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Thermodynamics and Thermochemistry

NEET > Chemistry > Chemical Thermodynamics

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Overview content

Chapter Snapshot - Thermodynamics and Thermochemistry

The most conceptually layered chapter in physical chemistry, covering every law and function that governs energy transfer in chemical systems. Three laws of thermodynamics, internal energy and enthalpy, heat capacity (Cp vs Cv), PV work for isothermal and adiabatic processes, Joule-Thomson effect, ten types of heats of reaction, Hess's law with Born-Haber cycle, Carnot cycle efficiency, entropy, Gibbs free energy with spontaneity criteria, and the third law form the backbone. NEET draws 2 to 3 questions reliably, covering Hess's law numericals, delta-G spontaneity, and enthalpy of formation or combustion calculations.

āœ“ Use This To Plan Your First 2–3 Hours
Expected Questions (Typical)
Q
2-3
NEET consistently draws 2 to 3 questions: one on enthalpy calculations (Hess's law, bond energy, or heat of formation/combustion), one on Gibbs free energy and spontaneity criteria (delta-G sign analysis), and occasionally one on first law or entropy concepts.
Time Required (Practical)
ā±
14-16 hrs
Thermodynamic terms and system types 1 hr; internal energy and first law 2 hrs; enthalpy and heat capacity with Cp-Cv relations 2 hrs; PV work (isothermal and adiabatic) 2 hrs; thermochemistry with ten heat types 3 hrs; Hess's law and Born-Haber cycle 2 hrs; entropy, Gibbs free energy, and spontaneity 2 hrs; MCQ practice 2 hrs.
Difficulty Level
⚔
Moderate-High
The chapter has many formulas but only a subset is heavily tested. The main difficulty lies in the Gibbs-Helmholtz equation (delta-G = delta-H minus T delta-S) where students must handle sign combinations for four cases of spontaneity. Hess's law numericals require careful sign management when reversing equations.
Most Asked Style: Numerical MCQ: calculate delta-H using Hess's law or bond energies; determine spontaneity from delta-H and delta-S signs at a given temperature; calculate work done in isothermal reversible expansion; identify the correct Born-Haber cycle step.Biggest Trap: Confusing the sign convention for work. In chemistry, w = -P(ext) delta-V (work done BY system is negative). In physics, w = +P delta-V. NEET chemistry uses the chemistry convention. Mixing the physics sign gives the opposite sign for work and consequently wrong delta-E.Fast Win: Memorise the four spontaneity cases from the Gibbs equation: (1) delta-H negative and delta-S positive means spontaneous at all temperatures; (2) delta-H positive and delta-S negative means non-spontaneous at all temperatures; (3) delta-H negative and delta-S negative means spontaneous at low T; (4) delta-H positive and delta-S positive means spontaneous at high T. One question per NEET paper comes from this table.Revision-Friendly: High. The Gibbs four-case table, Cp - Cv = R, and Hess's law formula (delta-H = sum of products minus sum of reactants) fit on a single revision card and cover the majority of NEET questions.

Subtopics - Thermodynamics and Thermochemistry (NEET)

Eight topic blocks: thermodynamic terms (systems, properties, processes), internal energy and first law, enthalpy with heat capacity, PV work for isothermal and adiabatic expansions with Joule-Thomson effect, thermochemistry with ten types of heats of reaction, Hess's law with Born-Haber cycle, second law with Carnot cycle and entropy, and Gibbs free energy with spontaneity criteria and the third law.

Revision tip: For every thermodynamics numerical: (1) identify whether the process is constant pressure (use delta-H) or constant volume (use delta-E), (2) check the sign convention (exothermic = negative delta-H), (3) for Hess's law, reverse equations carefully and change the sign of delta-H, (4) for Gibbs questions, write delta-G = delta-H minus T delta-S and check the sign of each term before substituting.
NCERT LinesMCQsQuick Test

1) Thermodynamic Terms and System Types

Defines system, surroundings, and boundary. Classifies systems as isolated, closed, and open. Distinguishes extensive properties (volume, mass, entropy, enthalpy, heat capacity) from intensive properties (temperature, pressure, density, molar volume). Defines four process types: adiabatic, isothermal, isobaric, and isochoric.

Isolated: no energy or matter exchangeCp and Cv are extensive, T and P are intensiveAdiabatic: q = 0Isochoric: delta-V = 0
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System and surroundingsA system is any part of the universe set off by definite boundaries for study. The rest of the universe is the surroundings. The boundary separates the two. Isolated system: neither energy nor matter crosses the boundary (e.g., thermos flask). Closed system: energy can cross but matter cannot (e.g., sealed flask on a hot plate). Open system: both energy and matter can cross (e.g., open beaker on a hot plate). For a homogeneous system of definite mass, the state is defined by P, V, and T through the equation of state PV = nRT.
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Extensive and intensive propertiesExtensive properties depend on the amount of matter: volume, mass, number of moles, enthalpy, entropy, free energy, and heat capacity. Intensive properties are independent of quantity: temperature, pressure, density, molar volume, refractive index, surface tension, viscosity, boiling point, and freezing point. The ratio of two extensive properties gives an intensive property (density = mass/volume).
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Thermodynamic processesFour standard processes: (1) Adiabatic: no heat exchange (q = 0); exothermic adiabatic raises temperature, endothermic lowers it. (2) Isothermal: constant temperature; system exchanges heat with surroundings. (3) Isobaric: constant pressure; most chemistry reactions at atmospheric pressure. (4) Isochoric: constant volume; no PV work done (w = 0).

2) Internal Energy, Zeroth Law, and First Law of Thermodynamics

Internal energy (E) is the sum of all forms of molecular energy. The zeroth law establishes thermal equilibrium and the concept of temperature. The first law (dq = dE + dw) is conservation of energy applied to thermodynamic systems. Special cases: adiabatic (dw = -dE), cyclic (dq = dw), and isochoric (dq = dE).

dq = dE + dwAdiabatic: work at cost of ECyclic: delta-E = 0Isochoric: all heat raises E
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Internal energyInternal energy (E) is the total energy of a system from molecular constitution (potential energy from bonds and intermolecular forces) and molecular motion (kinetic energy from translation, rotation, vibration). It includes nuclear energy, electronic energy, bond energy, and molecular kinetic and potential energy. E is a state function: its value depends only on the current state, not on the path. At constant T and V, delta-E equals the heat exchanged with surroundings.
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Zeroth law of thermodynamicsIf two bodies A and B are each in thermal equilibrium with a third body C, then A and B are in thermal equilibrium with each other. This law provides the logical basis for the concept of temperature and was formulated after the first and second laws but placed before them. Two objects at different temperatures in thermal contact tend toward the same temperature.
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First law of thermodynamicsEnergy can be converted from one form to another but cannot be created or destroyed. Mathematical form: dq = dE + dw, where q is heat absorbed, dE is internal energy change, and dw is work done by the system. q and w are path functions; E is a state function. Special cases: (1) Adiabatic (dq = 0): dw = -dE, work done at cost of internal energy. (2) Cyclic process (dE = 0): dq = dw, all heat converts to work. (3) Isochoric (dV = 0, dw = 0): dq = dE, all heat increases internal energy.

3) Enthalpy and Heat Capacity

Enthalpy H = E + PV is the heat content at constant pressure. Delta-H = delta-E + P delta-V at constant pressure. Specific heat capacity (per gram) and molar heat capacity (per mole) are defined at constant P and constant V. Cp - Cv = R. Gamma = Cp/Cv varies with atomicity: 1.66 (monoatomic), 1.40 (diatomic), 1.33 (triatomic).

H = E + PVdelta-H = Q at constant PCp - Cv = RGamma: 1.66, 1.40, 1.33
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Enthalpy and enthalpy changeEnthalpy H = E + PV. At constant pressure: delta-H = delta-E + P delta-V. Since most chemical reactions occur at constant (atmospheric) pressure, delta-H equals the heat absorbed or evolved: delta-H = Q(p). Enthalpy is a state function. For reactions involving gases: delta-H = delta-E + delta-n(g) RT, where delta-n(g) = moles of gaseous products minus moles of gaseous reactants.
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Specific and molar heat capacitySpecific heat capacity: heat required to raise 1 g of substance by 1 degree C. Molar heat capacity = specific heat times molecular weight. Cp > Cv because at constant pressure, additional energy goes into expansion work (P delta-V = R per mole per degree). Key relations: Cp - Cv = R = 8.314 J = 2 cal. Cv = (3/2)R for monoatomic ideal gas. Gamma = Cp/Cv: monoatomic = 5/3 = 1.66, diatomic = 7/5 = 1.40, triatomic = 8/6 = 1.33.

4) Work, PV Work, and Joule-Thomson Effect

Defines heat and work as path functions. PV work at constant pressure: w = P delta-V. Isothermal reversible expansion: w(rev) = 2.303 nRT log(V2/V1). Adiabatic expansion follows PV^gamma = constant and TV^(gamma-1) = constant. Joule-Thomson effect: adiabatic expansion through a porous plug lowers temperature (isoenthalpic process). Most gases cool at room temperature except H2 and He.

w(rev) = 2.303 nRT log(V2/V1)PV^gamma = constant (adiabatic)Joule-Thomson: isoenthalpicH2 and He heat at room T
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Isothermal expansion workFor isothermal process: delta-T = 0, delta-E = 0, so q = -w. Reversible isothermal expansion of n moles of ideal gas from V1 to V2: w(rev) = 2.303 nRT log(V2/V1) = 2.303 nRT log(P1/P2). This is the maximum work obtainable. Irreversible isothermal expansion against constant external pressure P(ext): w(irr) = -P(ext)(V2 - V1). w(rev) > w(irr) always. Free expansion (P(ext) = 0): w = 0.
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Adiabatic expansionFor adiabatic process: q = 0. Relations: PV^gamma = constant; TV^(gamma-1) = constant; T^gamma P^(1-gamma) = constant. Reversible adiabatic: P1 V1^gamma = P2 V2^gamma; (T1/T2)^gamma = (P1/P2)^(gamma-1). Irreversible free adiabatic expansion into vacuum: delta-T = 0, delta-E = 0, w = 0, delta-H = 0 (all thermodynamic quantities zero). Intermediate irreversible adiabatic: w = Cv(T2 - T1).
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Joule-Thomson effectWhen a gas expands adiabatically from high pressure to low pressure through a porous plug, temperature changes. The process is isoenthalpic (delta-H = 0). Joule-Thomson coefficient mu = (partial-T/partial-P) at constant H. If mu > 0: cooling effect. If mu < 0: heating effect. If mu = 0: no temperature change (at inversion temperature). Most gases have inversion temperature above room temperature and show cooling. H2 (inversion temp -80 degrees C) and He (-240 degrees C) show heating at room temperature.

5) Thermochemistry and Types of Heats of Reaction

Heat of reaction is the enthalpy change for a balanced equation at a given temperature. Sign convention: exothermic (delta-H negative), endothermic (delta-H positive). Ten types of heats: vaporisation, fusion, precipitation, sublimation, formation, standard heat of formation, combustion, neutralisation, solution, and dilution. Factors affecting heat of reaction: physical state, allotropic form, temperature (Kirchhoff's equation), and constant V vs constant P.

Exothermic: delta-H < 0delta-H(sub) = delta-H(fus) + delta-H(vap)delta-H = delta-E + delta-n(g) RTNeutralisation SA+SB = 13.7 kcal
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Heat of reaction and sign conventionsHeat of reaction: enthalpy change when reactants form products as shown in a balanced equation. At constant volume (bomb calorimeter): q(v) = delta-E. At constant pressure (open calorimeter): q(p) = delta-H. Exothermic: heat evolved, delta-H negative. Endothermic: heat absorbed, delta-H positive. Relation: delta-H = delta-E + delta-n(g) RT, where delta-n(g) = moles gaseous products minus moles gaseous reactants.
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Types of heats of reactionTen standard types: (1) Heat of vaporisation: H2O(l) to H2O(g), delta-H = +10.5 kcal. (2) Heat of fusion: H2O(ice) to H2O(l), delta-H = +1.44 kcal. (3) Heat of precipitation: heat evolved when one mole of sparingly soluble substance precipitates. (4) Heat of sublimation: delta-H(sub) = delta-H(fusion) + delta-H(vaporisation). (5) Heat of formation: enthalpy change when one mole of compound forms from elements. (6) Standard heat of formation: at 1 atm and specified T; zero for elements in most stable form. (7) Heat of combustion: when one mole burns completely in excess air. (8) Heat of neutralisation: 13.7 kcal for strong acid + strong base; less for weak acid or weak base because dissociation energy is consumed. (9) Heat of solution: when one mole dissolves in large excess of water. (10) Heat of dilution: heat change on diluting from one concentration to another.
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Factors influencing heat of reactionFour factors: (1) Physical state: H2 + 1/2 O2 to H2O(g) gives delta-H = -57.8 kcal but to H2O(l) gives -68.3 kcal. (2) Allotropic form: graphite combustion gives -94.3 kcal, diamond combustion gives -97.6 kcal. (3) Temperature: Kirchhoff's equation: delta-H2 - delta-H1 = delta-Cp (T2 - T1). (4) Constant volume vs constant pressure: delta-H = delta-E + delta-n(g) RT.

6) Hess's Law and Born-Haber Cycle

Hess's law: enthalpy change is path-independent. delta-H(reaction) = sum of delta-Hf(products) minus sum of delta-Hf(reactants). Applications: calculating heats of formation for compounds that cannot be synthesised directly, and determining lattice energy via the Born-Haber cycle. The Born-Haber cycle relates lattice energy to sublimation energy, bond dissociation energy, ionisation energy, electron affinity, and heat of formation.

delta-H is path-independentdelta-H = sum(products) - sum(reactants)Born-Haber: lattice energyBond energy vs bond dissociation energy
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Hess's law of constant heat summationThe enthalpy change for a process is the same whether it occurs in one step or several steps. delta-H = delta-H1 + delta-H2 + ... + delta-Hn. For reaction aA + bB to cC + dD: delta-H(reaction) = [c delta-Hf(C) + d delta-Hf(D)] - [a delta-Hf(A) + b delta-Hf(B)]. Application: calculating heats of formation for compounds like C6H6 and C2H6 whose direct synthesis from elements is not possible experimentally.
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Born-Haber cycleDevised by Born and Haber (1919) to relate lattice energy of an ionic crystal to measurable thermochemical quantities. The cycle converts elements in standard states to gaseous atoms, then to gaseous ions, and finally packs them into the crystal lattice. delta-Hf = delta-H(sublimation) + delta-H(bond dissociation)/2 + IE + EA + LE. Knowing five of the six quantities, the sixth (usually lattice energy or electron affinity) can be calculated. Bond dissociation energy equals bond energy for diatomic molecules but not for polyatomic molecules where successive bonds differ.

7) Second Law of Thermodynamics, Carnot Cycle, and Entropy

The second law states that heat cannot be completely converted into work in a cyclic process. The Carnot cycle demonstrates maximum efficiency: eta = (T2 - T1)/T2 < 1. Entropy S measures disorder: dS = dq(rev)/T. For isothermal reversible expansion: delta-S = 2.303 nR log(V2/V1). Entropy of the universe always increases for spontaneous processes.

eta = (T(hot) - T(cold))/T(hot)dS = dq(rev)/TSpontaneous: delta-S(universe) > 0Liquid to gas: S increases
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Carnot cycle and second lawThe Carnot cycle (1824) is a theoretical reversible cycle with four steps operating between hot (T2) and cold (T1) reservoirs. Efficiency eta = w/q2 = (T2 - T1)/T2. Since (T2 - T1)/T2 < 1, not all heat can convert to work. Larger temperature difference gives greater efficiency. The second law in various forms: (1) all spontaneous processes are irreversible; (2) heat cannot flow from cold to hot body without external work; (3) entropy of the universe always increases in spontaneous processes; (4) complete conversion of heat to work in a cyclic process is impossible.
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EntropyEntropy (S) is a state function measuring the disorder or randomness of a system. dS = dq(rev)/T. Standard absolute entropy S(standard) is the entropy at 298 K and 1 atm. For isothermal reversible expansion of ideal gas: delta-S = 2.303 nR log(V2/V1) = 2.303 nR log(P1/P2). Entropy increases: solid to liquid to gas, dissolution, heating. Entropy decreases: crystallisation, cooling, gas to liquid to solid.

8) Gibbs Free Energy, Spontaneity, and Third Law

Gibbs free energy G = H - TS gives the direction of spontaneous change at constant T and P. delta-G = delta-H - T delta-S (Gibbs-Helmholtz equation). delta-G < 0: spontaneous; delta-G = 0: equilibrium; delta-G > 0: non-spontaneous. Relation to equilibrium constant: delta-G(standard) = -2.303 RT log K. The third law: entropy of a perfect crystal is zero at absolute zero.

delta-G = delta-H - T delta-Sdelta-G < 0: spontaneousdelta-G(std) = -2.303 RT log KS = 0 at T = 0 K (perfect crystal)
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Gibbs free energy and Gibbs-Helmholtz equationGibbs free energy G = H - TS. At constant T and P: delta-G = delta-H - T delta-S (Gibbs-Helmholtz equation). delta-G is an extensive property and changes sign when process is reversed. delta-Gf(standard) = 0 for elements in standard state. For a reaction: delta-G(standard) = sum of delta-Gf(products) - sum of delta-Gf(reactants). Relation to equilibrium constant: delta-G(standard) = -RT ln K = -2.303 RT log K.
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Criteria for spontaneityFour cases from delta-G = delta-H - T delta-S: (1) delta-H < 0, delta-S > 0: delta-G always negative, spontaneous at all temperatures. (2) delta-H > 0, delta-S < 0: delta-G always positive, non-spontaneous at all temperatures. (3) delta-H < 0, delta-S < 0: delta-G negative at low T (spontaneous) but positive at high T (non-spontaneous). (4) delta-H > 0, delta-S > 0: delta-G negative at high T (spontaneous) but positive at low T (non-spontaneous). At delta-G = 0, the system is at equilibrium.
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Third law of thermodynamicsAt absolute zero temperature (0 K), the entropy of a perfectly crystalline substance is zero. This provides an absolute scale for entropy measurement. S(standard) values at 298 K are measured relative to this zero reference. The third law allows calculation of absolute entropies from heat capacity data.

Thermodynamics and Thermochemistry Download Notes & Weightage Plan

For each topic in the Thermodynamics and Thermochemistry chapter below, you get (2) the exact resources to download and how to use them, and (3) a simple importance & time plan so NEET students know what to do first and what to revise last.

2 Downloads

Thermodynamic Terms and System Types

Definitions of system, surroundings, boundary, three system types, extensive vs intensive properties, and four process types.

Conceptual recallIntensive vs extensive is tested1 MCQ every 2-3 yearsTable-based questions

1) Download Packs For This Topic (And How To Use Them)

Don't download everything and forget it. Use these like a small "attack kit": read → highlight → test → revise the same sheet again.

↓
Topic Notes (Condensed)System: part of universe under study. Surroundings: rest of universe. Isolated: no energy or matter exchange. Closed: energy but not matter. Open: both. Extensive properties depend on amount (V, mass, n, H, S, G, Cp). Intensive properties are independent (T, P, density, molar volume, surface tension, viscosity). Processes: adiabatic (q = 0), isothermal (delta-T = 0), isobaric (delta-P = 0), isochoric (delta-V = 0).
Download NotesPrintable PDF
ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Make a two-column table: extensive vs intensive with 7 examples each. Memorise the four process types with what is held constant. Know that thermos flask = isolated system, sealed flask on burner = closed system, open beaker = open system.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions0-1Conceptual MCQ on system classification or intensive/extensive property identification appears in roughly 1 in 3 NEET papers.
Time Required1 hr30 min on system types and properties; 30 min on process types.
DifficultyEasyPure recall of definitions. No calculations needed. The classification of heat capacity as extensive can be tricky (it depends on mass).
  • Scoring Focus: Identify: thermos flask = isolated, sealed test tube = closed. Know that density, temperature, and pressure are intensive. Heat capacity is extensive (depends on amount of substance).
  • High-risk Area: Heat capacity is extensive but specific heat capacity is intensive. Students confuse the two. Total heat capacity doubles when the amount of substance doubles. Specific heat (per gram) does not change.
  • Best Practice Style: For property classification: ask whether the value changes when the amount of substance changes. If yes, it is extensive. If no, it is intensive.
Priority rule: Low-moderate priority. Quick revision topic. Spend 1 hour and move on to the mathematically heavier topics.

Internal Energy, Zeroth Law, and First Law of Thermodynamics

Internal energy as a state function, the zeroth law (thermal equilibrium), and the first law (dq = dE + dw) with its three special cases.

dq = dE + dwState function vs path functionCyclic: delta-E = 0Isochoric: dq = dE

1) Download Packs For This Topic (And How To Use Them)

Don't download everything and forget it. Use these like a small "attack kit": read → highlight → test → revise the same sheet again.

↓
Topic Notes (Condensed)Internal energy E = sum of all molecular energies (kinetic + potential). E is a state function. Zeroth law: if A is in thermal equilibrium with C, and B with C, then A is in equilibrium with B. First law: dq = dE + dw. q and w are path functions; E is a state function. Adiabatic (q = 0): w = -delta-E. Cyclic (delta-E = 0): q = w. Isochoric (delta-V = 0, w = 0): q = delta-E.
Download NotesPrintable PDF
ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Write the first law equation and derive the three special cases from it. Memorise: adiabatic means work at the expense of internal energy; cyclic means q converts to w; isochoric means all heat goes to internal energy.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions0-1One conceptual question on state function identification or first law application. Which is not a state function? (Answer: q and w).
Time Required2 hrs30 min on internal energy; 15 min on zeroth law; 45 min on first law with three cases; 30 min MCQ practice.
DifficultyEasy-ModerateThe mathematics is simple. The conceptual distinction between state functions and path functions is the most tested idea.
  • Scoring Focus: State functions: E, H, S, G, T, P, V. Path functions: q (heat) and w (work). The combination q + w = delta-E is a state function even though q and w individually are not.
  • High-risk Area: Students sometimes think q + w (which equals delta-E) must also be a path function because q and w are path functions. But delta-E is a state function. The sum of two path functions can be a state function, which is counterintuitive. NEET tests this exact idea.
  • Best Practice Style: If the question asks about state functions, q and w are always path functions. Everything else on the standard list (E, H, S, G, T, P, V) is a state function.
Priority rule: Moderate priority. The state function vs path function distinction appears frequently. Master it in 2 hours.

Enthalpy and Heat Capacity

H = E + PV, delta-H at constant pressure, specific and molar heat capacities, Cp - Cv = R, and gamma values for monoatomic, diatomic, and triatomic gases.

H = E + PVCp - Cv = R = 8.314 JGamma = 1.66, 1.40, 1.33delta-H = delta-E + delta-n(g) RT

1) Download Packs For This Topic (And How To Use Them)

Don't download everything and forget it. Use these like a small "attack kit": read → highlight → test → revise the same sheet again.

↓
Topic Notes (Condensed)H = E + PV. delta-H = delta-E + P delta-V at constant P. delta-H = Q(p). delta-H = delta-E + delta-n(g) RT for gas-phase reactions. Cp - Cv = R = 8.314 J/mol K = 2 cal/mol K. For monoatomic ideal gas: Cv = (3/2)R, Cp = (5/2)R, gamma = 5/3 = 1.66. For diatomic: Cv = (5/2)R, Cp = (7/2)R, gamma = 7/5 = 1.40. For triatomic: Cv = 6R/2 = 3R, Cp = 4R, gamma = 4/3 = 1.33.
Download NotesPrintable PDF
ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Memorise: Cp - Cv = R and the three gamma values. Know how to use delta-H = delta-E + delta-n(g) RT to convert between bomb calorimeter (delta-E) and constant pressure (delta-H) values.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions0-1Numerical: given delta-E and the reaction, calculate delta-H using delta-n(g) RT. Or: what is gamma for a monoatomic gas?
Time Required2 hrs45 min on enthalpy definition and delta-H = delta-E + delta-n(g) RT; 45 min on heat capacities and gamma; 30 min MCQ practice.
DifficultyModerateThe delta-H = delta-E + delta-n(g) RT conversion requires counting gaseous moles correctly. Negative delta-n(g) makes delta-H less than delta-E, which can be confusing.
  • Scoring Focus: delta-n(g) = total moles of gaseous products minus total moles of gaseous reactants. Do NOT count solids or liquids. Use R = 8.314 J and T = 298 K unless specified otherwise.
  • High-risk Area: Counting delta-n(g) incorrectly by including solid or liquid species. For N2(g) + 3H2(g) to 2NH3(g): delta-n(g) = 2 - 4 = -2, not -1 or 0. Students who rush may miscount the 3 moles of H2.
  • Best Practice Style: Write out all gaseous species on each side. Count. Subtract. Then substitute into delta-H = delta-E + delta-n(g) RT.
Priority rule: Moderate priority. delta-H vs delta-E conversion is tested. Gamma values are tested in physics context more than chemistry.

Work, PV Work, and Joule-Thomson Effect

Defines PV work. Isothermal reversible expansion: w = 2.303 nRT log(V2/V1), maximum work. Adiabatic expansion: PV^gamma = constant. Free expansion: all thermodynamic quantities zero. Joule-Thomson effect and inversion temperature.

w(rev) = 2.303 nRT log(V2/V1)w(rev) > w(irr)Adiabatic: PV^gamma = constJ-T: mu > 0 means cooling

1) Download Packs For This Topic (And How To Use Them)

Don't download everything and forget it. Use these like a small "attack kit": read → highlight → test → revise the same sheet again.

↓
Topic Notes (Condensed)PV work at constant P: w = P delta-V. Isothermal reversible: w(rev) = 2.303 nRT log(V2/V1) = -2.303 nRT log(P2/P1). This is maximum work. Irreversible: w(irr) = P(ext)(V2 - V1) < w(rev). Free expansion: P(ext) = 0, w = 0. Adiabatic reversible: PV^gamma = constant; TV^(gamma-1) = constant; T^gamma P^(1-gamma) = constant. Free adiabatic expansion: delta-T = delta-E = w = delta-H = 0. Joule-Thomson: adiabatic expansion through porous plug, isoenthalpic (delta-H = 0). mu = (dT/dP) at constant H. mu > 0: cooling; mu < 0: heating; mu = 0: inversion temperature. Most gases cool at room T; H2 and He heat.
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ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Practise one numerical on isothermal reversible work. Know that w(rev) is maximum work. Memorise the three adiabatic relations (PV^gamma, TV^(gamma-1), T^gamma P^(1-gamma)). For Joule-Thomson: H2 and He are the exceptions.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions0-1Numerical on isothermal reversible work or a conceptual question on adiabatic process behaviour.
Time Required2 hrs45 min on isothermal work; 45 min on adiabatic relations; 15 min on Joule-Thomson; 15 min MCQ.
DifficultyModerateThe isothermal work formula involves logarithms. The adiabatic relations require remembering which exponent goes where.
  • Scoring Focus: For isothermal reversible work: w = 2.303 nRT log(V2/V1). Expansion (V2 > V1): w is positive (work done by system). For adiabatic: PV^gamma = constant, which means V increases and T decreases.
  • High-risk Area: Confusing isothermal and adiabatic: in isothermal expansion delta-T = 0 but q is not zero (heat is absorbed). In adiabatic expansion q = 0 but delta-T is not zero (temperature falls). Students who mix these two get both wrong.
  • Best Practice Style: Isothermal: T fixed, system exchanges heat. Adiabatic: q = 0, T changes. These are the two fundamental contrasts.
Priority rule: Moderate priority. Isothermal work calculation is tested. Adiabatic relations are more common in physics exams.

Thermochemistry and Types of Heats of Reaction

Defines ten types of heats. Key values: heat of neutralisation SA+SB = 13.7 kcal, heat of sublimation = fusion + vaporisation. Factors: physical state, allotropy, temperature (Kirchhoff), and constant P vs V.

SA+SB neutralisation = 13.7 kcaldelta-H(sub) = delta-H(fus) + delta-H(vap)Physical state mattersKirchhoff: delta-Cp(T2-T1)

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Topic Notes (Condensed)Ten heats: vaporisation (+10.5 kcal for water), fusion (+1.44 kcal for ice), precipitation (exothermic), sublimation = fusion + vaporisation, formation (one mole from elements), standard formation (at 1 atm, zero for elements), combustion (complete burning), neutralisation (13.7 kcal for SA+SB, less for WA or WB), solution (dissolving one mole), dilution (concentration change). Factors: physical state (H2O(g) vs H2O(l) differ by 10.5 kcal), allotropy (diamond vs graphite differ by 3.3 kcal), temperature (Kirchhoff: H2 - H1 = delta-Cp(T2 - T1)), constant V vs P (delta-H = delta-E + delta-n(g)RT).
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ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Make a flashcard with all ten heat types and one example each. The most tested are: heat of formation (zero for elements), heat of combustion (always negative), and heat of neutralisation (13.7 kcal for SA+SB). Know that sublimation = fusion + vaporisation.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions1One question on heat of neutralisation difference between SA+SB and WA+SB, or one on heat of formation (standard enthalpy of formation of O2(g) = 0).
Time Required3 hrs1 hr on definitions and examples for all ten types; 1 hr on factors affecting heat of reaction; 1 hr MCQ practice.
DifficultyEasy-ModerateMostly recall of definitions and values. The heat of neutralisation for weak acids is tricky: the difference from 13.7 kcal gives the dissociation energy.
  • Scoring Focus: Standard enthalpy of formation of elements in most stable form = 0. Heat of neutralisation for SA+SB = 13.7 kcal; for WA+SB it is less because energy goes to dissociate the weak acid first. The difference gives the enthalpy of ionisation of the weak acid.
  • High-risk Area: Forgetting that heat of combustion is ALWAYS exothermic (delta-H negative). Students sometimes write delta-H for combustion as positive. Also: standard heat of formation of O2(g), N2(g), C(graphite) etc. is zero, not undefined.
  • Best Practice Style: For any thermochemistry question: first identify the type of heat (formation, combustion, neutralisation, etc.), then apply the definition precisely. Formation = one mole from elements. Combustion = one mole burns completely.
Priority rule: High priority. Thermochemistry definitions are tested every year. The SA+SB neutralisation value of 13.7 kcal is a must-know.

Hess's Law and Born-Haber Cycle

Hess's law: path independence of enthalpy. delta-H(rxn) = sum delta-Hf(products) - sum delta-Hf(reactants). Born-Haber cycle for ionic lattice energy.

Path independentReverse equation: change signBorn-Haber: 5 energy termsLattice energy from cycle

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Topic Notes (Condensed)Hess's law: delta-H for a reaction is the same whether in one step or several. delta-H = delta-H1 + delta-H2 + ... + delta-Hn. For aA + bB to cC + dD: delta-H(rxn) = [c delta-Hf(C) + d delta-Hf(D)] - [a delta-Hf(A) + b delta-Hf(B)]. When reversing an equation, change the sign of delta-H. When multiplying by a coefficient, multiply delta-H by the same factor. Born-Haber cycle (1919): delta-Hf = delta-H(sublimation) + (1/2) delta-H(bond dissociation) + IE + EA + LE. Used to calculate lattice energy (LE) from known quantities or electron affinity from known LE.
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ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Practise two Hess's law numericals: one using standard enthalpies of formation, one using combustion data. For Born-Haber: draw the cycle for NaCl and label all five steps. Know the sign convention: sublimation and IE are positive, EA is negative, LE is negative.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions1One numerical on Hess's law using delta-Hf or combustion data, or one on Born-Haber cycle to find lattice energy.
Time Required2 hrs1 hr on Hess's law with worked examples; 30 min on Born-Haber cycle; 30 min MCQ practice.
DifficultyModerateThe calculation itself is arithmetic. The difficulty lies in correctly reversing equations and handling signs when combining multiple thermochemical equations.
  • Scoring Focus: Hess's law is the most numerically tested topic in NEET thermodynamics. Know the formula: delta-H(rxn) = sum of delta-Hf(products) minus sum of delta-Hf(reactants). For Born-Haber: NEET asks to identify which step in the cycle represents a given thermochemical quantity.
  • High-risk Area: Students reverse a thermochemical equation but forget to reverse the sign of delta-H. If A to B has delta-H = +100 kJ, then B to A has delta-H = -100 kJ. Also: multiplying the equation by 2 means delta-H is multiplied by 2. Students who forget this get answers off by a factor of 2.
  • Best Practice Style: When combining equations using Hess's law: (1) write the target equation, (2) manipulate given equations one at a time to match the target, (3) when reversing, change the sign, (4) when multiplying, multiply delta-H, (5) add all delta-H values.
Priority rule: Highest priority within this chapter. One Hess's law numerical appears in most NEET papers. Spend at least 2 hours on worked problems.

Second Law of Thermodynamics, Carnot Cycle, and Entropy

Second law: heat cannot fully convert to work. Carnot efficiency. Entropy as disorder: dS = dq(rev)/T. Entropy change for isothermal expansion.

eta = (T2-T1)/T2dS = dq(rev)/TS increases: disorder upUniverse entropy always increases

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Topic Notes (Condensed)Second law: impossible to convert heat completely to work in cyclic process. Carnot cycle efficiency: eta = (T2 - T1)/T2 where T2 > T1. Always less than 1. Entropy S: state function measuring disorder. dS = dq(rev)/T. For isothermal reversible expansion: delta-S = 2.303 nR log(V2/V1) = 2.303 nR log(P1/P2). Entropy increases: solid to liquid to gas, dissolution, temperature increase. In every spontaneous process, entropy of the universe increases.
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ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Memorise: Carnot efficiency formula, entropy formula for isothermal expansion, and the rule that S(universe) increases for spontaneous processes. One numerical on entropy calculation for isothermal expansion is sufficient.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions0-1Entropy or second law questions are less common than Gibbs free energy but appear occasionally: calculate delta-S for isothermal expansion, or identify the process where entropy decreases.
Time Required1.5 hrs30 min on Carnot and second law; 30 min on entropy formulas; 30 min MCQ practice.
DifficultyModerateThe entropy formula is similar to the work formula (same log ratio). The conceptual connection between disorder and entropy is intuitive but requires careful reasoning for edge cases.
  • Scoring Focus: Entropy increases: solid to liquid to gas; fewer moles to more moles of gas; mixing; dissolution. Entropy decreases: gas to liquid to solid; more moles to fewer moles of gas; crystallisation.
  • High-risk Area: For the reaction 2H2(g) + O2(g) to 2H2O(l): entropy decreases (3 moles gas to 0 moles gas). Students who see an exothermic combustion may think entropy increases, but the physical state change (gas to liquid) dominates.
  • Best Practice Style: Count moles of gas on each side. If gas moles increase, delta-S is positive. If gas moles decrease, delta-S is negative. This quick check works for most NEET questions.
Priority rule: Moderate priority. Spend 1.5 hours. The Gibbs equation covers entropy indirectly, so focus more on Gibbs.

Gibbs Free Energy, Spontaneity, and Third Law

G = H - TS. delta-G = delta-H - T delta-S. Criteria for spontaneity based on delta-G sign. Four cases from signs of delta-H and delta-S. Relation to equilibrium constant. Third law: S = 0 at 0 K for perfect crystals.

delta-G = delta-H - T delta-Sdelta-G < 0: spontaneousdelta-G(std) = -2.303 RT log KFour spontaneity cases

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Topic Notes (Condensed)G = H - TS. delta-G = delta-H - T delta-S (Gibbs-Helmholtz). delta-G < 0: spontaneous. delta-G = 0: equilibrium. delta-G > 0: non-spontaneous. Four cases: (1) delta-H < 0, delta-S > 0: always spontaneous. (2) delta-H > 0, delta-S < 0: never spontaneous. (3) delta-H < 0, delta-S < 0: spontaneous at low T. (4) delta-H > 0, delta-S > 0: spontaneous at high T. delta-G(standard) = -2.303 RT log K. delta-Gf(standard) = 0 for elements. Third law: S = 0 at 0 K for perfect crystal (Nernst).
Download NotesPrintable PDF
ā˜…
NCERT Key Lines (One-Liners)These are the lines NEET converts into "statement is correct/incorrect" questions.
NCERT LinesFlashcards
Q
Practice Set (MCQs + PYQs)Do 30–50 questions, then mark errors as "memory miss" or "confusion between options."
MCQ SetPYQs
How to revise: Draw the 2x2 table: delta-H (negative/positive) vs delta-S (positive/negative) with the resulting T-dependence of spontaneity. This single table answers most NEET Gibbs questions. Know the formula delta-G(standard) = -2.303 RT log K.

2) Importance, Weightage & Time Allocation (Practical)

Use this to avoid over-studying. This topic is usually low effort, quick return if your recall is clean.

Expected Questions1One MCQ asking: given delta-H and delta-S signs, is the reaction spontaneous at high or low temperature? Or: for a reaction at equilibrium, delta-G = 0.
Time Required2 hrs45 min on Gibbs equation and four cases; 30 min on delta-G and K relationship; 15 min on third law; 30 min MCQ practice.
DifficultyModerateThe Gibbs equation itself is simple. The difficulty is in correctly handling the four sign combinations and determining whether T must be high or low for spontaneity.
  • Scoring Focus: The four-case table is the highest-yield single item in this chapter. If delta-H is negative and delta-S is positive, delta-G is always negative: spontaneous at all temperatures. If both have the same sign, temperature becomes the deciding factor.
  • High-risk Area: When delta-H and delta-S are both negative: delta-G = (negative) - T(negative) = negative + T(positive). At low T, the delta-H term dominates and delta-G is negative (spontaneous). At high T, the T delta-S term dominates and delta-G becomes positive (non-spontaneous). Students often get confused about which term dominates at which temperature.
  • Best Practice Style: Use the four-case table. For the borderline cases (both same sign): the reaction is spontaneous when the dominant term makes delta-G negative. If delta-H < 0 and delta-S < 0, the enthalpy driving force wins at low T. If delta-H > 0 and delta-S > 0, the entropy driving force wins at high T.
Priority rule: Highest priority alongside Hess's law. The Gibbs spontaneity question appears in every NEET paper. Memorise the four-case table.

Thermodynamics and Thermochemistry Chapter NEET Traps & Common Mistakes (Topic-Wise)

Each subtopic below is of the Thermodynamics and Thermochemistry chapter and shows what NEET students usually do wrong in NEET examination, a short example of the mistake, and how NEET frames the question to trick you with close options are given below.

! Avoid Easy Negatives
Gibbs Free Energy and Spontaneity
NEETGibbsSpontaneitydelta-G

Mistake Snapshot (What Students Do Wrong)

  • Wrong temperature dependence of spontaneity: When delta-H < 0 and delta-S < 0, the reaction is spontaneous at LOW temperature (enthalpy-driven), not high temperature. Students who think exothermic always means spontaneous at all temperatures miss the entropy penalty at high T.
  • Thinking delta-G = 0 means no reaction occurs: delta-G = 0 means the system is at EQUILIBRIUM, not that the reaction is impossible. Both forward and reverse reactions occur at equal rates.
2–3 Line Example (Typical Error)

For the freezing of water at -5 degrees C: delta-H < 0 (exothermic), delta-S < 0 (liquid to solid, more ordered). At low T (below 0 degrees C), delta-G < 0: spontaneous. At high T (above 0 degrees C), delta-G > 0: non-spontaneous (ice melts instead). At exactly 0 degrees C, delta-G = 0: equilibrium.

How NEET Frames The Trap

NEET gives delta-H and delta-S signs and asks at what temperature the reaction is spontaneous.

NEET-Style Trap Question Format

Q. A reaction has delta-H = -50 kJ/mol and delta-S = -100 J/mol K. The reaction is spontaneous at
A. T < 500 K   B. T > 500 K   C. All temperatures   D. No temperature  
Trick: delta-G = delta-H - T delta-S = -50000 - T(-100) = -50000 + 100T. For spontaneity: delta-G < 0, so -50000 + 100T < 0, giving T < 500 K. Option A is correct. Option B reverses the inequality. Option C ignores the entropy term.

Quick rule: Same-sign case: delta-H and delta-S both negative means spontaneous at LOW T (enthalpy wins). Both positive means spontaneous at HIGH T (entropy wins). Crossover temperature: T = delta-H / delta-S.
Hess's Law Sign Error
NEETHessSign conventionEnthalpy

Mistake Snapshot (What Students Do Wrong)

  • Forgetting to reverse delta-H when reversing an equation: If A to B has delta-H = +100 kJ, then B to A has delta-H = -100 kJ. Students who add equations without reversing the sign get answers that are off by twice the delta-H of the reversed step.
  • Not multiplying delta-H when multiplying the equation coefficients: If C + O2 to CO2 has delta-H = -94 kcal, then 2C + 2O2 to 2CO2 has delta-H = -188 kcal. Forgetting to multiply gives half the correct answer.
2–3 Line Example (Typical Error)

Given: C + O2 to CO2, delta-H = -94 kcal; CO + 1/2 O2 to CO2, delta-H = -67.5 kcal. Find delta-H for C + 1/2 O2 to CO. Reverse the second equation: CO2 to CO + 1/2 O2, delta-H = +67.5 kcal. Add to first: C + O2 + CO2 to CO2 + CO + 1/2 O2. Cancel CO2: C + 1/2 O2 to CO, delta-H = -94 + 67.5 = -26.5 kcal. Without reversing the sign: delta-H = -94 + (-67.5) = -161.5 kcal, which is wrong.

How NEET Frames The Trap

NEET gives two thermochemical equations and asks for the delta-H of a third equation derived by combining them.

NEET-Style Trap Question Format

Q. Given: H2(g) + 1/2 O2(g) to H2O(l), delta-H = -286 kJ and H2(g) + 1/2 O2(g) to H2O(g), delta-H = -242 kJ. The enthalpy of vaporisation of water is
A. +44 kJ   B. -44 kJ   C. +528 kJ   D. -528 kJ  
Trick: H2O(l) to H2O(g): reverse first equation and add to second. delta-H = +286 + (-242) = +44 kJ (Option A). Option B forgets to reverse the sign. Options C and D multiply incorrectly.

Quick rule: Reverse = flip sign. Multiply = multiply delta-H. Add = add delta-H values. Always check: is the final delta-H positive or negative, and does it make physical sense?
delta-H vs delta-E Conversion
NEETEnthalpyInternal energydelta-n(g)

Mistake Snapshot (What Students Do Wrong)

  • Including solids and liquids in delta-n(g): delta-n(g) counts ONLY gaseous species. For CaCO3(s) to CaO(s) + CO2(g): delta-n(g) = 1 - 0 = 1, not 2 - 1 = 1 (which coincidentally gives the right answer here but would fail for other reactions).
  • Wrong sign or unit for R: When using delta-H = delta-E + delta-n(g)RT, R must be in the same unit system as delta-H. If delta-H is in kJ, use R = 8.314 x 10^-3 kJ/(mol K). Using R = 8.314 J gives an answer off by factor of 1000.
2–3 Line Example (Typical Error)

For N2(g) + 3H2(g) to 2NH3(g), delta-H = -92 kJ at 298 K. delta-n(g) = 2 - (1+3) = -2. delta-H = delta-E + delta-n(g)RT. -92 = delta-E + (-2)(8.314 x 10^-3)(298). -92 = delta-E - 4.95. delta-E = -92 + 4.95 = -87.05 kJ. If student counts delta-n(g) = -1 (forgetting 3H2 is 3 moles): delta-E = -89.5 kJ, which is wrong.

How NEET Frames The Trap

NEET gives delta-H and asks for delta-E, or vice versa. The distractors use wrong delta-n(g) counts.

NEET-Style Trap Question Format

Q. For the reaction C(s) + H2O(g) to CO(g) + H2(g), delta-H = 131.3 kJ. Calculate delta-E at 298 K.
A. 128.8 kJ   B. 131.3 kJ   C. 133.8 kJ   D. 126.3 kJ  
Trick: delta-n(g) = (1+1) - (1) = 1 (C is solid, not counted). delta-H = delta-E + delta-n(g)RT. 131.3 = delta-E + (1)(8.314 x 10^-3)(298) = delta-E + 2.48. delta-E = 131.3 - 2.48 = 128.8 kJ (Option A). Option B ignores the correction. Option C adds instead of subtracting.

Quick rule: delta-n(g): count only GAS moles. Products minus reactants. delta-H = delta-E + delta-n(g)RT. If delta-n(g) > 0: delta-H > delta-E. If delta-n(g) < 0: delta-H < delta-E.
Isothermal vs Adiabatic Process Confusion
NEETIsothermalAdiabaticProcess

Mistake Snapshot (What Students Do Wrong)

  • Thinking isothermal means no heat exchange: Isothermal means constant temperature. Heat IS exchanged with surroundings to maintain T. In contrast, adiabatic means q = 0 (no heat exchange) and T changes.
  • Applying isothermal work formula to adiabatic process: w = 2.303 nRT log(V2/V1) is valid only for isothermal reversible expansion. For adiabatic, the work depends on Cv(T1-T2) and the PV^gamma relations.
2–3 Line Example (Typical Error)

1 mole of ideal gas expands from 10 L to 20 L. Isothermal at 300K: w = 2.303(1)(8.314)(300) log(2) = 1729 J, and q = 1729 J (heat absorbed), delta-T = 0. Adiabatic: q = 0, T drops, w = Cv(T1-T2) = (3/2)(8.314)(T1-T2) for monoatomic gas.

How NEET Frames The Trap

NEET asks for work or delta-T under isothermal or adiabatic conditions. Applying the wrong formula gives the wrong answer.

NEET-Style Trap Question Format

Q. For an ideal gas undergoing adiabatic expansion, which is true?
A. Temperature decreases   B. Temperature remains constant   C. delta-E = 0   D. q = w  
Trick: Adiabatic: q = 0; gas does work at expense of internal energy, so E decreases and T decreases. Option A is correct. Option B is isothermal. Option C is isothermal. Option D is cyclic process.

Quick rule: Isothermal: delta-T = 0, q is not zero. Adiabatic: q = 0, delta-T is not zero. Free expansion (adiabatic into vacuum): everything is zero.
Heat of Neutralisation for Weak Acids
NEETNeutralisationWeak acidEnthalpy

Mistake Snapshot (What Students Do Wrong)

  • Assuming all neutralisations release 13.7 kcal: 13.7 kcal is for strong acid + strong base only. Weak acid + strong base releases less because part of the energy goes to dissociate the weak acid. The difference gives the enthalpy of ionisation of the weak acid.
  • Forgetting that the ionic reaction H+ + OH- to H2O gives 13.7 kcal: The actual neutralisation step is always H+ + OH- to H2O with delta-H = -13.7 kcal. For weak acids, the observed heat is less because dissociation of the weak acid consumes some energy.
2–3 Line Example (Typical Error)

Heat of neutralisation of CH3COOH with NaOH = -11.7 kcal. Enthalpy of ionisation of CH3COOH = 13.7 - 11.7 = 2.0 kcal. The 2.0 kcal is consumed in dissociating acetic acid before neutralisation can occur.

How NEET Frames The Trap

NEET gives heat of neutralisation of a weak acid and asks for the enthalpy of ionisation, or vice versa.

NEET-Style Trap Question Format

Q. The enthalpy of neutralisation of HCN with NaOH is -12.1 kcal. The enthalpy of ionisation of HCN is
A. 1.6 kcal   B. -1.6 kcal   C. 25.8 kcal   D. -25.8 kcal  
Trick: Ionisation energy = 13.7 - 12.1 = 1.6 kcal (Option A). Ionisation is endothermic (positive). Option B makes it exothermic. Options C and D add instead of subtract.

Quick rule: Enthalpy of ionisation of weak acid = 13.7 kcal - (observed heat of neutralisation). Always positive (endothermic).
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