In photophysics, Quantum Yield (Φ) and Fluorescence Lifetime (τ) are foundational parameters. They reveal both the efficiency of light emission and the dynamics of the excited state—crucial for fluorophores, quantum dots, sensors, and photovoltaics.
1. Quantum Yield (Φ)
Φ is the fraction of absorbed photons that are re-emitted as fluorescence:
Φ = 0.80 means 80% of absorbed photons produce fluorescence; the rest are lost to non-radiative processes (heat, vibrations, etc.).
Relative Method (Common Lab Practice)
(I = integrated fluorescence intensity, A = absorbance at excitation wavelength, n = refractive index. Use optical density correction 1–10–A for accuracy if OD > ~0.05.)
2. Fluorescence Lifetime (τ)
τ is the average time a molecule remains in the excited state before decaying to the ground state — typically 0.5–10 ns for organic fluorophores.
3. Connecting the Dots: Decay Rates
Two main pathways compete:
- Radiative decay (fluorescence): rate constant kr
- Non-radiative decay: rate constant knr (internal conversion, intersystem crossing, quenching, etc.)
Combining these yields the most powerful relationship:
Interactive Calculator: kr & knr from Φ and τ
Calculate Radiative & Non-Radiative Rates
Summary Table
| Metric | Symbol | Definition | Typical Units / Range |
|---|---|---|---|
| Quantum Yield | Φ | Photons emitted / absorbed | 0 – 1 |
| Lifetime | τ | Average excited-state duration | nanoseconds (ns) |
| Radiative Rate | kr | Rate of photon emission | 10⁷ – 10⁹ s⁻¹ (often 10–1000 × 10⁶ s⁻¹) |
| Non-Radiative Rate | knr | Rate of non-emissive decay | s⁻¹ (varies widely) |
Got your own Φ and τ data? Paste values or ask for interpretation — happy to help derive quenching mechanisms or compare to literature!



