De-excitation: Electrons in higher energy levels are often unstable and will eventually drop back down to a lower, more stable energy level.
Photon Release: As the electron moves to a lower level, the excess energy is released in the form of an EM wave (a photon).
Spectral Signature: Because energy levels are unique to each element, the frequencies emitted create a unique 'fingerprint' or line spectrum for that atom.
Ionization: If the incoming EM wave has a very high frequency (such as Ultraviolet, X-rays, or Gamma rays), it may provide enough energy to remove an electron from the atom entirely.
Nuclear Transitions: While most interactions involve electrons, extremely high-energy Gamma rays interact directly with the nucleus, causing it to change energy states.
Hazardous Effects: Ionizing radiation can damage biological tissues by breaking chemical bonds and causing mutations in DNA.
| Feature | Absorption | Emission |
|---|---|---|
| Electron Movement | Moves to a higher shell | Moves to a lower shell |
| Energy Flow | Energy is taken from the wave | Energy is released as a wave |
| Wave Frequency | Must match the energy gap | Determined by the energy gap |
Proportionality: Always remember that energy is directly proportional to frequency (). If an exam question mentions 'high energy,' look for 'high frequency' or 'short wavelength.'
Transition Direction: In diagrams, an arrow pointing away from the nucleus indicates absorption (energy gain), while an arrow pointing toward the nucleus indicates emission (energy loss).
Conservation of Energy: The energy of the emitted or absorbed photon is exactly equal to the difference between the two energy levels: .