Nuclei Chapter: All Important Formulas for NEET (Full List)

Physics · nuclei · NEET

The Nuclei chapter has about 10 core formulas you must remember: nuclear radius R = R0 A^(1/3), mass defect and binding energy (using 1 u = 931.5 MeV), the decay law N = N0 e^(-lambda t), half-life T = 0.693 / lambda, activity R = lambda N, and Q-value for fission and fusion. Memory hook: think "SIZE, MASS, DECAY" - first the nucleus SIZE (radius, density), then its MASS and binding energy, then how it DECAYS (half-life, activity, fission, fusion). If you group them this way, all 10 formulas fall into just 3 boxes.
Nuclei Formulas: 3 Groups to Remember1. SIZER = R0 A^(1/3)R0 = 1.2 fmdensity = const(no A term)2. MASSdm = Zmp+Nmn-MEb = dm x c^21 u = 931.5 MeVBE/nucleon=Eb/A3. DECAYN = N0 e^(-Lt)T = 0.693 / Ltau = 1 / LR = L N, Q=dm x 931.5L = lambda (decay const)
All Nuclei formulas sorted into three groups - SIZE (radius, density), MASS (mass defect, binding energy), and DECAY (decay law, half-life, activity, Q-value). Learn them box by box.

Your doubts, answered

What are the SIZE (radius and density) formulas I must know?

Two only. Nuclear radius R = R0 A^(1/3), where R0 = 1.2 fm (1 fm = 10^-15 m) and A is the mass number. Nuclear density is constant, about 2.3 x 10^17 kg/m^3, and it does NOT depend on A. Reason: mass grows as A, and volume also grows as A (since R^3 is proportional to A), so density = mass/volume stays the same for every nucleus.

How do I write mass defect and binding energy formulas correctly?

Mass defect: delta-m = [Z*mp + (A - Z)*mn] - M, where Z = number of protons, (A - Z) = number of neutrons, mp and mn are proton and neutron masses, and M is the actual nuclear (or atomic) mass. Binding energy: Eb = delta-m * c^2. For a quick NEET shortcut, use Eb = delta-m (in u) * 931.5 MeV. Binding energy per nucleon = Eb / A.

What is the difference between decay constant, half-life and mean life formulas?

They are three linked constants. Decay law: N = N0 e^(-lambda t). Half-life T(1/2) = 0.693 / lambda (0.693 = ln 2). Mean life tau = 1 / lambda. Combining: T(1/2) = 0.693 * tau, so half-life is always shorter than mean life. Never mix them up in a numerical.

What is the fastest formula for fraction left after n half-lives?

N = N0 * (1/2)^n, where n = t / T(1/2) is the number of half-lives passed. So after 1 half-life half is left, after 2 half-lives one-fourth is left, after 3 half-lives one-eighth is left. Activity falls the same way: R = R0 * (1/2)^n. This avoids the exponential and saves time in the exam.

How do I calculate energy released in fission and fusion (Q-value)?

Q-value = (mass of reactants - mass of products) * c^2 = delta-m (in u) * 931.5 MeV. If Q is positive, energy is released. Fission of one U-235 nucleus gives about 200 MeV. Fusion of light nuclei (like hydrogen to helium) gives energy because the products have higher binding energy per nucleon, so mass is lost and released as energy.

⚠️ The NEET trap
Using T(1/2) = 1 / lambda for half-life (confusing it with mean life).
Half-life is T(1/2) = 0.693 / lambda. Mean life is tau = 1 / lambda. The 0.693 factor (ln 2) must be there for half-life.
🧠 Half-life has the 0.693; mean life does not. If you forget the 0.693, you get mean life by mistake and lose the mark.
Next concept: What Is a Nucleus? Protons and Neutrons ExplainedKeep learning — 2 minFeeling ready? Solve the nuclei NEET PYQs ›Or practice on your phone — get the free MedicNEET app ›

Frequently asked

How many formulas are there in the Nuclei chapter for NEET?

About 10 core formulas: nuclear radius, nuclear density (constant), mass defect, binding energy, binding energy per nucleon, mass-energy relation E = mc^2, decay law, half-life, mean life, activity, and Q-value for fission and fusion. Grouping them as SIZE, MASS, DECAY makes them easy to recall.

What is the value of 1 atomic mass unit in energy?

1 u = 931.5 MeV. This is the most used conversion in the chapter. Whenever you find a mass defect in u, just multiply by 931.5 to get the energy in MeV directly.

Is the nuclear density the same for all nuclei?

Yes. Nuclear density is nearly constant, about 2.3 x 10^17 kg/m^3, and does not depend on the mass number A. This is because both mass and volume increase in proportion to A, so their ratio stays fixed.

Which formula do I use for energy released in fission or fusion?

Q = delta-m * 931.5 MeV, where delta-m is the mass lost (mass of reactants minus mass of products, in u). Fission of one U-235 nucleus releases about 200 MeV; fusion of light nuclei also releases energy because binding energy per nucleon rises.

What is the quick formula for how much sample remains after some time?

N = N0 * (1/2)^n, where n = t / T(1/2) is the number of half-lives that have passed. The same (1/2)^n factor also applies to activity, so you rarely need the full exponential in NEET numericals.