln(V_2/V_1) \n- Enthalpy: H=U+PVH = U + PV, ΔH=ΔU+ΔngRT\Delta H = \Delta U + \Delta n_g RT \n- Second Law: ΔStotal>0\Delta S_{total} > 0 (Spontaneous) \n- Entropy Change: ΔS=Qrev/T\Delta S = Q_{rev}/T \n- Gibbs Free Energy: ΔG=ΔHTΔS\Delta G = \Delta H - T\Delta S \n- Spontaneity: ΔG<0\Delta G < 0 (Spontaneous), ΔG=0\Delta G = 0 (Equilibrium), ΔG>0\Delta G > 0 (Non-spontaneous) \n- Equilibrium Constant: ΔG=RTlnK\Delta G^\circ = -RT \ln K \n- Third Law: S=0S = 0 at 0,K0,\text{K} for perfect crystal \n- Sign Conventions: Q (+ve absorbed, -ve released); W (+ve on system, -ve by system)

To remember the spontaneity conditions based on ΔH\Delta H and ΔS\Delta S: \n\n'Happy Students Get To Succeed' \nΔH\Delta H (Happy) and ΔS\Delta S (Students) determine ΔG\Delta G (Get) at Temperature (To) for Spontaneity (Succeed).

\n\n* H-ve, S+ve: Always spontaneous (Happy, Succeed). \n* H+ve, S-ve: Never spontaneous (Sad, Fail). \n* H-ve, S-ve: Spontaneous at Low T (Happy, but messy, so needs cool head). \n* H+ve, S+ve: Spontaneous at High T (Needs energy, but loves freedom, so needs hot environment).

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