1 Line-by-Line Walkthrough
Read each line, peek at the "Easy idea" for a friendly version, then move to the tables.
Thermodynamics is the branch of science that deals with energy changes accompanying physical and chemical transformations. It does not deal with rate or mechanism — only with the energy bookkeeping.
A thermodynamic system is the part of the universe under study; the rest is the surroundings. The boundary separates them. Systems are open (exchange both matter and energy), closed (energy only), or isolated (neither).
State of a system is defined by macroscopic properties like p, V, T and n. A state function depends only on the current state, not on how the system got there. Examples: U, H, S, G, T, P, V.
Path functions depend on the route taken between two states. The main examples are heat (q) and work (w). Different paths between the same two states give different q and w.
Internal energy U is the total energy stored inside a system — sum of all molecular kinetic and potential energies. It is a state function. For an ideal gas, U depends only on T.
First law of thermodynamics: energy can be neither created nor destroyed, only converted. Mathematically: ΔU = q + w. The change in internal energy equals heat added to the system plus work done on it.
Sign convention (IUPAC): q is positive if heat is absorbed BY system; negative if released. w is positive if work is done ON system; negative if done BY system. Compression ⇒ w > 0; expansion ⇒ w < 0.
Work of expansion against an external pressure: w = −pext · ΔV. For reversible isothermal expansion of an ideal gas: w = −nRT ln(V₂/V₁) — this gives maximum work.
Enthalpy H is defined as H = U + pV. For a process at constant pressure, ΔH equals heat absorbed: qp = ΔH. For constant volume: qv = ΔU. Relationship between them for gases: ΔH = ΔU + Δng · RT.
Heat capacity: C = q/ΔT. At constant volume: Cv = (∂U/∂T)V. At constant pressure: Cp = (∂H/∂T)p. For an ideal gas: Cp − Cv = R (Mayer's relation). For a monoatomic gas Cv = (3/2)R; diatomic ≈ (5/2)R.
Hess's law of constant heat summation: ΔH of a reaction is the same whether the reaction takes place in one step or several. This is a direct consequence of H being a state function. It allows calculation of ΔH for reactions that are difficult to measure directly.
Standard enthalpy changes: ΔH°_f (formation: 1 mole compound from elements in standard state), ΔH°_c (combustion in O₂), ΔH°_neut (acid + base → salt + water), ΔH°_sol (1 mole in large excess solvent). Standard state = 1 bar, specified T (usually 298 K).
Bond enthalpy is the average energy required to break one mole of a particular bond in a gas-phase molecule. ΔH of reaction ≈ Σ BE(bonds broken) − Σ BE(bonds formed). Useful estimate when calorimetric data is unavailable.
Spontaneous process is one that takes place by itself without outside help (e.g., water flowing downhill, heat flowing from hot to cold). Spontaneity is NOT about speed — only about direction.
Entropy S is a measure of disorder or number of microscopic arrangements. Boltzmann: S = kB · ln W. Second law: for a spontaneous process, ΔSuniverse > 0. Gas > liquid > solid in entropy.
Gibbs free energy G = H − TS. At constant T and p, the criterion for spontaneity is ΔG < 0. At equilibrium ΔG = 0. Relationship to equilibrium constant: ΔG° = −RT ln K = −2.303 RT log K.
Third law of thermodynamics: the entropy of a perfect crystalline substance is zero at absolute zero (0 K). This gives an absolute reference for entropy, unlike enthalpy (which only has relative values).
2 Concepts to know for NEET MCQs
| Concept | Key idea | NEET focus |
|---|---|---|
| System types | Open / closed / isolated | "Hot tea in open cup = ?" style MCQs |
| State vs path function | State: only start/end matter. Path: route matters | "Which is NOT a state function?" |
| Sign convention | q, w positive when heat/work flows INTO system (IUPAC) | Setting up first-law equations |
| First law ΔU = q + w | Energy conservation in any process | Calculating ΔU from q and w |
| Enthalpy H | H = U + pV; ΔH = qp | Heat of reaction at constant p |
| ΔH vs ΔU | ΔH = ΔU + Δng RT for gases | Common numerical pattern |
| Heat capacity | Cp − Cv = R for ideal gas; Cv depends on f | Adiabatic calculations |
| Hess's law | ΔH path-independent ⇒ can add/subtract steps | Indirect ΔH calculations |
| Bond enthalpy | ΔH ≈ Σ BE(broken) − Σ BE(formed) | Estimate ΔH from bond data |
| Spontaneity | ΔG < 0 at constant T, p | Predicting direction of change |
| Entropy | Measure of disorder; gas > liquid > solid | Sign of ΔS in given process |
| ΔG and K | ΔG° = −RT ln K | Connecting thermodynamics to equilibrium |
3 Formulas Bank
| Quantity / Process | Formula | Notes |
|---|---|---|
| First law | ΔU = q + w | IUPAC sign convention |
| Work (expansion/compression) | w = −pext · ΔV | Irreversible against constant pext |
| Reversible isothermal (ideal gas) | w = −nRT ln(V₂/V₁) = −nRT ln(p₁/p₂) | Maximum work |
| Heat at constant V | qv = ΔU = nCv ΔT | For ideal gas |
| Heat at constant p | qp = ΔH = nCp ΔT | For ideal gas |
| Enthalpy definition | H = U + pV | State function |
| ΔH vs ΔU for gases | ΔH = ΔU + Δng · R · T | Δng = mol gaseous products − mol gaseous reactants |
| Mayer's relation | Cp − Cv = R | Per mole, ideal gas |
| Adiabatic ideal gas | pV^γ = constant; TVγ−1 = constant | γ = Cp/Cv |
| Adiabatic work (ideal) | w = nCv(T₂ − T₁) = (p₁V₁ − p₂V₂)/(γ − 1) | q = 0 |
| Hess's law | ΔHoverall = Σ ΔHsteps | Path independent |
| Bond enthalpy | ΔHrxn = Σ BE(broken) − Σ BE(formed) | Estimate only |
| Entropy change (rev) | ΔS = qrev/T | For constant-T process |
| Phase change entropy | ΔSfus = ΔHfus/Tm; ΔSvap = ΔHvap/Tb | At constant T (mp or bp) |
| Boltzmann entropy | S = kB · ln W | W = microstates |
| Second law | ΔSuniv = ΔSsys + ΔSsurr ≥ 0 | > 0 for spontaneous |
| Gibbs energy | G = H − TS; ΔG = ΔH − TΔS | At constant T |
| Spontaneity (T, p) | ΔG < 0 ⇒ spontaneous; ΔG = 0 ⇒ equilibrium | The most important criterion |
| ΔG and K | ΔG° = −RT ln K = −2.303 RT log K | Connects thermo to equilibrium |
| ΔG and ΔG° | ΔG = ΔG° + RT ln Q | Q = reaction quotient |
| Carnot efficiency | η = 1 − Tcold/Thot | Best possible heat engine |
4 Facts you must remember
| Fact | Why it matters for NEET |
|---|---|
| For an ideal gas, U depends only on T | Isothermal ΔU = 0; free expansion ΔT = 0 |
| Standard state: 1 bar pressure, specified T (usually 298 K) | Definition trap in PYQs |
| ΔH°_f of element in standard state = 0 | Reference point for all formation enthalpies |
| Enthalpy of neutralisation of strong acid + strong base ≈ −57.1 kJ/mol | Standard NEET fact |
| Heat of fusion of ice = 6.01 kJ/mol; vaporisation of water = 40.66 kJ/mol | Phase-change PYQ fodder |
| For 1 mole gas: Cp − Cv = R | Used in nearly every adiabatic problem |
| Monoatomic: Cv = (3/2)R, γ = 5/3; Diatomic: Cv ≈ (5/2)R, γ = 7/5 | Common gas-property questions |
| For cyclic process: ΔU = ΔH = ΔG = ΔS = 0 | Identify path/state function quickly |
| Free expansion of ideal gas into vacuum: q = w = ΔU = 0 | Classic conceptual MCQ |
| Trouton's rule: ΔSvap ≈ 88 J/(K·mol) for normal liquids | Approximation question |
| Born-Haber cycle is used to find lattice enthalpy | Definition question |
| Carnot efficiency: η = 1 − Tc/Th; only depends on temperatures | Engine problems |
5 Controversial / Confusing Points
| Confusion | Clarification |
|---|---|
| "Sign convention for w" | IUPAC: w > 0 when work done ON system. Older convention: w > 0 when work done BY system. NEET uses IUPAC ⇒ wcompression > 0, wexpansion < 0. |
| "ΔH vs ΔU — when are they equal?" | For reactions with no change in moles of gas (Δng = 0). Also for purely solid/liquid reactions. |
| "Is q a state function?" | No. q and w are path functions. But qp = ΔH and qv = ΔU are special cases where heat equals a state function. |
| "Spontaneous = fast?" | No! Spontaneity says nothing about rate. Diamond → graphite is spontaneous but unimaginably slow. |
| "ΔG < 0 always means it will happen?" | Only that it's thermodynamically allowed. Activation energy may make it kinetically frozen. |
| "ΔSsystem can be negative even for spontaneous process?" | Yes — as long as ΔSuniverse (= ΔSsys + ΔSsurr) is positive. Water freezing below 0 °C: ΔSsys < 0 but ΔSsurr more positive. |
| "ΔG° vs ΔG" | ΔG° is under standard conditions (1 bar, 298 K). ΔG is under actual conditions. Related by ΔG = ΔG° + RT ln Q. |
| "At equilibrium ΔG = 0 but ΔG° ≠ 0" | ΔG = 0 at the actual equilibrium state. ΔG° = −RT ln K can be positive, negative or zero depending on K. |
6 Assumptions in this chapter
| Assumption | When it's invoked |
|---|---|
| Gas behaves ideally (pV = nRT) | All ideal-gas calculations (work, ΔU, ΔH) |
| For an ideal gas, U depends only on T | Used to set ΔU = 0 in isothermal processes |
| Reversible processes are infinitely slow (quasi-static) | Maximum-work derivations |
| Adiabatic means perfectly insulated (q = 0) | All adiabatic equations |
| Standard state is at 1 bar pressure (and specified T) | All standard ΔH°, ΔG° values |
| Bond enthalpies are averages over many molecules | Bond-enthalpy estimates of ΔH |
| Heat capacities Cp, Cv are independent of T | Simple integration of heat capacity |
| Perfect crystal exists at 0 K (third law) | Absolute entropy reference |
| Surroundings are effectively infinite at constant T | ΔSsurr = −qsys/T well-defined |
7 Exceptions to remember
| General rule | Exception |
|---|---|
| ΔH and ΔU are equal | Only when Δng = 0 (no change in moles of gas). Otherwise they differ by Δng RT. |
| For real gases, U = U(T) only | False for real gases — U depends on V too (only ideal gases have U = U(T)). |
| Free expansion is always isothermal | True for ideal gas only. Real gases cool slightly (Joule-Thomson effect). |
| Joule-Thomson coefficient is non-zero | Zero for ideal gas — H depends only on T, so no cooling on throttling. |
| Bond-enthalpy ΔH equals true reaction ΔH | Only an average estimate; actual values can deviate by 10–20 kJ/mol. |
| Trouton's rule applies to all liquids | Fails for H-bonded liquids (water, ethanol) due to abnormal structure in liquid. |
| For elements ΔH°_f = 0 | Only for standard state. Diamond ΔH°_f ≠ 0 because graphite is the standard form of carbon. |
| ΔS positive ⇒ spontaneous | True only when also considering ΔSuniverse. ΔSsystem alone is insufficient. |
| Third law: S = 0 at 0 K | Holds only for perfect crystals. Glassy/amorphous solids have residual entropy at 0 K. |
8 Scientists and years
| Scientist | Year | Contribution |
|---|---|---|
| Germain Henri Hess | 1840 | Hess's law of constant heat summation |
| James Prescott Joule | 1843–1850 | Mechanical equivalent of heat; conservation of energy |
| Rudolf Clausius | 1850, 1865 | Formulated first and second laws; coined the word entropy |
| William Thomson (Lord Kelvin) | 1851 | Absolute temperature scale; alternative statement of second law |
| Sadi Carnot | 1824 | Theoretical maximum efficiency of heat engines (Carnot cycle) |
| Hermann von Helmholtz | 1882 | Helmholtz free energy; A = U − TS |
| Josiah Willard Gibbs | 1873–1878 | Gibbs free energy G = H − TS; criterion for spontaneity |
| Ludwig Boltzmann | 1877 | Statistical definition of entropy: S = kB ln W |
| Walther Nernst | 1906 | Third law of thermodynamics (Nernst heat theorem) |
| James Joule & William Thomson | 1852 | Joule-Thomson effect (real-gas cooling on expansion) |
9 NEET traps to avoid
| Trap | How to avoid it |
|---|---|
| Mixing up sign conventions for w | NEET uses IUPAC. Heat IN, work IN ⇒ positive. wexpansion is negative. |
| Forgetting Δng in ΔH−ΔU | Always check whether moles of gas change. If only solids/liquids: ΔH ≈ ΔU. |
| Claiming ΔSsys > 0 ⇒ spontaneous | You need ΔSuniverse > 0. Or at const T, p use ΔG < 0. |
| Calling ΔG° = 0 at equilibrium | ΔG = 0 at equilibrium. ΔG° = −RT ln K which is generally non-zero. |
| Heat of formation = heat of combustion? | True only for H₂O(l) from H₂(g) and ½O₂(g). Not general. |
| "Spontaneous = fast" misconception | Spontaneity says nothing about rate. ΔG < 0 only means thermodynamically allowed. |
| Cyclic process gives non-zero ΔH | Cyclic ⇒ ΔX = 0 for any state function X. Heat and work can still be non-zero. |
| Adiabatic always means temperature constant | No — adiabatic means no heat exchange. Temperature usually changes. |
| Free expansion of ideal gas reduces T | For ideal gas, T is unchanged in free expansion (Joule expansion). |
| Negative ΔG means K < 1 | Opposite: ΔG° < 0 ⇒ K > 1 (products favoured). |
📊 Diagrams
a) Types of thermodynamic systems
Open exchanges matter and energy; closed exchanges only energy; isolated exchanges neither.
b) First law and sign convention
Energy flowing INTO the system (q, w) is taken as positive (IUPAC convention).
c) p–V curves for key processes
Isothermal (solid) is shallower; adiabatic (dashed) is steeper since γ > 1.
d) Enthalpy diagram for an exothermic reaction
Products sit lower in enthalpy than reactants ⇒ ΔH negative.
e) Spontaneity zones (ΔG = ΔH − TΔS)
Four quadrants depending on signs of ΔH and ΔS. Two are temperature-dependent.
f) Hess's law cycle
Direct ΔH equals the sum of step-wise ΔH values along any alternate path.
📝 50 PYQs — 25 NEET + 25 JEE Main
Each card shows a question-specific Easy idea, then Given / To find / Formula / Solution / Answer.