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Edexcel IAL·Physics·IAL Physics

Nuclear & Astrophysics

15 min read

Radioactive decay, half-life, nuclear equations, fission and fusion, and key ideas in astrophysics and cosmology.

Radioactivity

Unstable nuclei emit radiation:

  • Alpha (α): a helium nucleus; highly ionising, stopped by paper.
  • Beta (β⁻): a fast electron (a neutron → proton); stopped by aluminium.
  • Gamma (γ): an EM wave; very penetrating, reduced by lead.

Decay is random and spontaneous. Activity A=λNA = \lambda NA=λN, and: N=N0e−λt,t1/2=ln⁡2λN = N_0 e^{-\lambda t}, \quad t_{1/2} = \frac{\ln 2}{\lambda}N=N0​e−λt,t1/2​=λln2​ The half-life is the time for half the nuclei (or activity) to remain.

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