Fluorescence is a type of luminescence, meaning light emission that does not come from heat. Instead, it comes from how molecules interact with light at the electronic level.
Historically:
Molecules contain electrons in molecular orbitals, arranged by energy:
Key terms:
Electrons always fill the lowest energy orbitals first.
Light is electromagnetic radiation, often written as:
E = h u
Where:
If light has exactly the right energy, it can:
This creates an excited electronic state.
An excited molecule is unstable and must relax back to equilibrium.
Two possible outcomes:
Only molecules where light emission competes successfully with heat loss are fluorescent molecules.


Observations:
β οΈ This raises a puzzle:
If absorbed and emitted light involve the same electron transition, why are the wavelengths different?
The difference between:
is called the Stokes shift.
Since energy must be conserved, this means some energy is lost before emission β but where?
Key features:
This cannot be explained by electronic states alone.

A Jablonski diagram (named after a Polish physicist) shows:
β οΈ Energy increases upwards, even if the axis is not drawn.
Important insight:
So:
This creates vibrational excitation.
Key consequences:
Relaxation happens in this order:
β‘οΈ Result:
βοΈ This explains the Stokes shift
This creates:
Some molecules lose energy by:
Shown in diagrams as wavy arrows.
Fluorescence depends on competition between rates:
Rules of thumb:
β Fluorescence is quantum-mechanical β Light excites electrons (HOMO β LUMO) β Vibrational relaxation causes energy loss β Emitted light has lower energy (Stokes shift) β Fluorescence depends on relative rate constants