INI CET /Physics

Atoms & nuclei

Optics & Modern Physics · free study notes · Updated

Atoms & Nuclei – Physics Study Notes

(For the INI CET exam – Physics section)


1. Simple Explanation

  • Atoms are the basic units of matter.
  • An atom consists of a nucleus (protons + neutrons) surrounded by electrons.
  • The nucleus is the heavy, positively charged core.
  • Nuclear properties (mass, stability, reactions) are governed by the strong nuclear force, not by the electromagnetic force that keeps electrons in orbit.

2. Key Points

Concept What It Means Why It Matters
Atomic Number (Z) Number of protons Determines element identity
Mass Number (A) Total number of protons + neutrons Gives atomic mass
Neutrons (N) (N = A - Z) Influence stability, isotope variations
Binding Energy (BE) Energy that holds nucleus together Determines nuclear stability
Binding Energy per Nucleon (BE/A) Peak at Fe‑56; explains why light nuclei fission and heavy nuclei fuse
Radioactive Decay Spontaneous change of nucleus Types: α, β, γ, spontaneous fission
Decay Constants & Half‑Life (\lambda) and (t_{1/2}) Predict activity over time
Nuclear Reactions Fusion (light → heavy), Fission (heavy → light), Capture Power generation, medical isotopes
Conservation Laws Energy, mass‑energy, charge, baryon number Guide reaction equations

3. Worked Example

Problem

A nucleus of (^{12}!C) (6 p, 6 n) has a mass of 12.0000 u. The mass of a proton is 1.00728 u and a neutron is 1.00866 u.
Calculate the binding energy of the (^{12}!C) nucleus and the binding energy per nucleon.

Solution

  1. Compute the mass defect
    [ \begin{aligned} m_{\text{calc}} &= 6,m_p + 6,m_n \ &= 6(1.00728) + 6(1.00866) \ &= 6.04368 + 6.05196 = 12.09564\ \text{u} \end{aligned} ]

    [ \Delta m = m_{\text{calc}} - m_{\text{obs}} = 12.09564 - 12.0000 = 0.09564\ \text{u} ]

  2. Convert mass defect to energy
    (1\ \text{u} = 931.5\ \text{MeV})

    [ BE = \Delta m \times 931.5 = 0.09564 \times 931.5 \approx 89.2\ \text{MeV} ]

  3. Binding energy per nucleon

    [ \frac{BE}{A} = \frac{89.2}{12} \approx 7.43\ \text{MeV/nucleon} ]

Answer

  • Binding Energy: ≈ 89 MeV
  • Binding Energy per Nucleon: ≈ 7.4 MeV/nucleon

(Typical value for (^{12}!C) is 7.68 MeV/nucleon; the difference is due to rounding.)


4. Quick Revision Summary

  • Atomic structure: nucleus (Z protons, N neutrons) + electrons.
  • Mass number (A = Z + N).
  • Binding energy is the energy released when a nucleus forms from individual nucleons.
  • Binding energy per nucleon peaks at Fe‑56 (~8.8 MeV).
  • Radioactive decay types:
    • α‑decay: emits (^{4}!He).
    • β‑decay: (n \rightarrow p + e^- + \bar\nu_e) (β⁻) or (p \rightarrow n + e^+ + \nu_e) (β⁺).
    • γ‑decay: emits high‑energy photons.
  • Half‑life (t_{1/2} = \frac{\ln 2}{\lambda}).
  • Fusion (light → heavy) releases energy if (A) is < 56.
  • Fission (heavy → light) releases energy if (A) is > 56.
  • Conservation laws (energy, charge, baryon number) must hold in every nuclear reaction.

Use these points as a quick cheat‑sheet before the exam. Good luck!

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