Nuclei

Physics · Class 12

Lesson 11 of 11 · 12 min

Chapter review

Watch a class

The whole chapter on YouTube

Arvind AcademyWhole chapter · Hinglish

Mass defect and binding energy, full chapter

Next Toppers - 12th ScienceWhole chapter · Hinglish

Whole chapter revision for boards

Loading the full lesson

Must-know facts

16 facts

  1. 011 u = 1/12 of the mass of a ¹²C atom = 1.660539 × 10⁻²⁷ kg; its energy equivalent is 931.5 MeV.
  2. 02Chlorine: isotopes 34.98 u (75.4%) and 36.98 u (24.6%), average 35.47 u.
  3. 03mp = 1.00727 u = 1.67262 × 10⁻²⁷ kg; mn = 1.00866 u = 1.6749 × 10⁻²⁷ kg; me = 0.00055 u.
  4. 04Chadwick found the neutron in 1932 (Nobel Prize 1935); a free neutron decays with a mean life of about 1000 s.
  5. 05Z protons, N neutrons, A = Z + N nucleons; ¹⁹⁷₇₉Au has 79 protons and 118 neutrons.
  6. 06Isotopes: same Z. Isobars: same A (³₁H, ³₂He). Isotones: same N (¹⁹⁸₈₀Hg, ¹⁹⁷₇₉Au).
  7. 07R = R₀A^(1/3), R₀ = 1.2 fm, so volume ∝ A and nuclear density is the same for all nuclei, about 2.3 × 10¹⁷ kg m⁻³.
  8. 08E = mc²: 1 g of matter is equivalent to 9 × 10¹³ J.
  9. 09Mass defect ΔM = [Zmp + (A − Z)mn] − M; binding energy Eb = ΔMc².
  10. 10¹⁶O: ΔM = 0.13691 u, Eb = 127.5 MeV.
  11. 11Ebn is nearly constant (about 8 MeV) for 30 < A < 170, peaks at about 8.75 MeV at A = 56 and is 7.6 MeV at A = 238.
  12. 12Nuclear force: attractive, much stronger than the Coulomb force, short-ranged (a few fm), repulsive below about 0.8 fm, charge-independent.
  13. 13Becquerel discovered radioactivity in 1896; the decays are α (⁴₂He), β (electrons or positrons) and γ (photons).
  14. 14Fission of ²³⁵U by a neutron releases about 200 MeV per nucleus; 1 kg of uranium gives about 10¹⁴ J against 10⁷ J from 1 kg of coal.
  15. 15Two protons face a Coulomb barrier of about 400 keV; the sun's core is at 1.5 × 10⁷ K.
  16. 16Proton–proton cycle: four hydrogen atoms make one helium atom and release 26.7 MeV.

Common traps

Where marks are lost

Formulas

8 to know

Atomic mass unit

1 u = (mass of ¹²C atom)/12 = 1.660539 × 10⁻²⁷ kg

Energy equivalent 931.5 MeV.

Mass number

A = Z + N

Z protons, N neutrons.

Nuclear radius

R = R₀A^(1/3)

R₀ = 1.2 fm = 1.2 × 10⁻¹⁵ m.

Mass–energy equivalence

E = mc²

c ≈ 3 × 10⁸ m s⁻¹.

Mass defect

ΔM = [Zmp + (A − Z)mn] − M

M is the mass of the nucleus.

Binding energy

Eb = ΔMc²

1 u × c² = 931.5 MeV.

Binding energy per nucleon

Ebn = Eb/A

About 8 MeV for 30 < A < 170.

Q-value

Q = (sum of initial masses − sum of final masses)c²

Positive Q: energy released.

Key terms

13 terms

Atomic mass unit
One-twelfth of the mass of a carbon-12 atom, 1.660539 × 10⁻²⁷ kg.
Isotopes
Nuclides of one element: same Z, different N and A.
Isobars
Nuclides with the same mass number A.
Isotones
Nuclides with the same neutron number N but different Z.
Nucleon
A proton or a neutron.
Nuclide
A nuclear species, written ᴬ_ZX.
Mass defect
How much less a nucleus weighs than its separate protons and neutrons.
Binding energy
Energy needed to pull a nucleus fully apart into free nucleons, Eb = ΔMc².
Saturation
A nucleon interacts only with its close neighbours, so Ebn stays nearly constant.
Fission
A heavy nucleus splitting into two intermediate-mass fragments.
Fusion
Light nuclei joining into a heavier, more tightly bound nucleus.
Coulomb barrier
The electric repulsion two nuclei must overcome to come within reach of the nuclear force.
Thermonuclear fusion
Fusion driven by raising the temperature so that nuclei move fast enough to overcome the barrier.
Question bankTest yourself: 10 questionsExam-style questions on Nuclei, with full solutions.Start
Nuclei Revision Notes | Class 12 Physics NCERT