Fluorescence: Emission of Light at a Longer Wavelength

Fluorescence is the phenomenon in which a substance absorbs light or other electromagnetic radiation and then re-emits it almost immediately at a longer (lower energy) wavelength.

How It Works:

  1. Absorption: A molecule absorbs a high-energy photon (often ultraviolet light), exciting one of its electrons to a higher energy state.
  2. Relaxation: The excited electron quickly loses some energy through non-radiative processes (like vibrations).
  3. Emission: The electron then drops back to a lower energy state, releasing a photon of lower energy (longer wavelength) than the one absorbed.

Key Features:

  • The time between absorption and emission is usually very short — on the order of nanoseconds.
  • The emitted light is always lower in energy (red-shifted) due to the energy lost during the relaxation phase.
  • This shift is known as the Stokes shift.

Applications:

  • Biological imaging: Fluorescent dyes and proteins are used to tag cells and molecules.
  • Security: Fluorescent inks are used in banknotes and documents.
  • Mineralogy: Some minerals fluoresce under UV light, aiding identification.
  • Forensics: Detection of bodily fluids or residues.

Fluorescence is a powerful tool in science and technology, offering insight at microscopic levels and enabling various practical applications through its distinctive glowing property.

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