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Radioactive Decay, Half-Life (t½

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### Nuclear Physics: Radioactive Decay Kinetics & Half-Life Radioactive decay is a fundamental quantum mechanical Poisson process where unstable atomic nuclei spontaneously transform by emitting.

Reviewed by Sagar Sageer · Associate Engineer
Last updated:
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⚙ Input Values

📊 Results

Residual Amount & Half-Lives Elapsed Summary
Remaining: 25.000 (25.00% of N₀) ➔ Half-Lives: 2.00 | Decayed: 75.000 (75.00%) | Isotope: Iodine-131
Remaining Residual Quantity (N(t) = N₀·(½)^(t/t½))
25.0000 (25.00% of Initial)
Percentage Remaining vs Decayed (%)
25.00% Left | 75.00% Decayed
Number of Half-Lives Elapsed (n = t / t½)
2.000 Half-Lives Elapsed (t/t½)
Decay Constant (λ = ln(2)/t½ in s⁻¹)
λ = 1.0003e-6 s⁻¹
Mean Radioactive Lifetime (τ = 1/λ = 1.443·t½)
τ = 11.57 Days (1/λ)
✦ Nuclear Physics & Exponential Decay Diagnostic
Radioactive Decay & Half-Life Kinetics (Iodine-131 [t½ = 8.02 days] | N₀ = 100, Elapsed = 16.04 days): [1. Residual Quantity]: After 16.04 days (**2.000 half-lives**), initial amount N₀ = 100 decays to **N(t) = 25.0000 (25.00% remaining)**. [2. Decayed Disintegrations]: A total of **ΔN = 75.0000 (75.00%)** has decayed into stable daughter products. [3. Fundamental Nuclear Constants]: **Decay Constant λ = 1.0003e-6 s⁻¹** | **Mean Atomic Lifetime τ = 11.57 Days** (1.443 × t½). [4. Nuclear Rule of Thumb]: After 7 half-lives, less than 1% (0.78%) remains; after 10 half-lives, less than 0.1% (0.098%) remains.
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📐 Formula

Radioactive Decay Law (Ernest Rutherford, 1902) equations:
N(t) = N_0 × ((1 ÷ 2))^(t ÷ t_1/2) = N_0 × e^- t
Decay Constant: = ( (2) ÷ t_1/2) ≈ (0.69315 ÷ t_1/2)
Elapsed Half-Lives: n = (t ÷ t_1/2)
Decayed Fraction: Δ N = N_0 - N(t)
Mean Atomic Lifetime: = (1 ÷ ) = t_1/2 (2) ≈ 1.4427 × t_1/2

💡 Practical Example

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For example, evaluating a sample of Iodine-131) with initial radioactivity \ after \: Exactly \ have passed. Residual activity is \(N(t) = 100 \times (0.5)^2 = \mathbf{25.00\text{ MBq}}\) (\(25.00\%\) remaining, \(75.00\%\) decayed). The decay constant is \, with a mean atomic lifetime \.

📖 About Radioactive Decay, Half-Life (t½

Nuclear Physics: Radioactive Decay Kinetics & Half-Life

Radioactive decay is a fundamental quantum mechanical Poisson process where unstable atomic nuclei spontaneously transform by emitting ionizing radiation (alpha particles, beta particles, or gamma rays):

  • First-Order Exponential Decay: The decay rate) is strictly proportional to the number of radioactive atoms present.
  • Half-Life): The time required for exactly one-half of the parent nuclei to undergo radioactive transmutation into daughter nuclei. Half-life is invariant—completely unaffected by temperature, pressure, gravity, or chemical bonding.
  • The 10-Half-Life Decommissioning Rule: In nuclear medicine, hazardous radiation waste is typically safely disposed of after 10 half-lives), when residual activity has dropped below 0.1% of its original baseline.

How to Use This Calculator

Enter your Radionuclide / Isotope Preset — choose from Iodine-131 (t½ = 8.02 Days — Thyroid Radiotherapy), Technetium-99m (t½ = 6.01 Hours — Medical SPECT Imaging), Carbon-14 (t½ = 5,730 Years — Radiocarbon Dating), Initial Amount / Activity (N₀ in grams, MBq, or mCi) (e.g. 100), Elapsed Decay Time (Duration t) (e.g. 16.04), Elapsed Time Unit — choose from Hours, Days, Years, Custom Half-Life (t½ [if custom]) (e.g. 8.02), and Custom Half-Life Unit (if custom) — choose from Hours, Days, Years. Results update instantly as you type — adjust any value to compare scenarios.

The Formula

Radioactive Decay Law (Ernest Rutherford, 1902) equations:

N(t) = N_0 · ((1) / (2))^(t) / (t_1/2) = N_0 · e^-λ t

Decay Constant: λ = ((2)) / (t_1/2) ≈ (0.69315) / (t_1/2)

Elapsed Half-Lives: n = (t) / (t_1/2)

Decayed Fraction: Δ N = N_0 - N(t)

Mean Atomic Lifetime: τ = (1) / (λ) = t_1/2(2) ≈ 1.4427 · t_1/2

Worked Example

For example, evaluating a sample of Iodine-131) with initial radioactivity \ after Exactly \ have passed. Residual activity is N(t) = 100 × (0.5)^2 = 25.00 MBq (25.00\% remaining, 75.00\% decayed). The decay constant is with a mean atomic lifetime .

Understanding Your Result

Evaluate your result in the context of your specific use case and relevant industry standards or reference values. A single calculated result is a starting point — test two to three scenarios to understand how sensitive the outcome is to your key input assumptions. For high-stakes decisions, verify your result against a secondary source or subject-matter expert before acting.

💡 Methodological Standards & Calculation Accuracy

  • All calculations are performed client-side in your browser using verified, standards-compliant mathematical algorithms.
  • Results are provided for educational and informational analysis; verify critical applications with certified domain specialists.
  • Ensure input values are entered in consistent units matching the selector options to guarantee accurate outputs.
  • Periodic recalibration is recommended whenever baseline assumptions, operating parameters, or external conditions change.

Results are for informational and educational purposes only. Always verify critical decisions with a qualified professional.

❓ Frequently Asked Questions

What is the formula for radioactive half-life?

The remaining quantity is: N(t) = N0 × (0.5)^ = N0 × e^(-λt), where N0 is initial quantity, t is elapsed time, and t½ is half-life.

What is the decay constant (λ)?

The decay constant / t½ ≈ 0.69315 / t½) represents the probability per unit time that a single radioactive atom will undergo decay.

How much radioactive material remains after 3 half-lives?

After 3 half-lives,³ = 1/8 = 12.5% of the original radioactive substance remains (87.5% has decayed).

What is the difference between half-life (t½) and mean lifetime (τ)?

Half-life is the time for 50% of the sample to decay. Mean lifetime is the average lifespan of an individual radioactive nucleus before decaying.

Can chemical reactions or heat alter an isotope's half-life?

No. Radioactive decay is a fundamental nuclear process governed by the weak and strong nuclear forces, completely unaffected by external heat, pressure, or chemical bonds.

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