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JEE · NEET Physics

Class 12 · Chapter 13

Nuclei

Overview, notes, short notes, formula sheet, daily practice problems, previous year questions, and videos for this chapter — all in one place.

Nuclei Formula Sheet

12 formulas across 4 topics in Nuclei.

2 min read

Updated 2026-07-09 · v1.0.0

Nuclear Size, Density & Composition

Every nucleus, however different its mass, has almost exactly the same density — a striking clue that nucleons are packed together at a fixed spacing, like incompressible drops of nuclear fluid.

R = R₀ A^(1/3) , R₀ ≈ 1.2 fm

Nuclear radius

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Rnuclear radiusfm (femtometre)[L]
Amass number (total nucleons)dimensionless[M⁰L⁰T⁰]
R₀empirical constantR₀ ≈ 1.2 × 10⁻¹⁵ mfm[L]

Valid when

  • The A^(1/3) scaling (not A directly) is what keeps nuclear density roughly constant across all nuclei

ρ = mass / volume ≈ 2.3 × 10¹⁷ kg/m³ (constant, independent of A)

Nuclear density

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Mass ∝ A and volume ∝ R³ ∝ A both scale identically with A, so their ratio (density) is independent of A

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
ρnuclear densitykg/m³[ML⁻³]

Valid when

  • Nearly identical for every nucleus, light or heavy — direct evidence that nucleons pack together at a fixed characteristic spacing

Common mistakes

  • Nuclear density is essentially THE SAME for all elements — a very commonly tested one-line fact, don't assume heavier nuclei are denser

Mass–Energy Equivalence & Binding Energy

A nucleus weighs slightly LESS than the sum of its free, separated nucleons — that missing mass has been converted into the binding energy holding the nucleus together.

E = mc²

Einstein's mass–energy equivalence

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Eenergy equivalent of mass mJ[ML²T⁻²]

Valid when

  • The conversion factor used throughout nuclear physics: 1 u (atomic mass unit) = 931.5 MeV of energy

Δm = [Zm(p) + (A−Z)m(n)] − M(nucleus)

Mass defect

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Δmmass defect — the 'missing' massu or kg[M]
m(p), m(n)mass of a free proton and free neutronu[M]
Mactual measured mass of the nucleusu[M]

Valid when

  • Δm is always positive — a bound nucleus is always lighter than its separated, free constituent nucleons

BE = Δm c² (BE in MeV = Δm in u × 931.5)

Binding energy of a nucleus

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Direct application of E = mc² to the mass defect

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
BEbinding energy — energy needed to completely separate the nucleus into free nucleonsMeV[ML²T⁻²]

Valid when

  • Higher BE means a MORE stable (more tightly bound) nucleus

BE per nucleon = BE / A

Binding energy per nucleon

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The single most important quantity for judging nuclear stability, plotted against A gives the famous BE/A curve

Valid when

  • Peaks around A ≈ 56 (iron) — nuclei near this peak are the most stable; both fission (splitting heavy nuclei) and fusion (combining light nuclei) release energy by moving TOWARD this peak

Common mistakes

  • Both fission AND fusion release energy because both move the resulting nuclei's BE/A closer to the peak at iron — not because one 'always releases more' than the other in every case

Nuclear Fission & Fusion

Both processes release energy from the SAME underlying source — moving nuclei toward the binding-energy peak near iron — but they operate at opposite ends of the periodic table.

Q = [Σm(reactants) − Σm(products)] c²

Q-value of a nuclear reaction (fission or fusion)

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Conservation of mass-energy applied to the reactants and products of any nuclear reaction

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Qenergy released (Q > 0) or absorbed (Q < 0) in the reactionMeV[ML²T⁻²]

Valid when

  • Q > 0 means an exothermic (energy-releasing) reaction — true for both typical fission of heavy nuclei and fusion of light nuclei

Worth remembering

  • A nuclear chain reaction is self-sustaining only above a CRITICAL SIZE (critical mass) of fissile material — below it, too many neutrons escape without causing further fission
  • Fusion requires extremely high temperatures (tens of millions of kelvin) to overcome the strong electrostatic repulsion between positively charged nuclei before the short-range nuclear force can take over

Radioactive Decay

Radioactive decay is a purely random, memoryless process at the level of any single nucleus — yet a large enough sample decays with perfect statistical predictability, following one clean exponential law.

N = N₀ e^(−λt)

Law of radioactive decay

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Rate of decay is proportional to the number of undecayed nuclei present: dN/dt = −λN, solved as an exponential decay

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Nnumber of undecayed nuclei at time tdimensionless (a count)[M⁰L⁰T⁰]
N₀initial number of undecayed nucleidimensionless (a count)[M⁰L⁰T⁰]
λdecay constant, a property of the specific radioactive isotopes⁻¹[T⁻¹]

Valid when

  • Decay constant λ is completely independent of external conditions (temperature, pressure, chemical state) — purely a nuclear property

T(1/2) = ln2 / λ = 0.693/λ

Half-life in terms of the decay constant

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Time for N to fall to N₀/2 in the decay law: ½ = e^(−λT(1/2))

Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
T(1/2)half-life — time for half the sample to decays[T]

Valid when

  • Half-life is CONSTANT regardless of how much sample remains — it doesn't matter if you start with 1 gram or 1 kg, half of whatever is left decays in each successive half-life

τ = 1/λ = T(1/2) / ln2 ≈ 1.44 T(1/2)

Mean life (average life) of a radioactive sample

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
τmean life — average lifetime of a nucleus before decayings[T]

Valid when

  • Mean life is always LONGER than half-life (τ ≈ 1.44 T(1/2)) — a frequently tested numeric ratio

Common mistakes

  • Mean life and half-life are NOT the same quantity — mixing them up in a calculation gives an answer off by the factor 1.44 (or 0.693, its reciprocal)

A = λN = A₀ e^(−λt)

Activity of a radioactive sample

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Variables used in this formula, with units and dimensions
SymbolMeaningUnitDimension
Aactivity — number of decays per second1 Ci = 3.7 × 10¹⁰ BqBq (becquerel) or Ci (curie)[T⁻¹]

Valid when

  • Activity decays with the SAME time constant λ as N itself — halving N also halves the activity

N/N₀ = (1/2)^(t/T(1/2))

Fraction of a sample remaining after n half-lives

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Equivalent restatement of the decay law directly in terms of the number of elapsed half-lives

Valid when

  • Often the fastest way to solve a problem when t is given as a whole-number multiple of T(1/2)

Alpha decay reduces mass number by 4 and atomic number by 2; beta-minus decay keeps mass number the same but increases atomic number by 1 — boards frequently ask to balance a decay equation using these rules alongside the decay-law formulas.

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