Physic Labs

Frontier physics

Radioactivity and decay modes

Watch an ensemble of unstable nuclei decay and verify the exponential law N(t)=N0e−λtN(t)=N_0e^{-\lambda t} with half-life T1/2=ln⁡2/λT_{1/2}=\ln2/\lambda, while observing how random individual decays build the smooth average.

High school

⚠ Ionizing radiation is invisible and cumulative; real sources are handled only with shielding, distance, time limits and dosimeter badges in licensed labs.

Equipment

  • 3D population model of parent nuclei with decay events
  • Sliders “Tham số” and “Tham số vật lý” (decay-rate parameters)
  • Slider “Độ nhiễu” (noise level) for statistical fluctuations
  • “Chạy thời gian” (run time) control

Procedure

  1. Measure the half-life

    Start the time evolution with default parameters and let the parent-nucleus count run down. Note the time at which N crosses N0/2N_0/2, then N0/4N_0/4: equal ratios take equal times — the defining property of N(t)=N0e−λtN(t)=N_0e^{-\lambda t}.

  2. Extract λ and the activity

    From your measured T1/2T_{1/2} compute λ=ln⁡2/T1/2\lambda=\ln2/T_{1/2} and the activity A=λNA=\lambda N at two instants. Check that A falls by the same factor as N — activity is proportional to the surviving population.

  3. Explore the randomness

    Raise the noise slider and rerun: individual decays become visibly irregular around the mean curve. Then change the decay-rate parameter and predict the new half-life before measuring — a larger λ means faster decay, T1/2=ln⁡2/λT_{1/2}=\ln2/\lambda.

Simulation

Experiment history

Henri Becquerel discovered radioactivity in 1896 when uranium salts fogged photographic plates in a dark drawer — no phosphorescence required. Marie and Pierre Curie isolated polonium and radium by 1898, showing some elements transform themselves; Marie coined the term “radioactivity.” Ernest Rutherford and Frederick Soddy explained the phenomenon around 1902–03 as transmutation of elements with a statistical decay law, and Rutherford separated α, β and later γ radiation. The exponential law with constant half-life became the clock of nuclear physics — dating rocks, calibrating medical doses, and powering deep-space probes.

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